Master Projects

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The following Master thesis research projects are offered at Nikhef. If you are interested in one of these projects, please contact the coordinator listed with the project.  
 
The following Master thesis research projects are offered at Nikhef. If you are interested in one of these projects, please contact the coordinator listed with the project.  
  
== Projects with September 2019 start ==
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== Projects with September 2020 start ==
  
=== Theory: The Effective Field Theory Pathway to New Physics at the LHC ===
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=== ATLAS: Top Spin optimal observables using Artificial Intelligence ===
  
A very promising framework to parametrise in a robust and model-independent way deviations from the Standard Model (SM) induced by new heavy particles is the Standard  Model Effective Field Theory (SMEFT). In this formalism, Beyond the SM effects are encapsulated in higher-dimensional operators constructed from SM fields respecting their symmetry properties. In this project, we aim to carry out a global analysis of the SMEFT from high-precision LHC data, including Higgs boson production, flavour observables, and low-energy measurements. This analysis will be carried out in the context of the recently developed SMEFiT approach [1] based on Machine Learning techniques to efficiently explore the complex theory parameter space. The ultimate goal is either to uncover glimpses of new particles or interactions at the LHC, or to derive the most stringent model-independent bounds to date on general theories of New Physics.
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The top quark has an exceptional high mass, close to the electroweak symmetry breaking scale and therefore sensitive to new physics effects. Theoretically, new physics is well described in the EFT framework [1]. The (EFT) operators are experimentally well accessible in single top t-channel production where the top quark is produced spin polarized. The focus at Nikhef is the operator O_{tW} with a possible imaginary phase, leading to CP violation. Experimentally, many angular distribution are reconstructed in the top rest frame to hunt for these effects. We are looking for a limited set of optimal observables. The objective of your Master project would be to find optimal observables using simulated events including the detector effects and possible systematic deviations. All techniques are allowed, but promising new developments are methods which involve artifical intelligence. This work could lead to an ATLAS note.  
  
''Contact: [mailto:j.rojo@vu.nl Juan Rojo]"
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[1] https://arxiv.org/abs/1807.03576
  
[1] https://arxiv.org/abs/1901.05965
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''Contact: Marcel Vreeswijk [mailto:h73@nikhef.nl] and Jordy Degens [mailto:jdegens@nikhef.nl]  ''
  
=== Theory: Pinning down the initial state of heavy-ion collisions with Machine Learning ===
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=== ATLAS: The Next Generation ===
  
It has been known for more than three decades that the parton distribution functions (PDFs) of nucleons bound within heavy nuclei are modified with respect to their free-nucleon counterparts. Despite active experimental and theoretical investigations, the underlying mechanisms that drive these in-medium modifications of nucleon substructure have yet to be fully understood.  The determination of nuclear PDFs is a topic of high relevance in order both to improve our fundamental understanding of the strong interactions in the nuclear environment, as well as and for the interpretation of heavy ion collisions at RHIC and the LHC, in particular for the characterization of the Quark-Gluon Plasma. The goal of this project is to exploit Machine Learning and Artificial Intelligence tools [1,2] (neural networks trained by stochastic gradient descent) to pin down the initial state of heavy ion collisions  by using recent measurements from proton-lead collisions at the LHC. Emphasis will be put on the poorly-known nuclear modifications of the gluon PDFs, which are still mostly ''terra incognita'' and highly relevant for phenomenological applications. In addition to theory calculations, the project will also involve code development using modern AI/ML tools such as TensorFlow and Keras.
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After the observation of the coupling of Higgs bosons to fermions of the third generation, the search for the coupling to fermions of the second generation is one of the next priorities for research at CERN's Large Hadron Collider. The search for the decay of the Higgs boson to two charm quarks is very new [1] and we see various opportunities for interesting developments. For this project we propose improvements in reconstruction (using exclusive decays), advanced analysis techiques (using deep learning methods) and expanding the theory interpretation. Another opportunity would be the development of the first statistical combination of results between the ATLAS and CMS experiment, which could significantly improve the discovery potentional.
  
[1] https://arxiv.org/abs/1811.05858
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[1] https://arxiv.org/abs/1802.04329
[2] https://arxiv.org/abs/1410.8849
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''Contact: [mailto:j.rojo@vu.nl Juan Rojo]"
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''Contact: [mailto:tdupree@nikhef.nl Tristan du Pree and Marko Stamenkovic]''
  
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=== ATLAS: The Most Energetic Higgs Boson ===
  
=== Dark Matter: XENON1T Data Analysis ===
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The production of Higgs bosons at the highest energies could give the first indications for deviations from the standard model of particle physics, but production energies above 500 GeV have not been observed yet [1]. The LHC Run-2 dataset, collected during the last 4 years, might be the first opportunity to observe such processes, and we have various ideas for new studies. Possible developments include the improvement of boosted reconstruction techniques, for example using multivariate deep learning methods. Also, there are various opportunities for unexplored theory interpretations (using the MadGraph event generator), including effective field theory models (with novel ‘morphing’ techniques) and new interpretations of the newly observed boosted VZ(bb) process.
The XENON collaboration has used the XENON1T detector to achieve the world’s most sensitive direct detection dark matter results and is currently building the XENONnT successor experiment. The detectors operate at the Gran Sasso underground laboratory and consist of so-called dual-phase xenon time-projection chambers filled with ultra-pure xenon. Our group has an opening for a motivated MSc student to do analysis with the data from the XENON1T detector. The work will consist of understanding the detector signals and applying machine learning tools such as deep neutral networks to improve the reconstruction performance in our Python-based analysis tool, following the approach described in arXiv:1804.09641. The final goal is to improve the energy and position reconstruction uncertainties for the dark matter search. There will also be opportunity to do data-taking shifts at the Gran Sasso underground laboratory in Italy.  
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:z37@nikhef.nl Auke Colijn]''
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[1] https://arxiv.org/abs/1709.05543
  
=== Dark Matter: XAMS  R&D Setup ===
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''Contact: [mailto:tdupree@nikhef.nl Tristan du Pree and Brian Moser]''
The Amsterdam Dark Matter group operates an R&D xenon detector at Nikhef. The detector is a dual-phase xenon time-projection chamber and contains about 4kg of ultra-pure liquid xenon. We plan to use this detector for the development of new detection techniques (such as utilizing new photosensors) and to improve the understanding of the response of liquid xenon to various forms of radiation. The results could be directly used in the XENON experiment, the world’s most sensitive direct detection dark matter experiment at the Gran Sasso underground laboratory. We have several interesting projects for this facility. We are looking for someone who is interested in working in a laboratory on high-tech equipment, modifying the detector, taking data and analyzing the data him/herself. You will "own" this experiment.
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:z37@nikhef.nl Auke Colijn]''
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=== LHCb: Measurement of delta md  ===
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The decay B0->D-pi+ is very abundant in LHCb, and therefore ideal to study the oscillation frequency
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delta md, with which B0 mesons oscillate into anti-B0 mesons, and vice versa.
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This process proceeds through a so-called box diagram which might hide new yet-undiscovered particles.
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Recently, it has been realized that value of delta md is in tension with the valu of CKM-angle gamma,
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triggering renewed interest in this measurement.
  
=== Dark Matter: DARWIN Sensitivity Studies ===
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''Contact: [mailto:Marcel.Merk@nikhef.nl Marcel Merk]''
DARWIN is the "ultimate" direct detection dark matter experiment, with the goal to reach the so-called "neutrino floor", when neutrinos become a hard-to-reduce background. The large and exquisitely clean xenon mass will allow DARWIN to also be sensitive to other physics signals such as solar neutrinos, double-beta decay from Xe-136, axions and axion-like particles etc. While the experiment will only start in 2025, we are in the midst of optimizing the experiment, which is driven by simulations. We have an opening for a student to work on the GEANT4 Monte Carlo simulations for DARWIN, as part of a simulation team together with the University of Freiburg and Zurich. We are also working on a "fast simulation" that could be included in this framework. It is your opportunity to steer the optimization of a large and unique experiment. This project requires good programming skills (Python and C++) and data analysis/physics interpretation skills.  
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:z37@nikhef.nl Auke Colijn]''
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=== LHCb: Searching for CPT violation ===
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CPT symmetry is closely linked to Lorentz symmetry, and any violation
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would revolutionize science. There are possibilities though that supergravity could
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cause CPT violating effects in the system of neutral mesons.
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The precise study of B0s oscillations in the abundant Bs->Dspi decays can
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give the most stringent limits on Im(z) to date.
  
=== The Modulation Experiment: Data Analysis ===
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''Contact: [mailto:Marcel.Merk@nikhef.nl Marcel Merk]''
There exist a few measurements that suggest an annual modulation in the activity of radioactive sources. With a few groups from the XENON collaboration we have developed four sets of table-top experiments to investigate this effect on a few well known radioactive sources. The experiments are under construction in Purdue University (USA), a mountain top in Switzerland, a beach in Rio de Janeiro and the last one at Nikhef in Amsterdam. We urgently need a master student to (1) analyze the first big data set, and (2) contribute to the first physics paper from the experiment. We are looking for all-round physicists with interest in both lab-work and data-analysis. The student(s) will directly collaborate with the other groups in this small collaboration (around 10 people), and the goal is to have the first physics publication ready by the end of the project. During the 2018-2019 season there are positions for two MSc students.
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''Contact: [mailto:z37@nikhef.nl Auke Colijn]''
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=== LHCb: BR(B0->D-pi+) and fd/fu with B+->D0pi+ ===
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The abundant decay B0->D-pi+ is often used as normalization channel, given its
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clean signal, and well-known branching fraction, as measured by the B-factories.
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However, this branching fraction can be determined more precisely, when comparing
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to the decay B+->D0pi+ , which has a twice better precision.
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In addition, the production of B0 and B+ mesons is often assumed to be equal,
 +
based on isospin symmetry. The study of B+->D0pi+ and B0->D-pi+ allows for the
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first measurement of this ratio, fd/fu.
  
=== ATLAS : Excited lepton searches with multiple leptons ===
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''Contact: [mailto:Marcel.Merk@nikhef.nl Marcel Merk]''
  
The Standard Model of particle physics (SM) is extremely successful, but would it hold against check with data containing multiple leptons? Although very rare process, the production of leptons is calculated in SM with high precision. On detector side the leptons (electrons and muons) are easy to reconstruct and such a sample contains very little "non-lepton" background. This analysis has an ambitious goal to find beyond Standard Model processes like Excited leptons using events with 4 leptons.  With this project, the student would gain close familiarity with modern experimental techniques (statistical analysis, SM predictions, search for rare signals), with Monte Carlo generators and the standard HEP analysis tools (ROOT, C++, python).
 
  
''Contact: [mailto:O.Igonkina@nikhef.nl Olya Igonkina and Marcus Morgenstern and Pepijn Bakker]''
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=== LHCb: Optimization studies for Vertex detector at the High Lumi LHCb ===
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The LHCb experiment is dedicated to measure tiny differences between matter and antimatter through the precise study of rare processes involving b or c quarks. The LHCb detector will undergo a major modification in order to dramatically increase the luminosity and be able to  measure indirect effects of physics beyond the standard model. In this environment, over 42 simultaneous collisions are expected to happen at a time interval of 200 ps where the two proton bunches overlap. The particles of interest have a relatively long lifetime and therefore the best way to distinguish them from the background collisions is through the precise reconstruction of displaced vertices and pointing directions.  The new detector considers using extremely recent or even future technologies to measure space (with resolutions below 10 um) and time (100 ps or better) to efficiently reconstruct the events of interest for physics.  The project involves changing completely  the LHCb Vertex Locator (VELO) design in simulation and determine what can be the best performance for the upgraded detector, considering different spatial and temporal resolutions.
  
=== ATLAS : A search for lepton non-universality in Bc meson decays ===
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''Contact: [mailto:kazu.akiba@nikhef.nl Kazu Akiba]''
  
Recently, LHCb experiment has reported a number of intriguing deviations from SM in leptonic decays of B mesons. With this project we would like to probe if ATLAS also observes the same kind of deviation, e.g. in Bc->Jpsi+tau+nu channel w.r.t BC->Jpsi+mu+nu.  Success of project will be essential to understand if we finally observe beyond SM process or if LHCb has some detector biasThe student would gain close familiarity with modern experimental techniques (statistical analysis, SM predictions, search for rare signals), background suppression techniques and the standard HEP analysis tools (ROOT, C++, python).
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=== LHCb: Measurement of charge multiplication in heavily irradiated sensors ===
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During the R&D phase for the LHCb VELO Upgrade detector a few sensor prototypes were irradiated to the extreme fluence expected to be achieved during the detector lifetime. These samples were tested using high energy particles at the SPS facility at CERN with their trajectories reconstructed by the Timepix3 telescope. A preliminary analysis revealed that at the highest irradiation levels the amount of signal observed is higher than expected, and even larger than the signal obtained at lower doses.   At the Device Under Test (DUT) position inside the telescope, the spatial resolution attained by this system is below 2 um. This means that a detailed analysis can be performed in order to study where and how this signal amplification happens within the 55x55 um^2 pixel cellThis project involves analysing the telescope and DUT data to investigate the charge multiplication mechanism at the microscopic level.
  
''Contact: [mailto:O.Igonkina@nikhef.nl Olya Igonkina and JJ Teoh]''
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''Contact: [mailto:kazu.akiba@nikhef.nl Kazu Akiba]''
  
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=== ALICE: Searching for the strongest magnetic field in nature ===
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In case of a non-central collision between two Pb ions, with a large value of impact parameter (b), the charged nucleons that do not participate in the interaction (called spectators) create strong magnetic fields. A back of the envelope calculation using the Biot-Savart law brings the magnitude of this filed close to 10^19Gauss in agreement with state of the art theoretical calculation, making it the strongest magnetic field in nature. The presence of this field could have direct implications in the motion of final state particles. The magnetic field, however, decays rapidly. The decay rate depends on the electric conductivity of the medium which is experimentally poorly constrained. Overall, the presence of the magnetic field, the main goal of this project, is so far not confirmed experimentally.
  
=== ATLAS : The lifetime of the Higgs boson ===
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''Contact: [mailto:Panos.Christakoglou@nikhef.nl Panos Christakoglou]''
  
While the Higgs boson was discovered in 2012, many of its properties still remain unconstrained. This master student project revolves around one such property, the lifetime of the Higgs boson. The lifetime can be obtained by measuring the width of the boson, but because the width is a few hundred times smaller than the detector resolution, a direct measurement is impossible at the moment. But there is an idea to overcome that limitation. By utilizing the interference between the Higgs boson decay and background processes we can perform an indirect measurement. This measurement potentially has the sensitivity that will allow us to perform a measurement of the width (or lifetime) as predicted by the Standard Model. Specifically, the master project will be about predicting the sensitivity of this measurement for different predictions of the Higgs width. The project is on the interface of theory and experiment, making use of Monte Carlo generators and the standard HEP analysis tools (ROOT, C++, python).  
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=== ALICE: Looking for parity violating effects in strong interactions ===
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Within the Standard Model, symmetries, such as the combination of charge conjugation (C) and parity (P), known as CP-symmetry, are considered to be key principles of particle physics. The violation of the CP-invariance can be accommodated within the Standard Model in the weak and the strong interactions, however it has only been confirmed experimentally in the former. Theory predicts that in heavy-ion collisions, in the presence of a deconfined state, gluonic fields create domains where the parity symmetry is locally violated. This manifests itself in a charge-dependent asymmetry in the production of particles relative to the reaction plane, what is called the Chiral Magnetic Effect (CME).
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The first experimental results from STAR (RHIC) and ALICE (LHC) are consistent with the expectations from the CME, however further studies are needed to constrain background effects. These highly anticipated results have the potential to reveal exiting, new physics.
  
''Contact: [mailto:mveen@nikhef.nl Michiel Veen] or [mailto:Ivo.van.Vulpen@nikhef.nl Hella Snoek & Ivo van Vulpen]''
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''Contact: [mailto:Panos.Christakoglou@nikhef.nl Panos Christakoglou]''
  
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=== ALICE: Machine learning techniques as a tool to study the production of heavy flavour particles ===
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There was recently a shift in the field of heavy-ion physics triggered by experimental results obtained in collisions between small systems (e.g. protons on protons). These results resemble the ones obtained in collisions between heavy ions. This consequently raises the question of whether we create the smallest QGP droplet in collisions between small systems. The main objective of this project will be to study the production of charm particles such as D-mesons and Λc-baryons in pp collisions at the LHC. This will be done with the help of a new and innovative technique which is based on machine learning (ML). The student will also extend the studies to investigate how this production rate depends on the event activity e.g. on how many particles are created after every collision.
  
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''Contact: [mailto:Panos.Christakoglou@nikhef.nl Panos Christakoglou] and [mailto:Alessandro.Grelli@cern.ch Alessandro Grelli]''
  
=== LHCb : Measurement of Central Exclusive Production Rates of Chi_c using converted photons in LHCb ===
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=== ALICE: Energy Loss of Energetic Quarks and Gluons in the Quark-Gluon Plasma ===
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One of the ways to study the quark-gluon plasma that is formed in high-energy nuclear collisions, is using high-energy partons (quarks or gluons) that are produced early in the collision and interact with the quark-gluon plasma as they propagate through it. There are several current open questions related to this topic, which can be explored in a Master's project. For example, we would like to use the new Monte Carlo generator framework JetScape to simulate collisions to see whether we can extract information about the interaction with the quark-gluon plasma. In the project you will collaborate with one of the PhD students or postdocs in our group to use the model to generate predictions of measurements and compare those to data analysis results. Depending on your interests, the project can focus more on the modeling aspects or on the analysis of experimental data from the ALICE detector at the LHC.
  
Central exclusive production (CEP) of particles at the LHC is characterised by a extremely clean signature. Differently from the typical inelastic collisions where many particles are created resulting in a so-called Primary Vertex, CEP events have only the final state particles of interest. In this project the particle of interest is a pair of charmed quarks creating a chi_c particle. In theory this process is generated by a long range gluon exchange and can elucidate the nature of the strong force, described by the quantum chromodynamics in the the standard model. The proposed work involves  analysing a pre-existing dataset with reconstructed chi_c and simulating events at the LHCb in order to obtain the relative occurrence rate of each chi_c species (spins 0, 1, 2), a quantity that can be easily compared to theoretical predictions.
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''Contact: [mailto:marco.van.leeuwen@cern.ch Marco van Leeuwen] and [mailto:marta.verweij@cern.ch Marta Verweij]''
  
"Contact: [mailto:K.Akiba@nikhef.nl Kazu Akiba]"
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=== ALICE: Extreme Rare Probes of the Quark-Gluon Plasma ===
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The quark-gluon plasma is formed in high-energy nuclear collisions and also existed shortly after the big bang.  With the large amount of data collected in recent years at the Large Hadron Collider at CERN, rare processes that previously were not accessible provide now new ways to study how the quark-gluon plasma emerges from the fundamental theory of strong interaction. One of such processes is the heavy W boson which in many cases decays to two quarks. The W boson itself doesn’t interact with the quark-gluon plasma because it doesn’t carry color, but the quark decay products do interact with the plasma and therefore provide an ideal tool to study the space-time evolution of this hot and dense medium. In this project you will use data from the ALICE detector at the LHC and simulated data from generators to study various physics mechanisms that could be happening in the real collisions.
  
=== LHCb : Optimization studies for Vertex detector at the High Lumi LHCb  ===
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''Contact: [mailto:marta.verweij@cern.ch Marta Verweij] and [mailto:marco.van.leeuwen@cern.ch Marco van Leeuwen]''
  
The LHCb experiment is dedicated to measure tiny differences between matter and antimatter through the precise study of rare processes involving b or c quarks.  The LHCb detector will undergo a major modification in order to dramatically increase the luminosity and be able to  measure indirect effects of physics beyond the standard model.  In this environment, over 42 simultaneous collisions are expected to happen at a time interval of 200 ps where the two proton bunches overlap. The particles of interest have a relatively long lifetime and therefore the best way to distinguish them from the background collisions is through the precise reconstruction of displaced vertices and pointing directions.  The new detector considers using extremely recent or even future technologies to measure space (with resolutions below 10 um) and time (100 ps or better) to efficiently reconstruct the events of interest for physics.  The project involves changing completely  the LHCb Vertex Locator (VELO) design in simulation and determine what can be the best performance for the upgraded detector, considering different spatial and temporal resolutions.
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=== ALICE: Jet Quenching with Machine Learning ===
  
"Contact: [mailto:K.Akiba@nikhef.nl Kazu Akiba]"
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Machine learning applications are rising steadily as a vital tool in the field of data science but are relatively new in the particle physics community. In this project machine learning tools will be used to gain insights into the modification of a parton shower in the quark-gluon plasma (QGP). The QGP is created in high-energy nuclear collisions and only lives for a very short period of time. Highly energetic partons created in the same collisions interact with the plasma while they travers it and are observed as a collimated spray of particles, known as jets, in the detector.  One of the key recent insights is that the internal structure of jets provides information about the evolution of the QGP. With data recorded by the ALICE experiment, you will use jet substructure techniques in combination with machine learning algorithms to dissect the structure of the QGP. Machine learning will be used to select the regions of radiation phase space that are affected by the presence of the QGP.
  
=== LHCb : Measurement of charge multiplication in heavily irradiated sensors ===
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''Contact: [mailto:marta.verweij@cern.ch Marta Verweij] and [mailto:marco.van.leeuwen@cern.ch Marco van Leeuwen]''
  
During the R&D phase for the LHCb VELO Upgrade detector a few sensor prototypes were irradiated to the extreme fluence expected to be achieved during the detector lifetime. These samples were tested using high energy particles at the SPS facility at CERN with their trajectories reconstructed by the Timepix3 telescope. A preliminary analysis revealed that at the highest irradiation levels the amount of signal observed is higher than expected, and even larger than the signal obtained at lower doses.   At the Device Under Test (DUT) position inside the telescope, the spatial resolution attained by this system is below 2 um. This means that a detailed analysis can be performed in order to study where and how this signal amplification happens within  the 55x55 um^2 pixel cell.  This project involves analysing the telescope and DUT data to investigate the charge multiplication mechanism at the microscopic level.
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=== Lepton Collider: Pixel TPC testbeam ===
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In the Lepton Collider group at Nikhef we work on a tracking detector for a future Collider (e.g. the ILC in Japan). We are developing a gaseous Time Projection Chamber with a pixel readout. At Nikhef we have built an 8-quad GridPix module based on the Timepix3 chip, which is a detector of about 20 cm x 40 cm x 10 cm in size. In August 2020 we will test the device at the DESY particle accelerator in Hamburg. For the project you could work on preparations for the test beam (e.g. running the data acquisition, perform data monitoring using our set up in the lab). The next topics will be the participation in the data taking during the test beam at DESY, the analysis of the data using C++ and ROOT and - finally - publication of the results in a scientific journal.
  
"Contact: [mailto:K.Akiba@nikhef.nl Kazu Akiba]"
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Our latest paper can be found in https://www.nikhef.nl/~s01/quad_paper.pdf [www.nikhef.nl].
  
=== Detector R&D : Studying fast timing detectors ===
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''Contact: [mailto:Peter.Kluit@nikhef.nl Peter Kluit] and Kees Ligtenberg''
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=== Dark Matter: Sensitive tests of wavelength-shifting properties of materials for dark matter detectors ===
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Rare event search experiments that look for neutrino and dark matter interactions are performed with highly sensitive detector systems, often relying on scintillators, especially liquid noble gases, to detect particle interactions. Detectors consist of structural materials that are assumed to be optically passive, and light detection systems that use reflectors, light detectors, and sometimes, wavelength-shifting materials. MSc theses are available related to measuring the efficiency of light detection systems that might be used in future detectors. Furthermore, measurements to ensure that presumably passive materials do not fluoresce, at the low level relevant to the detectors, can be done. Part of the thesis work can include Monte Carlo simulations and data analysis for current and upcoming dark matter detectors, to study the effect of different levels of desired and nuisance wavelength shifting. In this project, students will acquire skills in photon detection, wavelength shifting technologies, vacuum systems, UV and extreme-UV optics, detector design, and optionally in C++ programming, data analysis, and Monte Carlo techniques.
  
Fast timing detectors are the solution for future tracking detectors. In future LHC operation conditions and future colliders, more and more particles are produced per collision. The high particle densities make it increasingly more difficult to separate particle trajectories with the spatial information that current silicon tracking detectors provide. A solution would be to add very precise (in order of 10ps) timestamps to the spatial measurements of the particle trackers. A good understanding of the performance of fast timing detectors is necessary. With the user of a pulsed laser in the lab we study the characteristics of several prototype detectors.
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''Contact: [mailto:Tina.Pollmann@tum.de Tina Pollmann] and [mailto:decowski@nikhef.nl Patrick Decowski]''
  
"Contact: [mailto:H.Snoek@nikhef.nl Hella Snoek, Martin van Beuzekom, Kazu Akiba, Daniel Hynds]"
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=== Dark Matter: Signal reconstruction in XENONnT ===
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The next generation direct detection dark matter experiment - XENONnT - comprises close to 500 photomultiplier tubes (PMTs) in the main detector volume. These PMTs are configured to be able to detect even single photons. When a single photoelectron (PE) signal is detected the detected signal (a pulse) is convoluted with the detector response of the PMT. Due to this detector response the pulse shape of a single PE is spread out in time. For XENONnT we would like to explore the possibility to implement a digital (software) filter to deconvolve the detected pulse back to the “true” instantaneous shape (without the detector spread). This is a virtually unexplored new step in the Xenon analysis framework. Later in the analysis framework these pulses from all the PMTs are combined into a signal referred to as a ‘peak’. For XENONnT it is of essence to be extremely good in discriminating between two types of peaks caused by interactions in the detector; a prompt primary scintillation signal (S1) and a secondary ionization signal (S2). The parameters in the software haven’t - as of the time of writing - been optimized for the XENONnT-detector conditions.
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The student would investigate how a deconvolution filter would benefit the XENONnT analysis framework and develop such a filter. Furthermore, the student will work on the classification of these signals to fully exploit the XENONnT-detector to optimize the classification. This will be done with simulated data at first but may later even be performed on actual XENONnT-data. As an extension, the possibility of applying machine learning to correctly distinguish between the two signals could be explored. This is a data-analysis oriented project where Python skills are paramount.
  
=== KM3NeT : Reconstruction of first neutrino interactions in KM3NeT ===
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:j.angevaare@nikhef.nl Joran Angevaare]''
  
The neutrino telescope KM3NeT is under construction in the Mediterranean Sea aiming to detect cosmic neutrinos. Its first few strings with sensitive photodetectors have been deployed at both the Italian and the French detector sites. Already these few strings provide for the option to reconstruct in the detector the abundant muons stemming from interactions of cosmic rays with the atmosphere and to identify neutrino interactions. In order to identify neutrinos an accurate reconstruction and optimal understanding of the backgrounds are crucial. In this project we will use the available data to identify and reconstruct the first neutrino interactions in the KM3NeT detector and with this pave the path towards accurate neutrino oscillation measurements and neutrino astronomy.
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=== Dark Matter: XAMS  R&D Setup ===
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The Amsterdam Dark Matter group operates an R&D xenon detector at Nikhef. The detector is a dual-phase xenon time-projection chamber and contains about 4kg of ultra-pure liquid xenon. We use this detector for the development of new detection techniques - such as utilizing our newly installed silicon photomultipliers - and to improve the understanding of the response of liquid xenon to various forms of radiation. The results could be directly used in the XENONnT experiment, the world’s most sensitive direct detection dark matter experiment at the Gran Sasso underground laboratory, or for future Dark Matter experiments like DARWIN. We have several interesting projects for this facility. We are looking for someone who is interested in working in a laboratory on high-tech equipment, modifying the detector, taking data and analyzing the data him/herself. You will "own" this experiment.  
  
Programming skills are essential, mostly root and C++ will be used.
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:z37@nikhef.nl Auke Colijn]''
  
'' Contact: [mailto:bruijn@nikhef.nl Ronald Bruijn] [mailto:dosamtnikhef.nl Dorothea Samtleben]'''
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=== Dark Matter: DARWIN Sensitivity Studies ===
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DARWIN is the "ultimate" direct detection dark matter experiment, with the goal to reach the so-called "neutrino floor", when neutrinos become a hard-to-reduce background. The large and exquisitely clean xenon mass will allow DARWIN to also be sensitive to other physics signals such as solar neutrinos, double-beta decay from Xe-136, axions and axion-like particles etc. While the experiment will only start in 2025, we are in the midst of optimizing the experiment, which is driven by simulations. We have an opening for a student to work on the GEANT4 Monte Carlo simulations for DARWIN, as part of a simulation team together with the University of Freiburg and Zurich. We are also working on a "fast simulation" that could be included in this framework. It is your opportunity to steer the optimization of a large and unique experiment. This project requires good programming skills (Python and C++) and data analysis/physics interpretation skills.  
  
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:z37@nikhef.nl Auke Colijn]''
  
=== KM3NeT : Acoustic detection of ultra-high energy cosmic-ray neutrinos  (2 projects) ===
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=== Dark Matter: Fast simulation studies ===
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For Dark Matter experiments it is crucial to understand sources of backgrounds in great detail. The most common way to study the effect of backgrounds to the Dark Matter sensitivity is by the
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use of Monte Carlo simulations. Unfortunately, the standard Monte Carlo techniques are extremely inefficient. One needs to sometimes simulate millions of events before one background event appears in the Dark Matter search area. We have developed a Monte Carlo technique that accelerates this process by up to 1000x. The method has been validated on very simple and unrealistic detector models. In goal of this project is to make a realistic detector model for the fast detector simulations. For this we are looking for a student with good programming skills, an interest in a software project, and the desire to deeply understand analysis of Dark Matter experimental data. 
  
The study of the cosmic neutrinos of energies above 1017 eV, the so-called ultra-high
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:z37@nikhef.nl Auke Colijn]''
energy neutrinos, provides a unique view on the universe and may provide insight
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in the origin of the most violent astrophysical sources, such as gamma ray bursts,
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supernovae or even dark matter. In addition, the observation of high energy neutrinos
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may provide a unique tool to study interactions at high energies.
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The energy deposition of these extreme neutrinos in water induce a thermo-
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acoustic signal, which can be detected using sensitive hydrophones. The expected
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neutrino flux is however extremely low and the signal that neutrinos induce is small.
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TNO is presently developing sensitive hydrophone technology based on fiber optics.
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Optical fibers form a natural way to create a distributed sensing system. Using this
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technology a large scale neutrino telescope can be built in the deep sea. TNO is aiming
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for a prototype hydrophone which will form the building block of a future telescope.
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The work will be executed at the Nikhef institute and/or the TNO laboratories in Delft. In this project there are two opportunities for master students to participate:<br>
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=== Dark Matter & Amsterdam Scientific Instruments: Simulations for Industry ===
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In the Nikhef Dark Matter group we have built up an extensive expertise with Monte Carlo simulations of ionizing radiation. Although these simulations have the aim to estimate background levels in our XENON experiments, the same techniques can be applied to study radiation transport in industrial devices. Amsterdam Scientific Instruments (ASI) is a company at Science Park that develops and sells radiation imaging equipment that is used amongst others in electron microscopy. For this application ASI needs a detailed study of gamma ray backgrounds to optimize shielding for their products. The project aims at optimizing a shielding design based on GEANT4 simulations. The results may be implemented in next generation products of ASI. We are looking for a student with preferably strong computing skills, and with an interest in science-industrial collaboration.
  
<b>student project 1: </b> Hardware development on fiber optics hydrophones technology<br>
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''Contact: [mailto:decowski@nikhef.nl Patrick Decowski] and [mailto:z37@nikhef.nl Auke Colijn]''
Goal: characterise existing proto-type optical fibre hydrophones in an anechoic basin at TNO laboratory. Data collection, calibration, characterisation, analysis of consequences for design future acoustic hydrophone neutrino telescopes<br>
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Keywords: Optical fiber technology, signal processing, electronics, lab.
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<b>student project 2:</b> Investigation of ultra-high energy neutrinos and their interactions with matter.<br>
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=== The Modulation experiment: Data Analysis  ===
Goal: simulate (currently imperfectly modelled) interaction for extremely high energy interactions, characterise differences with currently available physics models and impact on physics reach for future acoustic hydrophone neutrino telescopes<br>
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For years there have been controversial claims of potential new-physics on the basis of time-varying decay rates of radioactive sources on top of ordinary exponential decay. While some of these claims have been refuted, others have still to be confirmed or falsified. To this end, a dedicated experiment - the modulation experiment - has been designed and operational for the past four years. Using four identical and independent setups the experiment is almost ready for a final analysis to conclude on these claims. In this project the student will perform this analysis, preferably resulting in a conclusive paper. This will require combining the data of the four setups and close collaboration with a small group constituting a collaboration of the four different involved institutes (Purdue University (USA), Universität Zürich (Switzerland), Centro Brasileiro de Pesquisas Fisicas (Brasil) and Nikhef). This project is data-analysis oriented. Additionally, lab-skills can be required as one of the setups is situated at Nikhef.
Keywords: Monte Carlo simulations, particle physics, cosmology. <br>
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''Contact: [mailto:z37@nikhef.nl Auke Colijn] and [mailto:j.angevaare@nikhef.nl Joran Angevaare]''
  
Further information:<br>
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=== Detector R&D: Laser Interferometer Space Antenna (LISA) ===
- Info on ultra-high energy neutrinos can be found at: http://arxiv.org/abs/1102.3591<br>
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The space-based gravitational wave antenna LISA is, without a doubt, one of the most challenging space missions ever proposed. ESA plans to launch around 2030 three spacecraft that are separated by a few million kilometers to measure tiny variations in the distances between test-masses located in each satellite to detect the gravitational waves from sources such as supermassive black holes. The triangular constellation of the LISA mission is dynamic, requiring a constant fine-tuning related to the pointing of the laser links between the spacecraft and a simultaneous refocusing of the telescope. The noise sources related to the laser links expect to provide a dominant contribution to the LISA performance.
- Info on acoustic detection of neutrinos can be found at: http://arxiv.org/abs/1311.7588
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An update and extension of the LISA science simulation software are needed to assess the hardware development for LISA at Nikhef, TNO, and SRON. A position is therefore available for a master student to study the impact of instrumental noise on the performance of LISA. Realistic simulations based on hardware (noise) characterization measurements performed at TNO will be carried out and compared to the expected tantalizing gravitational wave sources.
  
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''Contact: [mailto:nielsvb@nikhef.nl Niels van Bakel],[mailto:ernst-jan.buis@tno.nl  Ernst-Jan Buis]''
  
'' Contact: [mailto:ernst-jan.buis@tno.nl Ernst-Jan Buis] and [mailto:ivo.van.vulpen@nikhef.nl Ivo van Vulpen]'''
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=== Detector R&D: Spectral X-ray imaging - Looking at colours the eyes can't see ===
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When a conventional X-ray image is taken, one acquires an image that only shows intensities. a ‘black and white’ image. Most of the information carried by the photon energy is lost. Lacking spectral information can result in an ambiguity between material composition and amount of material in the sample. If the X-ray intensity as a function of the energy can be measured (i.e. a ‘colour’ X-ray image) more information can be obtained from a sample. This translates to less required dose and/or to a better understanding of the sample that is being investigated. For example, two fields that can benefit from spectral X-ray imaging are mammography and real time CT.
  
== Projects with September 2018 start ==
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Detectors using Medipix3 chips are used for X-ray imaging. Such a detector is composed of a pixel chip with a semiconductor sensor bonded on top of it. Photoelectric absorption of X-rays in the sensor results in an amount of charge being released that is proportional to the X-ray energy. This charge is registered by a pixel. Depending on configuration, in each pixel 1, 2, 4 or 8 detection thresholds can be set and so, a number of energy bins can be defined. One of the challenges is to maximise X-ray image quality by minimising effects caused by dispersion in the sensitivity of the pixels. The effects of this dispersion can partly be compensated by applying a specific measurement method in combination with image post processing.
  
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You can work on improving measurement methods and on improving post processing methods. There is flexibility of the planned work depending on the skillset you have. The aim is to get the best X-ray energy resolution over the entire pixel chip. This in turn improves image quality and therefore X-ray CT reconstruction quality.
  
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Important note: Much of this work is to be performed in the laboratory. For as long as corona safety measures are active, the labs at Nikhef are not accessible for students and this project cannot be worked on except for post-processing in software. Currently we hope that the situation will have improved by August.
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Please see the following videos for examples of our work:
  
=== Theory: Stress-testing the Standard Model at the high-energy frontier ===
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https://youtu.be/cgwQvjfUYns
  
A suitable framework to parametrise in a model-independent way deviations from the SM induced by new heavy particles is the Standard Model Effective Field Theory (SMEFT). In this formalism, bSM effects are encapsulated in higher-dimensional operators constructed from SM fields respecting their symmetry properties. Here we aim to perform a global analysis of the SMEFT from high-precision LHC data. This will be achieved by extending the NNPDF fitting framework to constrain the SMEFT coefficients, with the ultimate aim of identifying possible bSM signals.
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https://youtu.be/tf9ZLALPVNY
  
''Contact: [mailto:j.rojo@vu.nl Juan Rojo]''
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https://youtu.be/vjPX7SxvSUk
  
=== Theory: The quark and gluon internal structure of heavy nuclei in the LHC era  ===
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https://youtu.be/LqjNVSm7Hoo
  
A precise knowledge of the parton distribution functions (PDFs) of the proton is essential in order to make predictions for the Standard Model and beyond at hadron colliders. The presence of nuclear medium and collective phenomena which involve several nucleons modifies the parton distribution functions of nuclei (nPDFs) compared to those of a free nucleon. These modifications have been investigated by different groups using global analyses of high energy nuclear reaction world data. It is important to determine the nPDFs not only for establishing perturbative QCD factorisation in nuclei but also for applications to heavy-ion physics and neutrino physics. In this project the student will join an ongoing effort towards the determination of a data-driven model of nPDFs, and will learn how to construct tailored Artificial Neural Networks (ANNs).  
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''Contact: [mailto:martinfr@nikhef.nl Martin Fransen],[mailto:navritb@nikhef.nl Navrit Bal]''
  
"Further information [[http://pcteserver.mi.infn.it/~nnpdf/VU/2018-MasterProject-nPDFs.pdf here]]
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=== Detector R&D: Holographic projector ===
  
''Contact: [mailto:j.rojo@vu.nl Juan Rojo]''
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A difficulty in projecting holograms (based on the interference of light) is the required dense pixel pitch of a projector. One would need a pixel pitch of less than 200 nanometer. With larger pixels artefacts occur due to spatial under sampling. A pixel pitch of 200 nanometer is difficult, if not, impossible, to achieve, especially for larger areas. Another challenge is the massive amount of computing power that would be required to control such a dense pixel matrix.  
  
=== Theory:  Combined QCD analysis of parton distribution and fragmentation functions ===
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A new holographic projection method has been developed that reduces under sampling artefacts for projectors with a ‘low’ pixel density. It uses 'pixels' at random but known positions, resulting in an array of (coherent) light points that lacks (or has suppressed) spatial periodicity. As a result a holographic projector can be built with a significantly lower pixel density and correspondingly less required computing power. This could bring holography in reach for many applications like display, lithography, 3D printing, metrology, etc...
  
The formation of hadrons from quarks and gluons, or collectively partons, is a fundamental QCD process that has yet to be fully understood. Since parton-to-hadron fragmentation occurs over long-distance scales, such information can only be extracted from experimental observables that identify mesons and baryons in the final state. Recent progress has been made to determine these fragmentation functions (FFs) from charged pion and kaon production in single inclusive e+e−-annihilation (SIA) and additionally pp-collisions and semi-inclusive deep inelastic scattering (SIDIS). However, charged hadron production in unpolarized pp and inelastic lepton-proton scattering also require information about the momentum distributions of the quarks and gluons in the proton, which is encoded in non-perturbative parton distribution functions (PDFs). In this project, a simultaneous treatment of both PDFs and FFs in a global QCD analysis of single inclusive hadron production processes will be made to determine the individual parton-to-hadron FFs. Furthermore, a robust statistical methodology with an artificial neural network learning algorithm will be used to obtain a precise estimation of the FF uncertainties. This work will emphasis in particular the impact of pp-collision and SIDIS data on the gluon and separated quark/anti-quark FFs, respectively.
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Of course, nothing comes for free: With less pixels, holograms become noisier and the contrast will be reduced (not all light ends up in the hologram). The questions: How does the quality of a hologram depend on pixel density? How do we determine projector requirements based on requirements for hologram quality?
  
"Further information [[http://pcteserver.mi.infn.it/~nnpdf/VU/2018-MasterProject-FFpPDFs.pdf here]]
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Requirements for a hologram can be expressed in terms of: Noise, contrast, resolution, suppression of under sampling artefacts, etc..  
  
''Contact: [mailto:j.rojo@vu.nl Juan Rojo]''
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For this project we have built a proof of concept holographic emitter. This set-up will be used to verify simulation results (and also to project some cool holograms of course ;-).  
  
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Examples of what you could be working on:
  
=== ALICE: Charm is in the Quark Gluon Plasma ===
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a. Calibration/characterisation of the current projector and compensation of systematic errors.
The goal of heavy-ion physics is to study the Quark Gluon Plasma (QGP), a hot and dense medium where quarks and gluons move freely over large distances, larger than the typical size of a hadron. Hydrodynamic simulations expect that the QGP will expand under its own pressure, and cool while expanding. These simulations are particularly successful in describing some of the key observables measured experimentally, such as particle spectra and various orders of flow harmonics. Charm quarks are produced very early during the evolution of a heavy-ion collision and can thus serve as an idea probe of the properties of the QGP. The goal of the project is to study higher order flow harmonics (e.g. triangular flow - v3) that are more sensitive to the transport properties of the QGP for charm-mesons, such as D0, D*, Ds. This will be the first ever measurement of this kind.  
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''Contact: [mailto:Panos.Christakoglou@nikhef.nl Panos Christakoglou and Paul Kuijer]''
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b. To realize a phased array of randomly placed light sources the pixel matrix of the projector must be ‘relayed’ onto a mask with apertures at random but precisely known positions. Determine the best possible relaying optics and design an optimized mask accordingly. Factors like deformation of the projected pixel matrix and limitations in resolving power of the lens system must be taken into account for mask design.
  
=== ALICE: Probing the time evolution of particle production in the Quark-Gluon Plasma ===
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Important note: Much of this work is to be performed in the laboratory. For as long as corona safety measures are active, the labs at Nikhef are not accessible for students and this project cannot be worked on. Currently we hope that the situation will have improved by august.  
Particle production is governed by conservation laws, such as local charge conservation. The latter ensures that each charged particle is balanced by an oppositely-charged partner, created at the same location in space and time. The charge-dependent angular correlations, traditionally studied with the balance function, have emerged as a powerful tool to probe the properties of the Quark-Gluon Plasma (QGP) created in high energy collisions. The goal of this project is to take full advantage of the unique, among all LHC experiments, capabilities of the ALICE detector that is able to identify particles to extend the studies to different particle species (e.g. pions, kaons, protons…). These studies are highly anticipated by both the experimental and theoretical communities.
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''Contact: [mailto:Panos.Christakoglou@nikhef.nl Panos Christakoglou]''
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''Contact: [mailto:martinfr@nikhef.nl Martin Fransen]''
  
=== ALICE: CP violating effects in QCD: looking for the chiral magnetic effect with ALICE at the LHC ===
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=== Theory: The Effective Field Theory Pathway to New Physics at the LHC ===
Within the Standard Model, symmetries, such as the combination of charge conjugation (C) and parity (P), known as CP-symmetry, are considered to be key principles of particle physics. The violation of the CP-invariance can be accommodated within the Standard Model in the weak and the strong interactions, however it has only been confirmed experimentally in the former. Theory predicts that in heavy-ion collisions gluonic fields create domains where the parity symmetry is locally violated. This manifests itself in a charge-dependent asymmetry in the production of particles relative to the reaction plane, which is called Chiral Magnetic Effect (CME). The first experimental results from STAR (RHIC) and ALICE (LHC) are consistent with the expectations from the CME, but background effects have not yet been properly disentangled. In this project you will develop and test new observables of the CME, trying to understand and discriminate the background sources that affects such a measurement.  
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A promising framework to parametrise in a robust and model-independent way deviations from the Standard Model (SM) induced by new heavy particles is the Standard Model Effective Field Theory (SMEFT). In this formalism, beyond the SM effects are encapsulated in higher-dimensional operators constructed from SM fields respecting their symmetry properties. In this project, we aim to carry out a global analysis of the SMEFT from high-precision LHC data, including Higgs boson production, flavour observables, and low-energy measurements. This analysis will be carried out in the context of the recently developed SMEFiT approach [1] based on Machine Learning techniques to efficiently explore the complex theory parameter space. The ultimate goal is either to uncover glimpses of new particles or interactions at the LHC, or to derive the most stringent model-independent bounds to date on general theories of New Physics. Of particular interest are novel methods for charting the parameter space [2], the matching to UV-complete theories in explicit BSM scenarios [3], and the interplay between EFT-based model-independent searches for new physics and determinations of the proton structure from LHC data [4].
  
''Contact: [mailto:Panos.Christakoglou@nikhef.nl Panos Christakoglou]''
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[1] https://arxiv.org/abs/1901.05965
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[2] https://arxiv.org/abs/1906.05296
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[3] https://arxiv.org/abs/1908.05588
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[4] https://arxiv.org/abs/1905.05215
  
=== LHCb: Searching for dark matter in exotic six-quark particles ===
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''Contact: [mailto:j.rojo@vu.nl Juan Rojo]''
3/4 of the mass in the Universe is of unknown type. Many hypotheses about this dark matter have been proposed, but none confirmed. Recently it has been proposed that it could be made of particles made of the six quarks uuddss. Such a particle could be produced in decays of heavy baryons. It is proposed to use Xi_b baryons produced at LHCb to search for such a state. The latter would appear as missing 4-momentum in a kinematically constrained decay. The project consists in optimising a selection and applying it to LHCb data. See [https://arxiv.org/abs/1708.08951 arXiv:1708.08951]
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''Contact: [mailto:patrick.koppenburg@cern.ch Patrick Koppenburg]''
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=== Theory: Charting the quark and gluon structure of protons and nuclei with Machine Learning ===
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Deepening our knowledge of the partonic content of nucleons and nuclei [1] represents a central endeavour of modern high-energy and nuclear physics, with ramifications in related disciplines such as astroparticle physics. There are two main scientific drivers motivating these investigations of the partonic structure of hadrons. On the one hand, addressing fundamental open issues in our understanding in the strong interactions such as the origin of the nucleon mass, spin, and transverse structure; the presence of heavy quarks in the nucleon wave function; and the possible onset of novel gluon-dominated dynamical regimes. On the other hand, pinning down with the highest possible precision the substructure of nucleons and nuclei is a central component for theoretical predictions in a wide range of experiments, from proton and heavy ion collisions at the Large Hadron Collider to ultra-high energy neutrino interactions at neutrino telescopes. The goal of this project is to exploit Machine Learning and Artificial Intelligence tools [2,3] (neural networks trained by stochastic gradient descent) to pin down the quark and gluon substructure of protons and nuclei by using recent measurements from proton-proton and proton-lead collisions at the LHC. Topics of special interest are i) the strange content of protons and nuclei, ii) parton distributions at higher-orders in the QCD couplings for precision Higgs physics, iii) the interplay between jet, photon, and top quark production data to pin down the large-x gluon, and iv) charm quarks as a probe of gluon shadowing at small-x. The project also involves developing projects for the Electron-Ion Collider (EIC), a new lepton-nucleus experiment to start operations in the next years.
  
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[1] https://arxiv.org/abs/1910.03408
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[2] https://arxiv.org/abs/1904.00018
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[3] https://arxiv.org/abs/1706.00428
  
=== LHCb: Measurement of BR(B0 → Ds+ Ds-) ===
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''Contact: [mailto:j.rojo@vu.nl Juan Rojo]''
  
This project aims to discover the branching fraction of the decay B0->Ds- Ds+. The decay B0->Ds- Ds+ is quite rare, because it occurs through the exchange of a W-boson between the b and the d-quark of the B0-meson. This decay proceeds via Cabibbo-suppressed W-exchange and has not yet been observed; theoretical calculations predict a branching fraction at the order of 10^-5 with a best experimental upper limit of 3.6x10^-5.
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=== Theory: Machine learning for Electron Microscopy for next-generation materials ===
A measurement of the decay rate of B0 -> Ds+Ds- relative to that of B0 -> D+D- can provide an estimate of the W-exchange contribution to the latter decay, a crucial piece of information for extracting the CKM angle gamma from B0 -> D(*)D(*).
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Machine Learning tools developed and applied for particle physics hold great potential for applications in material science, in particular concerning faithful uncertainty estimation and model training for large parameter spaces. In this project, carried out in collaboration with the group of Dr. Sonia Conesa-Boj from the Kavli Institute Nanoscience Delft, http://www.conesabojlab.tudelft.nl, we will  develop and deploy ML tools for data analysis in Electron Microscopy. We will focus on pinning down the properties of novel quantum materials such as topological insulators and van der Waals materials. Examples of possible applications include model-independent background subtraction in electron-energy loss spectroscopy, automatic classification of crystalline structures, and enhancing spatial and spectral resolution using convolutional networks.
The aim is to determine the relative branching fraction of B0->Ds+Ds- with respect to B0->Ds+D- decays (which has the best known branching ratio at present, (7.2 +- 0.8)x10^-3), in close collaboration with the PhD. The aim is that this project results in a journal publication on behalf of the LHCb collaboration. For this project computer skills are needed. The ROOT programme and C++ and/or Python macros are used. This is a project that is closely related to previous analyses in the group. Weekly video meetings with CERN coordinate the efforts with in the LHCb collaboration.
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Relevant information:
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[1] M.Jung and S.Schacht, "Standard Model Predictions and New Physics Sensitivity in B -> DD Decays" https://arxiv.org/pdf/1410.8396.pdf
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[2] L.Bel, K.de Bruyn, R. Fleischer, M.Mulder, N.Tuning, "Anatomy of B -> DD Decays" https://arxiv.org/pdf/1505.01361.pdf
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[3] A.Zupanc et al [Belle Collaboration] "Improved measurement of B0 -> DsD+ and search for B0 -> Ds+Ds at Belle" https://arxiv.org/pdf/hep-ex/0703040.pdf
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[4] B.Aubert et al. [Babar Collaboration] "Search for the W-exchange decays B0 -> DD+" https://arxiv.org/pdf/hep-ex/0510051.pdf
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[5] R.Aaij et al. [LHCb Collaboration], "First observations of B0s -> D+D, Ds+D and D0D0 decays" https://arxiv.org/pdf/1302.5854.pdf
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''Contact: [mailto:niels.tuning@nikhef.nl Niels Tuning], [mailto:m.veronesi@nikhef.nl Michele Veronesi (PhD)], [mailto:s.esen@nikhef.nl Sevda Esen (postdoc)]''
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''Contact: [mailto:j.rojo@vu.nl Juan Rojo]''
  
=== LHCb: Measurement of relative ratio of B+ → D0D+ and B+ → D0Ds decays ===
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===Theory: The electroweak phase transition and baryogenesis/gravitational wave production ===
  
This decay is closely related to B0->Ds- Ds+ (see above), and close collaboration between the two master projects is foreseen. The decay mode B+->D0D+ is expected to be dominated by tree diagrams with some additional contributions from penguin diagrams. Assuming SU(3) symmetry, measurement of its branching fraction relative to Cabibbo-favored B+->D0D will enable better understanding of penguin contributions to the CP violating mixing phase.
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In extensions of the Standard Model the electroweak phase transition can be first order and proceed via the nucleation of bubbles. Colliding bubbles can produce gravitational waves [1] and plasma particles interacting with the bubbles can generate a matter-antimatter asymmetry [2]. A detailed understanding of the dynamics of the phase transitions is needed to accurately describe these processes. One project is to study QFT at finite temperature and compare/apply methods that address the non-perturbative IR dynamics of the thermal processes [3,4]. Another project is to calculate the velocity by which the bubbles expand, which is an important parameter for gravitational waves production and baryogensis. This entails among other things tunneling dymamics, (thermal) scattering rates and Boltzmann equations [5].
Relevant information:
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[1] L.Bel, K.de Bruyn, R. Fleischer, M.Mulder, N.Tuning, "Anatomy of B -> DD Decays" https://arxiv.org/pdf/1505.01361.pdf
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[2] R.Aaij et al. [LHCb Collaboration], "First observations of B0s -> D+D, Ds+D and D0D0 decays" https://arxiv.org/pdf/1302.5854.pdf
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[3] PDG: http://pdglive.lbl.gov/BranchingRatio.action?desig=261&parCode=S041
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''Contact: [mailto:niels.tuning@nikhef.nl Niels Tuning], [mailto:m.veronesi@nikhef.nl Michele Veronesi (PhD)], [mailto:s.esen@nikhef.nl Sevda Esen (postdoc)]''
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[1]https://arxiv.org/abs/1705.01783
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[2]https://arxiv.org/pdf/hep-ph/0609145.pdf
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[3]https://arxiv.org/pdf/1609.06230.pdf
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[4]https://arxiv.org/pdf/1612.00466.pdf
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[5]https://arxiv.org/pdf/1809.04907.pdf
  
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''Contact: [mailto:mpostma@nikhef.nl Marieke Postma]''
  
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===Theory: Cosmology of the QCD axion ===
  
=== Virgo: Fast determination of gravitational wave properties ===
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The QCD axion provides an elegant solution to the strong CP problem in QCD[1]. This project focus on the cosmological dynamics of this hypothesized axion field, and in particular the possibility that it can both produce the observed matter-antimatter asymmetry and dark matter abundance in our universe [2,3].
  
In the era of multi-messenger astronomy, the development of fast, accurate and computationally cheap methods for inference of properties of gravitational wave signal is of paramount importance. In this work, we will work on the development of rapid bayesian parameter estimation method for binary neutron stars as well as precessing black hole binaries. Bayesian parameter estimation methods require the evaluation of a likelihood that describe the probability of obtaining data for a given set of model parameters, which are parameters of gravitational wave signals in this particular problem. Bayesian inference for gravitational wave parameter estimation may require millions of these evaluation making them computationally costly. This work will combine the benefits of machine learning/ deep learning methods and order reduction methods of gravitational wave source modelling to speed up Bayesian inference of gravitational waves.
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[1]https://arxiv.org/abs/1812.02669
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[2]https://arxiv.org/pdf/hep-ph/0609145.pdf
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[3]https://arxiv.org/pdf/1910.02080.pdf
  
''Contact: [mailto:caudills@nikhef.nl Sarah Caudill]''
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''Contact: [mailto:mpostma@nikhef.nl Marieke Postma]''
  
=== Virgo: Simulations of Binary Neutron Star Mergers and applications for multimessenger astronomy ===
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===Theory: Neutrinos, hierarchy problem and cosmology ===
  
With the detection of the binary neutron star merger in August 2017 (GW170817) a new era of multi-messenger astronomy started. GW170817 proved that neutron star mergers are ideal laboratories to constrain the equation of state of cold supranuclear matter, to study the central engines of short GRBs, and to understand the origin and production of heavy elements.
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The electroweak hierachy problem is absent if the quadratic term in the Higgs potential is generated dynamically. This is achieved in 'the neutrino option' [1] where the Higgs potential stems exclusively from quantum effects of heavy right-handed neutrinos, which can also generate the mass pattern of the oberved left-handed neutrinos. The project focusses on model building aspects (e.g. [2]) and the cosmology (e.g. leptogenesis [3]) of these set-ups.
The fundamental tool to understand the last stages of the binary dynamics are numerical relativity simulations. In this project the student will be introduced to the basics of numerical relativity simulations of binary neutron star simulations and will be able to perform simulations on its own. Based on these simulations and the first experience it will be possible to focus on one of the following aspects:
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- the estimation of the ejected material released from the merger and the development of models for the electromagnetic signals
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[1] https://arxiv.org/pdf/1703.10924.pdf
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[2] https://arxiv.org/pdf/1807.11490.pdf
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[3] https://arxiv.org/pdf/1905.12642.pdf
  
- further improvement of gravitational waveform models including numerical relativity information
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''Contact: [mailto:mpostma@nikhef.nl Marieke Postma]''
  
- further improvement of the construction of the initial conditions of binary neutron star simulations
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=== KM3NeT: Reconstruction of first neutrino interactions in KM3NeT ===
  
- code improvements of the evolution code incorporating additional microphysical aspects as magnetic fields, tabulated equation of states, or neutrino leakage schemes.
+
The neutrino telescope KM3NeT is under construction in the Mediterranean Sea aiming to detect cosmic neutrinos. Its first few strings with sensitive photodetectors have been deployed at both the Italian and the French detector sites. Already these few strings provide for the option to reconstruct in the detector the abundant muons stemming from interactions of cosmic rays with the atmosphere and to identify neutrino interactions. In this project the available data will be used together with simulations to best reconstruct the event topologies and optimally identify and reconstruct the first neutrino interactions in the KM3NeT detector and with this pave the path towards accurate neutrino oscillation measurements and neutrino astronomy.  
  
- studying the merger properties of neutron stars with exotic objects as boson or axion stars.  
+
Programming skills are essential, mostly root and C++ will be used.
 +
''Contact: [mailto:bruijn@nikhef.nl Ronald Bruijn] [mailto:dosamtnikhef.nl Dorothea Samtleben]'''
  
''Contact: [mailto:diettim@nikhef.nl Tim Dietrich]''
+
=== KM3NeT: Searching for New Heavy Neutrinos ===
  
=== Virgo: Measuring cosmological parameters from gravitational-wave observations of compact binaries ===
+
In this project we will be searching for a new heavy neutrino, looking at signatures created by atmospheric neutrinos interacting in the detector volume of KM3NeT-ORCA. The aim of this project is to study a specific event topology which appears as double blobs of signals detected separately by densely instrumented ORCA detector units. We will be exploiting the tau reconstruction algorithms to verify the possibility of ORCA to detect such signals and to estimate the potential sensitivity of the experiment as well. Basic knowledge of elementary particle physics and data analysis techniques will be advantageous. The knowledge of programming languages e.g. python (and possibly C++) and ROOT are advantageous but not mandatory.
  
Gravitational wave observation of the binary neutron star merger GW170817 with its coincident optical counterpart led to a first "standard siren" measurement of the Hubble parameter independent of the cosmological distance ladder. While multiple similar observations are expected to improve the precision of the measurement, a statistical method of cross correlation with galaxy catalogues of gravitational-wave distance estimates is expected to work even without identified electromagnetic transients, and for binary black hole mergers in particular. The project would primarily be a study of various systematic effects in this analysis and correcting for them. The work will involve use of computational techniques to analyze LIGO-Virgo data. Some prior experience of programmimg is expected.
+
''Contact: [mailto:suzanbp@nikhef.nl Suzan B. du Pree] [mailto:dveijk@nikhef.nl Daan van Eijk]''
  
''Contact: [mailto:archis@nikhef.nl Archisman Ghosh] and [mailto:vdbroeck@nikhef.nl Chris Van Den Broeck]''
+
=== KM3NeT: Dark Matter with KM3NeT-ORCA ===
  
=== Detector R&D: Spectral X-ray imaging - Looking at colours the eyes can't see ===
+
Dark Matter is thought to be everywhere (we should be swimming through it), but we have no idea what it is. Using the good energy and angular resolutions of the KM3NeT neutrino telescope, we can search for Dark Matter signatures that originate from the center of our galaxy. In this project, we will search for such signatures using the reconstructed track and shower events with the KM3NeT-ORCA detector to discover relatively light Dark Matter particles. Since this year, the KM3NeT-ORCA  experiment has 6 detection lines under the Mediterranean Sea: fully operational and continuously taking data. Using the available data, it is possible to compare data and simulation for different event topologies and to estimate the experiment's sensitivity. The project is suitable for a student who is interested to explore new physics scenarios and willing to develop new skills. Basic knowledge of elementary particle physics and data analysis techniques will be advantageous. The knowledge of programming languages e.g. python (possibly C++) and ROOT data analysis tool are advantageous but not mandatory.
  
When a conventional X-ray image is made to analyse the composition of a sample, or to perform a medical examination on a patient, one acquires an image that only shows intensities. One obtains a ‘black and white’ image. Most of the information carried by the photon energy is lost. Lacking spectral information can result in an ambiguity between material composition and amount of material in the sample. If the X-ray intensity as a function of the energy can be measured (i.e. a ‘colour’ X-ray image) more information can be obtained from a sample. This translates to less required dose and/or to a better understanding of the sample that is being investigated. For example, two fields that can benefit from spectral X-ray imaging are mammography and real time CT.
+
''Contact: [mailto:suzanbp@nikhef.nl Suzan B. du Pree] [mailto:dveijk@nikhef.nl Daan van Eijk]''
  
X-ray detectors based on Medipix/Timepix pixel chips have spectral resolving capabilities and can be used to make polychromatic X-ray images. Medipix and Timepix chips have branched from pixel chips developed for detectors for high energy physics collider experiments.
 
  
Activities in the field of (spectral) CT scans are performed in a collaboration between two institutes (Nikhef and CWI) and two companies (ASI and XRE).
+
=== Gravitational Waves: Unraveling the structure of neutron stars with gravitational wave observations ===
  
Some activities that students can work on:
+
Neutron stars were first discovered more than half a century ago, yet their detailed internal structure largely remains a mystery. A range of theoretical models have been put forward for the neutron star "equation of state", but until recently there was no real way to test them. The direct detection of gravitational waves with LIGO and Virgo has the potential to remedy the situation. When two neutron stars spiral towards each other, they get tidally deformed in a way that is determined by the equation of state, and these deformations get imprinted upon the shape of the gravitational wave that gets emitted. After the first gravitational wave observation of such an event in 2017, several equation of state models could already be ruled out. With expected upgrades of the detectors, we will at some point have access not only to the "inspiral" of binary neutron stars, but to the merger itself, and what happens afterwards. The project will consist of using results from large-scale numerical simulations to come up with a heuristic model for the waveform that describes the inspiral-merger-postmerger process with sufficient accuracy given expected detector sensitivities, and to develop data analysis techniques to efficiently use this model to extract information about the neutron star equation of state.
  
- Medical X-ray imaging (CT and ‘flat’ X-ray images): Detection of iodine contrast agent. Detection of calcifications (hint for a tumour).
+
''Contact: [mailto:vdbroeck@nikhef.nl Chris Van Den Broeck]''
  
- Material research: Using spectral information to identify materials and recognise compounds.
 
  
- Determine how much existing applications can benefit from spectral X-ray imaging and look for potential new applications.  
+
=== Gravitational Waves: Searches for gravitational waves from compact binary coalescence ===
 +
Searches for gravitational waves from the mergers of black holes and neutron stars have been extraordinarily successful in the last four years. We are now beginning to study a population of heavy stellar-mass black holes in detail, including understanding how these systems came to form and whether they are consistent with general relativity. Additionally, the detection of binary neutron star mergers is allowing us to probe their extreme matter. However, we’ve only just scratched the surface of possible signals and the new physics they’d allow us to study. The detection of highly spinning and precessing systems would allow us to perform black hole population statistics to an extraordinary degree of accuracy. Detection of sub-solar mass systems would provide evidence of dark matter. However, these searches are difficult because they require us to work in high-dimensional spaces and develop new statistical methods. There are possibilities for several projects that involve the development and implementation of these new searches as well as the interpretation of the results, particularly in terms of the physics describing compact binary mergers.
  
- Characterise, calibrate, optimise X-ray imaging detector systems.  
+
''Contact: [mailto:physarah@gmail.com Sarah Caudill]''
  
''Contact: [mailto:martinfr@nikhef.nl Martin Fransen]''
 
  
=== Detector R&D: Compton camera ===
+
=== Gravitational Waves: Computer modelling to design the laser interferometers for the Einstein telescope ===
  
In the Nikhef R&D group we develop instrumentation for particle physics but we also investigate how particle physics detectors can be used for different purposes. A successful development is the Medipix chip that can be used in X-ray imaging. For use in large scale medical applications compton scattering limits however the energy resolving possibilities. You will investigate whether it is in principle possible to design a X-ray application that detects the compton scattered electron and the absorbed photon. Your ideas can be tested in practice in the lab where a X-ray scan can be performed.
+
A new field of instrument science led to the successful detection of gravitational waves by the LIGO detectors in 2015. We are now preparing the next generation of gravitational wave observatories, such as the Einstein Telescope, with the aim to increase the detector sensitivity by a factor of ten, which would allow, for example, to detect stellar-mass black holes from early in the universe when the first stars began to form. This ambitious goal requires us to find ways to significantly improve the best laser interferometers in the world.
  
''Contact: [mailto:martinfr@nikhef.nl Martin Fransen]''
+
Gravitational wave detectors, such as LIGO and VIRGO, are complex Michelson-type interferometers enhanced with optical cavities. We develop and use numerical models to study these laser interferometers, to invent new optical techniques and to quantify their performance. For example, we synthesize virtual mirror surfaces to study the effects of higher-order optical modes in the interferometers, and we use opto-mechanical models to test schemes for suppressing quantum fluctuations of the light field. We can offer several projects based on numerical modelling of laser interferometers. All projects will be directly linked to the ongoing design of the Einstein Telescope.
  
=== Detector R&D: Holographic projector ===
+
''Contact: [mailto:a.freise@nikhef.nl Andreas Freise]''
  
A difficulty in generating holograms (based on the interference of light) is the required dense pixel pitch. One would need a pixel pitch of less than 200 nanometer. With larger pixels artefacts occur due to spatial under sampling. A pixel pitch of 200 nanometer is difficult, if not, impossible, to achieve, especially for larger areas. Another challenge is the massive amount of computing power that would be required to control such a dense pixel matrix.
 
  
A new holographic projection method has been developed that reduces under sampling artefacts for projectors with a ‘low’ pixel density. It is using 'pixels' at random but known positions, resulting in an array of (coherent) light points that lacks (or has strongly surpressed) spatial periodicity. As a result a holographic projector can be built with a significantly lower pixel density and correspondingly less required computing power. This could bring holography in reach for many applications like display, lithography, 3D printing, metrology, etc..
+
=== Gravitational Waves: Digging away the noise to find the signal ===
+
Of course, nothing comes for free: With less pixels, holograms become noisier and the contrast will be reduced. The big question: How do we determine the requirements (in terms of pixel density, pixel positioning, etc..) for the holographic projector based on requirements for the holograms?
+
Requirements for a hologram can be expressed in terms of: Noise, contrast, resolution, suppression of under sampling artefacts, etc..
+
 
+
For this project we are building a proof of concept holographic emitter. This set-up will be used to verify simulation results (and also to project some cool holograms of course).
+
 
+
Students can do hands on lab-work (building and testing the proto type projector) and/or work on setting up simulation methods and models. Simulations in this field can be highly parallelized and are preferably written for parallel computing and/or GPU computing.
+
 
+
 
+
''Contact: [mailto:martinfr@nikhef.nl Martin Fransen]
+
 
+
=== Detector R&D: Laser Interferometer Space Antenna (LISA) ===
+
 
+
The space-based gravitational wave antenna LISA is without doubt one of the most challenging space missions ever proposed. ESA plans to launch around 2030 three spacecrafts that are separated by a few million kilometers to measure tiny variations in the distances between test-masses located in each spacecraft to detect the gravitational waves from sources such as supermassive black holes. The triangular constellation of the LISA mission is dynamic requiring a constant fine tuning related to the pointing of the laser links between the spacecrafts and a simultaneous refocusing of the telescope. The noise sources related to the laser links are expected to provide a dominant contribution to the LISA performance.
+
 
+
An update and extension of the LISA science simulation software is needed to assess the hardware development for LISA at Nikhef, TNO and SRON. A position is therefore available for a master student to study the impact of instrumental noise on the performance of LISA. Realistic simulations based on hardware (noise) characterization measurements that were done at TNO will be carried out and compared to the expected tantalizing gravitational wave sources.
+
 
+
Key words: LISA, space, gravitational waves, simulations, signal processing
+
 
+
''Contact: [mailto:nielsvb@nikhef.nl Niels van Bakel],[mailto:ernst-jan.buis@tno.nl  Ernst-Jan Buis]''
+
 
+
=== KM3NeT : Reconstruction of first neutrino interactions in KM3NeT ===
+
 
+
The neutrino telescope KM3NeT is under construction in the Mediterranean Sea aiming to detect cosmic neutrinos. Its first two strings with sensitive photodetectors have been deployed 2015&2016. Already these few strings provide for the option to reconstruct in the detector the abundant muons stemming from interactions of cosmic rays with the atmosphere and to identify neutrino interactions. In order to identify neutrinos an accurate reconstruction and optimal understanding of the backgrounds are crucial. In this project we will use the available data to identify and reconstruct the first neutrino interactions in the KM3NeT detector and with this pave the path towards neutrino astronomy.
+
 
+
Programming skills are essential, mostly root and C++ will be used.
+
  
'' Contact: [mailto:bruijn@nikhef.nl Ronald Bruijn]''
+
Gravitational Wave interferometers are extremely sensitive, but suffer
 +
from instrumental issues that produce noise that mimics astrophysical
 +
signals. This needs to be solved as much as possible before the data
 +
analysis. The problem is that  instrumentalists don't know about
 +
analysis pipelines, and data analysts don't know about experimental
 +
details. We need your help to bridge the gap. This is a good opportunity
 +
to learn about both sides and contribute directly to a booming
 +
international field. We have several tools and new ideas for correlating
 +
noises with the state of the instrument. These need to be developed
 +
further, used on years of data, and written up. Will require Python,
 +
signal processing and statistics.
  
=== ANTARES: Analysis of IceCube neutrino sources. ===
+
''Contact: [mailto:swinkels@nikhef.nl Bas Swinkels] and [mailto:physarah@gmail.com Sarah Caudill]''
  
The only evidence for high energetic neutrinos from cosmic sources so far comes from detections with the IceCube detector. Most of the detected events were reconstructed with a large uncertainty on their direction, which has prevented an association to astrophysical sources. Only for the high energetic muon neutrino candidates a high resolution in the direction has been achieved, but also for those no significant correlation to astrophysical sources has to date been detected.
 
The ANTARES neutrino telescope has since 2007 continuously taken neutrino data with high angular resolution, which can be exploited to further scrutinize the locations of these neutrino sources. In this project we will address the neutrino sources in a stacked analysis to further probe the origin of the neutrinos with enhanced sensitivity.
 
  
Programming skills are essential, mainly C++ and root will be used.  
+
=== Gravitational Waves: Machine Learning techniques for GW Interferometers ===
 +
The control of suspended optical cavities in the non linear regime. 
 +
Gravitational Wave interferometers are extremely sensitive, however suffer from a very small control range, causing unlocks,
 +
reducing the robustness of these instruments.
 +
In this project we will use a table top replica of a suspended optical cavity,
 +
located in the new R&D laser lab at Nikhef, for the development of a neural
 +
network to construct the positions from free falling mirror by using beam
 +
images. A database with simulated beam images can be used to train
 +
various neural networks before deployment in the table top experiment.
 +
We are looking for a hands-on and enthusiastic master student, interested
 +
in machine learning and experienced in programming languages like Python.
 +
Contacts: Rob Walet, Frank Linde
  
'' Contact: [mailto:dosamt@nikhef.nl Dorothea Samtleben]''
+
''Contact: [mailto:r.walet@nikhef.nl Rob Walet] and [mailto:f.l.linde@gmail.com Frank Linde]''
  
 
=== VU LaserLaB: Measuring the electric dipole moment (EDM) of the electron ===
 
=== VU LaserLaB: Measuring the electric dipole moment (EDM) of the electron ===
Line 308: Line 329:
 
At LaserLaB VU, we are responsible for building and testing a cryogenic source of BaF molecules. The main parts of this source are currently being constructed in the workshop. We are looking for enthusiastic master students to help setup the laser system that will be used to detect BaF. Furthermore, projects are available to perform simulations of trajectory simulations to design a lens system that guides the BaF molecules from the exit of the cryogenic source to the experiment.
 
At LaserLaB VU, we are responsible for building and testing a cryogenic source of BaF molecules. The main parts of this source are currently being constructed in the workshop. We are looking for enthusiastic master students to help setup the laser system that will be used to detect BaF. Furthermore, projects are available to perform simulations of trajectory simulations to design a lens system that guides the BaF molecules from the exit of the cryogenic source to the experiment.
  
'' Contact: [mailto:H.L.Bethlem@vu.nl Rick Bethlem]''
+
''Contact: [mailto:H.L.Bethlem@vu.nl Rick Bethlem]''
  
 
+
=== VU LaserLaB: Physics beyond the Standard model from molecules ===
=== VU LaserLab: Physics beyond the Standard model from molecules ===
+
  
 
Our team, with a number of staff members (Ubachs, Eikema, Salumbides, Bethlem, Koelemeij) focuses on precision measurements in the hydrogen molecule, and its isotopomers. The work aims at testing the QED calculations of energy levels in H2, D2, T2, HD, etc. with the most precise measurements, where all kind of experimental laser techniques play a role (cw and pulsed lasers, atomic clocks, frequency combs, molecular beams). Also a target of studies is the connection to the "Proton size puzzle", which may be solved  through studies in the hydrogen molecular isotopes.
 
Our team, with a number of staff members (Ubachs, Eikema, Salumbides, Bethlem, Koelemeij) focuses on precision measurements in the hydrogen molecule, and its isotopomers. The work aims at testing the QED calculations of energy levels in H2, D2, T2, HD, etc. with the most precise measurements, where all kind of experimental laser techniques play a role (cw and pulsed lasers, atomic clocks, frequency combs, molecular beams). Also a target of studies is the connection to the "Proton size puzzle", which may be solved  through studies in the hydrogen molecular isotopes.
Line 328: Line 348:
 
This is also a study of the hydrogen molecular ion HD+, where important results were  obtained not so long ago, and where we have a strong activity: http://www.nat.vu.nl/~wimu/Publications/ncomms10385.pdf
 
This is also a study of the hydrogen molecular ion HD+, where important results were  obtained not so long ago, and where we have a strong activity: http://www.nat.vu.nl/~wimu/Publications/ncomms10385.pdf
  
These five results mark the various directions we are pursuing, and in all directions we aim at obtaining improvements. Specific projects with students can be defined; those are mostly experimental, although there might be some theoretical tasks, like:
+
These five results mark the various directions we are pursuing, and in all directions we aim at obtaining improvements. Specific projects with students can be defined; those are mostly experimental, although there might be some theoretical tasks, like performing calculations of hyperfine structures.  
* Performing calculations of hyperfine structures
+
''Contact: [mailto:w.m.g.ubachs@vu.nl Wim Ubachs] [mailto:k.s.e.eikema@vu.nl Kjeld Eikema] [mailto:h.l.bethlem@vu.nl Rick Bethlem]''
 
+
As for the theory there might also be an international connection for specifically bright theory students: we collaborate closely with prof. Krzystof Pachucki; we might find an opportunity
+
for a student to perform (the best !) QED calculations in molecules, when working in Warsaw and partly in Amsterdam. Prof Frederic Merkt from the ETH Zurich, an expert in the field, will come to work with us on "hydrogen"
+
during August - Dec 2018 while on sabbatical.
+
 
+
'' Contact: [mailto:w.m.g.ubachs@vu.nl Wim Ubachs] [mailto:k.s.e.eikema@vu.nl Kjeld Eikema] [mailto:h.l.bethlem@vu.nl Rick Bethlem]''
+
 
+
  
  
  
 
[[Last years MSc Projects|Last year's MSc Projects]]
 
[[Last years MSc Projects|Last year's MSc Projects]]

Latest revision as of 11:35, 22 June 2020

Master Thesis Research Projects

The following Master thesis research projects are offered at Nikhef. If you are interested in one of these projects, please contact the coordinator listed with the project.

Contents

[edit] Projects with September 2020 start

[edit] ATLAS: Top Spin optimal observables using Artificial Intelligence

The top quark has an exceptional high mass, close to the electroweak symmetry breaking scale and therefore sensitive to new physics effects. Theoretically, new physics is well described in the EFT framework [1]. The (EFT) operators are experimentally well accessible in single top t-channel production where the top quark is produced spin polarized. The focus at Nikhef is the operator O_{tW} with a possible imaginary phase, leading to CP violation. Experimentally, many angular distribution are reconstructed in the top rest frame to hunt for these effects. We are looking for a limited set of optimal observables. The objective of your Master project would be to find optimal observables using simulated events including the detector effects and possible systematic deviations. All techniques are allowed, but promising new developments are methods which involve artifical intelligence. This work could lead to an ATLAS note.

[1] https://arxiv.org/abs/1807.03576

Contact: Marcel Vreeswijk [1] and Jordy Degens [2]

[edit] ATLAS: The Next Generation

After the observation of the coupling of Higgs bosons to fermions of the third generation, the search for the coupling to fermions of the second generation is one of the next priorities for research at CERN's Large Hadron Collider. The search for the decay of the Higgs boson to two charm quarks is very new [1] and we see various opportunities for interesting developments. For this project we propose improvements in reconstruction (using exclusive decays), advanced analysis techiques (using deep learning methods) and expanding the theory interpretation. Another opportunity would be the development of the first statistical combination of results between the ATLAS and CMS experiment, which could significantly improve the discovery potentional.

[1] https://arxiv.org/abs/1802.04329

Contact: Tristan du Pree and Marko Stamenkovic

[edit] ATLAS: The Most Energetic Higgs Boson

The production of Higgs bosons at the highest energies could give the first indications for deviations from the standard model of particle physics, but production energies above 500 GeV have not been observed yet [1]. The LHC Run-2 dataset, collected during the last 4 years, might be the first opportunity to observe such processes, and we have various ideas for new studies. Possible developments include the improvement of boosted reconstruction techniques, for example using multivariate deep learning methods. Also, there are various opportunities for unexplored theory interpretations (using the MadGraph event generator), including effective field theory models (with novel ‘morphing’ techniques) and new interpretations of the newly observed boosted VZ(bb) process.

[1] https://arxiv.org/abs/1709.05543

Contact: Tristan du Pree and Brian Moser

[edit] LHCb: Measurement of delta md

The decay B0->D-pi+ is very abundant in LHCb, and therefore ideal to study the oscillation frequency delta md, with which B0 mesons oscillate into anti-B0 mesons, and vice versa. This process proceeds through a so-called box diagram which might hide new yet-undiscovered particles. Recently, it has been realized that value of delta md is in tension with the valu of CKM-angle gamma, triggering renewed interest in this measurement.

Contact: Marcel Merk

[edit] LHCb: Searching for CPT violation

CPT symmetry is closely linked to Lorentz symmetry, and any violation would revolutionize science. There are possibilities though that supergravity could cause CPT violating effects in the system of neutral mesons. The precise study of B0s oscillations in the abundant Bs->Dspi decays can give the most stringent limits on Im(z) to date.

Contact: Marcel Merk

[edit] LHCb: BR(B0->D-pi+) and fd/fu with B+->D0pi+

The abundant decay B0->D-pi+ is often used as normalization channel, given its clean signal, and well-known branching fraction, as measured by the B-factories. However, this branching fraction can be determined more precisely, when comparing to the decay B+->D0pi+ , which has a twice better precision. In addition, the production of B0 and B+ mesons is often assumed to be equal, based on isospin symmetry. The study of B+->D0pi+ and B0->D-pi+ allows for the first measurement of this ratio, fd/fu.

Contact: Marcel Merk


[edit] LHCb: Optimization studies for Vertex detector at the High Lumi LHCb

The LHCb experiment is dedicated to measure tiny differences between matter and antimatter through the precise study of rare processes involving b or c quarks. The LHCb detector will undergo a major modification in order to dramatically increase the luminosity and be able to measure indirect effects of physics beyond the standard model. In this environment, over 42 simultaneous collisions are expected to happen at a time interval of 200 ps where the two proton bunches overlap. The particles of interest have a relatively long lifetime and therefore the best way to distinguish them from the background collisions is through the precise reconstruction of displaced vertices and pointing directions. The new detector considers using extremely recent or even future technologies to measure space (with resolutions below 10 um) and time (100 ps or better) to efficiently reconstruct the events of interest for physics. The project involves changing completely the LHCb Vertex Locator (VELO) design in simulation and determine what can be the best performance for the upgraded detector, considering different spatial and temporal resolutions.

Contact: Kazu Akiba

[edit] LHCb: Measurement of charge multiplication in heavily irradiated sensors

During the R&D phase for the LHCb VELO Upgrade detector a few sensor prototypes were irradiated to the extreme fluence expected to be achieved during the detector lifetime. These samples were tested using high energy particles at the SPS facility at CERN with their trajectories reconstructed by the Timepix3 telescope. A preliminary analysis revealed that at the highest irradiation levels the amount of signal observed is higher than expected, and even larger than the signal obtained at lower doses. At the Device Under Test (DUT) position inside the telescope, the spatial resolution attained by this system is below 2 um. This means that a detailed analysis can be performed in order to study where and how this signal amplification happens within the 55x55 um^2 pixel cell. This project involves analysing the telescope and DUT data to investigate the charge multiplication mechanism at the microscopic level.

Contact: Kazu Akiba

[edit] ALICE: Searching for the strongest magnetic field in nature

In case of a non-central collision between two Pb ions, with a large value of impact parameter (b), the charged nucleons that do not participate in the interaction (called spectators) create strong magnetic fields. A back of the envelope calculation using the Biot-Savart law brings the magnitude of this filed close to 10^19Gauss in agreement with state of the art theoretical calculation, making it the strongest magnetic field in nature. The presence of this field could have direct implications in the motion of final state particles. The magnetic field, however, decays rapidly. The decay rate depends on the electric conductivity of the medium which is experimentally poorly constrained. Overall, the presence of the magnetic field, the main goal of this project, is so far not confirmed experimentally.

Contact: Panos Christakoglou

[edit] ALICE: Looking for parity violating effects in strong interactions

Within the Standard Model, symmetries, such as the combination of charge conjugation (C) and parity (P), known as CP-symmetry, are considered to be key principles of particle physics. The violation of the CP-invariance can be accommodated within the Standard Model in the weak and the strong interactions, however it has only been confirmed experimentally in the former. Theory predicts that in heavy-ion collisions, in the presence of a deconfined state, gluonic fields create domains where the parity symmetry is locally violated. This manifests itself in a charge-dependent asymmetry in the production of particles relative to the reaction plane, what is called the Chiral Magnetic Effect (CME). The first experimental results from STAR (RHIC) and ALICE (LHC) are consistent with the expectations from the CME, however further studies are needed to constrain background effects. These highly anticipated results have the potential to reveal exiting, new physics.

Contact: Panos Christakoglou

[edit] ALICE: Machine learning techniques as a tool to study the production of heavy flavour particles

There was recently a shift in the field of heavy-ion physics triggered by experimental results obtained in collisions between small systems (e.g. protons on protons). These results resemble the ones obtained in collisions between heavy ions. This consequently raises the question of whether we create the smallest QGP droplet in collisions between small systems. The main objective of this project will be to study the production of charm particles such as D-mesons and Λc-baryons in pp collisions at the LHC. This will be done with the help of a new and innovative technique which is based on machine learning (ML). The student will also extend the studies to investigate how this production rate depends on the event activity e.g. on how many particles are created after every collision.

Contact: Panos Christakoglou and Alessandro Grelli

[edit] ALICE: Energy Loss of Energetic Quarks and Gluons in the Quark-Gluon Plasma

One of the ways to study the quark-gluon plasma that is formed in high-energy nuclear collisions, is using high-energy partons (quarks or gluons) that are produced early in the collision and interact with the quark-gluon plasma as they propagate through it. There are several current open questions related to this topic, which can be explored in a Master's project. For example, we would like to use the new Monte Carlo generator framework JetScape to simulate collisions to see whether we can extract information about the interaction with the quark-gluon plasma. In the project you will collaborate with one of the PhD students or postdocs in our group to use the model to generate predictions of measurements and compare those to data analysis results. Depending on your interests, the project can focus more on the modeling aspects or on the analysis of experimental data from the ALICE detector at the LHC.

Contact: Marco van Leeuwen and Marta Verweij

[edit] ALICE: Extreme Rare Probes of the Quark-Gluon Plasma

The quark-gluon plasma is formed in high-energy nuclear collisions and also existed shortly after the big bang. With the large amount of data collected in recent years at the Large Hadron Collider at CERN, rare processes that previously were not accessible provide now new ways to study how the quark-gluon plasma emerges from the fundamental theory of strong interaction. One of such processes is the heavy W boson which in many cases decays to two quarks. The W boson itself doesn’t interact with the quark-gluon plasma because it doesn’t carry color, but the quark decay products do interact with the plasma and therefore provide an ideal tool to study the space-time evolution of this hot and dense medium. In this project you will use data from the ALICE detector at the LHC and simulated data from generators to study various physics mechanisms that could be happening in the real collisions.

Contact: Marta Verweij and Marco van Leeuwen

[edit] ALICE: Jet Quenching with Machine Learning

Machine learning applications are rising steadily as a vital tool in the field of data science but are relatively new in the particle physics community. In this project machine learning tools will be used to gain insights into the modification of a parton shower in the quark-gluon plasma (QGP). The QGP is created in high-energy nuclear collisions and only lives for a very short period of time. Highly energetic partons created in the same collisions interact with the plasma while they travers it and are observed as a collimated spray of particles, known as jets, in the detector. One of the key recent insights is that the internal structure of jets provides information about the evolution of the QGP. With data recorded by the ALICE experiment, you will use jet substructure techniques in combination with machine learning algorithms to dissect the structure of the QGP. Machine learning will be used to select the regions of radiation phase space that are affected by the presence of the QGP.

Contact: Marta Verweij and Marco van Leeuwen

[edit] Lepton Collider: Pixel TPC testbeam

In the Lepton Collider group at Nikhef we work on a tracking detector for a future Collider (e.g. the ILC in Japan). We are developing a gaseous Time Projection Chamber with a pixel readout. At Nikhef we have built an 8-quad GridPix module based on the Timepix3 chip, which is a detector of about 20 cm x 40 cm x 10 cm in size. In August 2020 we will test the device at the DESY particle accelerator in Hamburg. For the project you could work on preparations for the test beam (e.g. running the data acquisition, perform data monitoring using our set up in the lab). The next topics will be the participation in the data taking during the test beam at DESY, the analysis of the data using C++ and ROOT and - finally - publication of the results in a scientific journal.

Our latest paper can be found in https://www.nikhef.nl/~s01/quad_paper.pdf [www.nikhef.nl].

Contact: Peter Kluit and Kees Ligtenberg

[edit] Dark Matter: Sensitive tests of wavelength-shifting properties of materials for dark matter detectors

Rare event search experiments that look for neutrino and dark matter interactions are performed with highly sensitive detector systems, often relying on scintillators, especially liquid noble gases, to detect particle interactions. Detectors consist of structural materials that are assumed to be optically passive, and light detection systems that use reflectors, light detectors, and sometimes, wavelength-shifting materials. MSc theses are available related to measuring the efficiency of light detection systems that might be used in future detectors. Furthermore, measurements to ensure that presumably passive materials do not fluoresce, at the low level relevant to the detectors, can be done. Part of the thesis work can include Monte Carlo simulations and data analysis for current and upcoming dark matter detectors, to study the effect of different levels of desired and nuisance wavelength shifting. In this project, students will acquire skills in photon detection, wavelength shifting technologies, vacuum systems, UV and extreme-UV optics, detector design, and optionally in C++ programming, data analysis, and Monte Carlo techniques.

Contact: Tina Pollmann and Patrick Decowski

[edit] Dark Matter: Signal reconstruction in XENONnT

The next generation direct detection dark matter experiment - XENONnT - comprises close to 500 photomultiplier tubes (PMTs) in the main detector volume. These PMTs are configured to be able to detect even single photons. When a single photoelectron (PE) signal is detected the detected signal (a pulse) is convoluted with the detector response of the PMT. Due to this detector response the pulse shape of a single PE is spread out in time. For XENONnT we would like to explore the possibility to implement a digital (software) filter to deconvolve the detected pulse back to the “true” instantaneous shape (without the detector spread). This is a virtually unexplored new step in the Xenon analysis framework. Later in the analysis framework these pulses from all the PMTs are combined into a signal referred to as a ‘peak’. For XENONnT it is of essence to be extremely good in discriminating between two types of peaks caused by interactions in the detector; a prompt primary scintillation signal (S1) and a secondary ionization signal (S2). The parameters in the software haven’t - as of the time of writing - been optimized for the XENONnT-detector conditions. The student would investigate how a deconvolution filter would benefit the XENONnT analysis framework and develop such a filter. Furthermore, the student will work on the classification of these signals to fully exploit the XENONnT-detector to optimize the classification. This will be done with simulated data at first but may later even be performed on actual XENONnT-data. As an extension, the possibility of applying machine learning to correctly distinguish between the two signals could be explored. This is a data-analysis oriented project where Python skills are paramount.

Contact: Patrick Decowski and Joran Angevaare

[edit] Dark Matter: XAMS R&D Setup

The Amsterdam Dark Matter group operates an R&D xenon detector at Nikhef. The detector is a dual-phase xenon time-projection chamber and contains about 4kg of ultra-pure liquid xenon. We use this detector for the development of new detection techniques - such as utilizing our newly installed silicon photomultipliers - and to improve the understanding of the response of liquid xenon to various forms of radiation. The results could be directly used in the XENONnT experiment, the world’s most sensitive direct detection dark matter experiment at the Gran Sasso underground laboratory, or for future Dark Matter experiments like DARWIN. We have several interesting projects for this facility. We are looking for someone who is interested in working in a laboratory on high-tech equipment, modifying the detector, taking data and analyzing the data him/herself. You will "own" this experiment.

Contact: Patrick Decowski and Auke Colijn

[edit] Dark Matter: DARWIN Sensitivity Studies

DARWIN is the "ultimate" direct detection dark matter experiment, with the goal to reach the so-called "neutrino floor", when neutrinos become a hard-to-reduce background. The large and exquisitely clean xenon mass will allow DARWIN to also be sensitive to other physics signals such as solar neutrinos, double-beta decay from Xe-136, axions and axion-like particles etc. While the experiment will only start in 2025, we are in the midst of optimizing the experiment, which is driven by simulations. We have an opening for a student to work on the GEANT4 Monte Carlo simulations for DARWIN, as part of a simulation team together with the University of Freiburg and Zurich. We are also working on a "fast simulation" that could be included in this framework. It is your opportunity to steer the optimization of a large and unique experiment. This project requires good programming skills (Python and C++) and data analysis/physics interpretation skills.

Contact: Patrick Decowski and Auke Colijn

[edit] Dark Matter: Fast simulation studies

For Dark Matter experiments it is crucial to understand sources of backgrounds in great detail. The most common way to study the effect of backgrounds to the Dark Matter sensitivity is by the use of Monte Carlo simulations. Unfortunately, the standard Monte Carlo techniques are extremely inefficient. One needs to sometimes simulate millions of events before one background event appears in the Dark Matter search area. We have developed a Monte Carlo technique that accelerates this process by up to 1000x. The method has been validated on very simple and unrealistic detector models. In goal of this project is to make a realistic detector model for the fast detector simulations. For this we are looking for a student with good programming skills, an interest in a software project, and the desire to deeply understand analysis of Dark Matter experimental data.

Contact: Patrick Decowski and Auke Colijn

[edit] Dark Matter & Amsterdam Scientific Instruments: Simulations for Industry

In the Nikhef Dark Matter group we have built up an extensive expertise with Monte Carlo simulations of ionizing radiation. Although these simulations have the aim to estimate background levels in our XENON experiments, the same techniques can be applied to study radiation transport in industrial devices. Amsterdam Scientific Instruments (ASI) is a company at Science Park that develops and sells radiation imaging equipment that is used amongst others in electron microscopy. For this application ASI needs a detailed study of gamma ray backgrounds to optimize shielding for their products. The project aims at optimizing a shielding design based on GEANT4 simulations. The results may be implemented in next generation products of ASI. We are looking for a student with preferably strong computing skills, and with an interest in science-industrial collaboration.

Contact: Patrick Decowski and Auke Colijn

[edit] The Modulation experiment: Data Analysis

For years there have been controversial claims of potential new-physics on the basis of time-varying decay rates of radioactive sources on top of ordinary exponential decay. While some of these claims have been refuted, others have still to be confirmed or falsified. To this end, a dedicated experiment - the modulation experiment - has been designed and operational for the past four years. Using four identical and independent setups the experiment is almost ready for a final analysis to conclude on these claims. In this project the student will perform this analysis, preferably resulting in a conclusive paper. This will require combining the data of the four setups and close collaboration with a small group constituting a collaboration of the four different involved institutes (Purdue University (USA), Universität Zürich (Switzerland), Centro Brasileiro de Pesquisas Fisicas (Brasil) and Nikhef). This project is data-analysis oriented. Additionally, lab-skills can be required as one of the setups is situated at Nikhef.

Contact: Auke Colijn and Joran Angevaare

[edit] Detector R&D: Laser Interferometer Space Antenna (LISA)

The space-based gravitational wave antenna LISA is, without a doubt, one of the most challenging space missions ever proposed. ESA plans to launch around 2030 three spacecraft that are separated by a few million kilometers to measure tiny variations in the distances between test-masses located in each satellite to detect the gravitational waves from sources such as supermassive black holes. The triangular constellation of the LISA mission is dynamic, requiring a constant fine-tuning related to the pointing of the laser links between the spacecraft and a simultaneous refocusing of the telescope. The noise sources related to the laser links expect to provide a dominant contribution to the LISA performance. An update and extension of the LISA science simulation software are needed to assess the hardware development for LISA at Nikhef, TNO, and SRON. A position is therefore available for a master student to study the impact of instrumental noise on the performance of LISA. Realistic simulations based on hardware (noise) characterization measurements performed at TNO will be carried out and compared to the expected tantalizing gravitational wave sources.

Contact: Niels van Bakel,Ernst-Jan Buis

[edit] Detector R&D: Spectral X-ray imaging - Looking at colours the eyes can't see

When a conventional X-ray image is taken, one acquires an image that only shows intensities. a ‘black and white’ image. Most of the information carried by the photon energy is lost. Lacking spectral information can result in an ambiguity between material composition and amount of material in the sample. If the X-ray intensity as a function of the energy can be measured (i.e. a ‘colour’ X-ray image) more information can be obtained from a sample. This translates to less required dose and/or to a better understanding of the sample that is being investigated. For example, two fields that can benefit from spectral X-ray imaging are mammography and real time CT.

Detectors using Medipix3 chips are used for X-ray imaging. Such a detector is composed of a pixel chip with a semiconductor sensor bonded on top of it. Photoelectric absorption of X-rays in the sensor results in an amount of charge being released that is proportional to the X-ray energy. This charge is registered by a pixel. Depending on configuration, in each pixel 1, 2, 4 or 8 detection thresholds can be set and so, a number of energy bins can be defined. One of the challenges is to maximise X-ray image quality by minimising effects caused by dispersion in the sensitivity of the pixels. The effects of this dispersion can partly be compensated by applying a specific measurement method in combination with image post processing.

You can work on improving measurement methods and on improving post processing methods. There is flexibility of the planned work depending on the skillset you have. The aim is to get the best X-ray energy resolution over the entire pixel chip. This in turn improves image quality and therefore X-ray CT reconstruction quality.

Important note: Much of this work is to be performed in the laboratory. For as long as corona safety measures are active, the labs at Nikhef are not accessible for students and this project cannot be worked on except for post-processing in software. Currently we hope that the situation will have improved by August. Please see the following videos for examples of our work:

https://youtu.be/cgwQvjfUYns

https://youtu.be/tf9ZLALPVNY

https://youtu.be/vjPX7SxvSUk

https://youtu.be/LqjNVSm7Hoo

Contact: Martin Fransen,Navrit Bal

[edit] Detector R&D: Holographic projector

A difficulty in projecting holograms (based on the interference of light) is the required dense pixel pitch of a projector. One would need a pixel pitch of less than 200 nanometer. With larger pixels artefacts occur due to spatial under sampling. A pixel pitch of 200 nanometer is difficult, if not, impossible, to achieve, especially for larger areas. Another challenge is the massive amount of computing power that would be required to control such a dense pixel matrix.

A new holographic projection method has been developed that reduces under sampling artefacts for projectors with a ‘low’ pixel density. It uses 'pixels' at random but known positions, resulting in an array of (coherent) light points that lacks (or has suppressed) spatial periodicity. As a result a holographic projector can be built with a significantly lower pixel density and correspondingly less required computing power. This could bring holography in reach for many applications like display, lithography, 3D printing, metrology, etc...

Of course, nothing comes for free: With less pixels, holograms become noisier and the contrast will be reduced (not all light ends up in the hologram). The questions: How does the quality of a hologram depend on pixel density? How do we determine projector requirements based on requirements for hologram quality?

Requirements for a hologram can be expressed in terms of: Noise, contrast, resolution, suppression of under sampling artefacts, etc..

For this project we have built a proof of concept holographic emitter. This set-up will be used to verify simulation results (and also to project some cool holograms of course ;-).

Examples of what you could be working on:

a. Calibration/characterisation of the current projector and compensation of systematic errors.

b. To realize a phased array of randomly placed light sources the pixel matrix of the projector must be ‘relayed’ onto a mask with apertures at random but precisely known positions. Determine the best possible relaying optics and design an optimized mask accordingly. Factors like deformation of the projected pixel matrix and limitations in resolving power of the lens system must be taken into account for mask design.

Important note: Much of this work is to be performed in the laboratory. For as long as corona safety measures are active, the labs at Nikhef are not accessible for students and this project cannot be worked on. Currently we hope that the situation will have improved by august.

Contact: Martin Fransen

[edit] Theory: The Effective Field Theory Pathway to New Physics at the LHC

A promising framework to parametrise in a robust and model-independent way deviations from the Standard Model (SM) induced by new heavy particles is the Standard Model Effective Field Theory (SMEFT). In this formalism, beyond the SM effects are encapsulated in higher-dimensional operators constructed from SM fields respecting their symmetry properties. In this project, we aim to carry out a global analysis of the SMEFT from high-precision LHC data, including Higgs boson production, flavour observables, and low-energy measurements. This analysis will be carried out in the context of the recently developed SMEFiT approach [1] based on Machine Learning techniques to efficiently explore the complex theory parameter space. The ultimate goal is either to uncover glimpses of new particles or interactions at the LHC, or to derive the most stringent model-independent bounds to date on general theories of New Physics. Of particular interest are novel methods for charting the parameter space [2], the matching to UV-complete theories in explicit BSM scenarios [3], and the interplay between EFT-based model-independent searches for new physics and determinations of the proton structure from LHC data [4].

[1] https://arxiv.org/abs/1901.05965 [2] https://arxiv.org/abs/1906.05296 [3] https://arxiv.org/abs/1908.05588 [4] https://arxiv.org/abs/1905.05215

Contact: Juan Rojo

[edit] Theory: Charting the quark and gluon structure of protons and nuclei with Machine Learning

Deepening our knowledge of the partonic content of nucleons and nuclei [1] represents a central endeavour of modern high-energy and nuclear physics, with ramifications in related disciplines such as astroparticle physics. There are two main scientific drivers motivating these investigations of the partonic structure of hadrons. On the one hand, addressing fundamental open issues in our understanding in the strong interactions such as the origin of the nucleon mass, spin, and transverse structure; the presence of heavy quarks in the nucleon wave function; and the possible onset of novel gluon-dominated dynamical regimes. On the other hand, pinning down with the highest possible precision the substructure of nucleons and nuclei is a central component for theoretical predictions in a wide range of experiments, from proton and heavy ion collisions at the Large Hadron Collider to ultra-high energy neutrino interactions at neutrino telescopes. The goal of this project is to exploit Machine Learning and Artificial Intelligence tools [2,3] (neural networks trained by stochastic gradient descent) to pin down the quark and gluon substructure of protons and nuclei by using recent measurements from proton-proton and proton-lead collisions at the LHC. Topics of special interest are i) the strange content of protons and nuclei, ii) parton distributions at higher-orders in the QCD couplings for precision Higgs physics, iii) the interplay between jet, photon, and top quark production data to pin down the large-x gluon, and iv) charm quarks as a probe of gluon shadowing at small-x. The project also involves developing projects for the Electron-Ion Collider (EIC), a new lepton-nucleus experiment to start operations in the next years.

[1] https://arxiv.org/abs/1910.03408 [2] https://arxiv.org/abs/1904.00018 [3] https://arxiv.org/abs/1706.00428

Contact: Juan Rojo

[edit] Theory: Machine learning for Electron Microscopy for next-generation materials

Machine Learning tools developed and applied for particle physics hold great potential for applications in material science, in particular concerning faithful uncertainty estimation and model training for large parameter spaces. In this project, carried out in collaboration with the group of Dr. Sonia Conesa-Boj from the Kavli Institute Nanoscience Delft, http://www.conesabojlab.tudelft.nl, we will develop and deploy ML tools for data analysis in Electron Microscopy. We will focus on pinning down the properties of novel quantum materials such as topological insulators and van der Waals materials. Examples of possible applications include model-independent background subtraction in electron-energy loss spectroscopy, automatic classification of crystalline structures, and enhancing spatial and spectral resolution using convolutional networks.

Contact: Juan Rojo

[edit] Theory: The electroweak phase transition and baryogenesis/gravitational wave production

In extensions of the Standard Model the electroweak phase transition can be first order and proceed via the nucleation of bubbles. Colliding bubbles can produce gravitational waves [1] and plasma particles interacting with the bubbles can generate a matter-antimatter asymmetry [2]. A detailed understanding of the dynamics of the phase transitions is needed to accurately describe these processes. One project is to study QFT at finite temperature and compare/apply methods that address the non-perturbative IR dynamics of the thermal processes [3,4]. Another project is to calculate the velocity by which the bubbles expand, which is an important parameter for gravitational waves production and baryogensis. This entails among other things tunneling dymamics, (thermal) scattering rates and Boltzmann equations [5].

[1]https://arxiv.org/abs/1705.01783 [2]https://arxiv.org/pdf/hep-ph/0609145.pdf [3]https://arxiv.org/pdf/1609.06230.pdf [4]https://arxiv.org/pdf/1612.00466.pdf [5]https://arxiv.org/pdf/1809.04907.pdf

Contact: Marieke Postma

[edit] Theory: Cosmology of the QCD axion

The QCD axion provides an elegant solution to the strong CP problem in QCD[1]. This project focus on the cosmological dynamics of this hypothesized axion field, and in particular the possibility that it can both produce the observed matter-antimatter asymmetry and dark matter abundance in our universe [2,3].

[1]https://arxiv.org/abs/1812.02669 [2]https://arxiv.org/pdf/hep-ph/0609145.pdf [3]https://arxiv.org/pdf/1910.02080.pdf

Contact: Marieke Postma

[edit] Theory: Neutrinos, hierarchy problem and cosmology

The electroweak hierachy problem is absent if the quadratic term in the Higgs potential is generated dynamically. This is achieved in 'the neutrino option' [1] where the Higgs potential stems exclusively from quantum effects of heavy right-handed neutrinos, which can also generate the mass pattern of the oberved left-handed neutrinos. The project focusses on model building aspects (e.g. [2]) and the cosmology (e.g. leptogenesis [3]) of these set-ups.

[1] https://arxiv.org/pdf/1703.10924.pdf [2] https://arxiv.org/pdf/1807.11490.pdf [3] https://arxiv.org/pdf/1905.12642.pdf

Contact: Marieke Postma

[edit] KM3NeT: Reconstruction of first neutrino interactions in KM3NeT

The neutrino telescope KM3NeT is under construction in the Mediterranean Sea aiming to detect cosmic neutrinos. Its first few strings with sensitive photodetectors have been deployed at both the Italian and the French detector sites. Already these few strings provide for the option to reconstruct in the detector the abundant muons stemming from interactions of cosmic rays with the atmosphere and to identify neutrino interactions. In this project the available data will be used together with simulations to best reconstruct the event topologies and optimally identify and reconstruct the first neutrino interactions in the KM3NeT detector and with this pave the path towards accurate neutrino oscillation measurements and neutrino astronomy.

Programming skills are essential, mostly root and C++ will be used. Contact: Ronald Bruijn Dorothea Samtleben'

[edit] KM3NeT: Searching for New Heavy Neutrinos

In this project we will be searching for a new heavy neutrino, looking at signatures created by atmospheric neutrinos interacting in the detector volume of KM3NeT-ORCA. The aim of this project is to study a specific event topology which appears as double blobs of signals detected separately by densely instrumented ORCA detector units. We will be exploiting the tau reconstruction algorithms to verify the possibility of ORCA to detect such signals and to estimate the potential sensitivity of the experiment as well. Basic knowledge of elementary particle physics and data analysis techniques will be advantageous. The knowledge of programming languages e.g. python (and possibly C++) and ROOT are advantageous but not mandatory.

Contact: Suzan B. du Pree Daan van Eijk

[edit] KM3NeT: Dark Matter with KM3NeT-ORCA

Dark Matter is thought to be everywhere (we should be swimming through it), but we have no idea what it is. Using the good energy and angular resolutions of the KM3NeT neutrino telescope, we can search for Dark Matter signatures that originate from the center of our galaxy. In this project, we will search for such signatures using the reconstructed track and shower events with the KM3NeT-ORCA detector to discover relatively light Dark Matter particles. Since this year, the KM3NeT-ORCA experiment has 6 detection lines under the Mediterranean Sea: fully operational and continuously taking data. Using the available data, it is possible to compare data and simulation for different event topologies and to estimate the experiment's sensitivity. The project is suitable for a student who is interested to explore new physics scenarios and willing to develop new skills. Basic knowledge of elementary particle physics and data analysis techniques will be advantageous. The knowledge of programming languages e.g. python (possibly C++) and ROOT data analysis tool are advantageous but not mandatory.

Contact: Suzan B. du Pree Daan van Eijk


[edit] Gravitational Waves: Unraveling the structure of neutron stars with gravitational wave observations

Neutron stars were first discovered more than half a century ago, yet their detailed internal structure largely remains a mystery. A range of theoretical models have been put forward for the neutron star "equation of state", but until recently there was no real way to test them. The direct detection of gravitational waves with LIGO and Virgo has the potential to remedy the situation. When two neutron stars spiral towards each other, they get tidally deformed in a way that is determined by the equation of state, and these deformations get imprinted upon the shape of the gravitational wave that gets emitted. After the first gravitational wave observation of such an event in 2017, several equation of state models could already be ruled out. With expected upgrades of the detectors, we will at some point have access not only to the "inspiral" of binary neutron stars, but to the merger itself, and what happens afterwards. The project will consist of using results from large-scale numerical simulations to come up with a heuristic model for the waveform that describes the inspiral-merger-postmerger process with sufficient accuracy given expected detector sensitivities, and to develop data analysis techniques to efficiently use this model to extract information about the neutron star equation of state.

Contact: Chris Van Den Broeck


[edit] Gravitational Waves: Searches for gravitational waves from compact binary coalescence

Searches for gravitational waves from the mergers of black holes and neutron stars have been extraordinarily successful in the last four years. We are now beginning to study a population of heavy stellar-mass black holes in detail, including understanding how these systems came to form and whether they are consistent with general relativity. Additionally, the detection of binary neutron star mergers is allowing us to probe their extreme matter. However, we’ve only just scratched the surface of possible signals and the new physics they’d allow us to study. The detection of highly spinning and precessing systems would allow us to perform black hole population statistics to an extraordinary degree of accuracy. Detection of sub-solar mass systems would provide evidence of dark matter. However, these searches are difficult because they require us to work in high-dimensional spaces and develop new statistical methods. There are possibilities for several projects that involve the development and implementation of these new searches as well as the interpretation of the results, particularly in terms of the physics describing compact binary mergers.

Contact: Sarah Caudill


[edit] Gravitational Waves: Computer modelling to design the laser interferometers for the Einstein telescope

A new field of instrument science led to the successful detection of gravitational waves by the LIGO detectors in 2015. We are now preparing the next generation of gravitational wave observatories, such as the Einstein Telescope, with the aim to increase the detector sensitivity by a factor of ten, which would allow, for example, to detect stellar-mass black holes from early in the universe when the first stars began to form. This ambitious goal requires us to find ways to significantly improve the best laser interferometers in the world.

Gravitational wave detectors, such as LIGO and VIRGO, are complex Michelson-type interferometers enhanced with optical cavities. We develop and use numerical models to study these laser interferometers, to invent new optical techniques and to quantify their performance. For example, we synthesize virtual mirror surfaces to study the effects of higher-order optical modes in the interferometers, and we use opto-mechanical models to test schemes for suppressing quantum fluctuations of the light field. We can offer several projects based on numerical modelling of laser interferometers. All projects will be directly linked to the ongoing design of the Einstein Telescope.

Contact: Andreas Freise


[edit] Gravitational Waves: Digging away the noise to find the signal

Gravitational Wave interferometers are extremely sensitive, but suffer from instrumental issues that produce noise that mimics astrophysical signals. This needs to be solved as much as possible before the data analysis. The problem is that instrumentalists don't know about analysis pipelines, and data analysts don't know about experimental details. We need your help to bridge the gap. This is a good opportunity to learn about both sides and contribute directly to a booming international field. We have several tools and new ideas for correlating noises with the state of the instrument. These need to be developed further, used on years of data, and written up. Will require Python, signal processing and statistics.

Contact: Bas Swinkels and Sarah Caudill


[edit] Gravitational Waves: Machine Learning techniques for GW Interferometers

The control of suspended optical cavities in the non linear regime. Gravitational Wave interferometers are extremely sensitive, however suffer from a very small control range, causing unlocks, reducing the robustness of these instruments. In this project we will use a table top replica of a suspended optical cavity, located in the new R&D laser lab at Nikhef, for the development of a neural network to construct the positions from free falling mirror by using beam images. A database with simulated beam images can be used to train various neural networks before deployment in the table top experiment. We are looking for a hands-on and enthusiastic master student, interested in machine learning and experienced in programming languages like Python. Contacts: Rob Walet, Frank Linde

Contact: Rob Walet and Frank Linde

[edit] VU LaserLaB: Measuring the electric dipole moment (EDM) of the electron

In collaboration with Nikhef and the Van Swinderen Institute for Particle Physics and Gravity at the University of Groningen, we have recently started an exciting project to measure the electric dipole moment (EDM) of the electron in cold beams of barium-fluoride molecules. The eEDM, which is predicted by the Standard Model of particle physics to be extremely small, is a powerful probe to explore physics beyond this Standard Model. All extensions to the Standard Model, most prominently supersymmetry, naturally predict an electron EDM that is just below the current experimental limits. We aim to improve on the best current measurement by at least an order of magnitude. To do so we will perform a precision measurement on a slow beam of laser-cooled BaF molecules. With this low-energy precision experiment, we test physics at energies comparable to those of LHC!

At LaserLaB VU, we are responsible for building and testing a cryogenic source of BaF molecules. The main parts of this source are currently being constructed in the workshop. We are looking for enthusiastic master students to help setup the laser system that will be used to detect BaF. Furthermore, projects are available to perform simulations of trajectory simulations to design a lens system that guides the BaF molecules from the exit of the cryogenic source to the experiment.

Contact: Rick Bethlem

[edit] VU LaserLaB: Physics beyond the Standard model from molecules

Our team, with a number of staff members (Ubachs, Eikema, Salumbides, Bethlem, Koelemeij) focuses on precision measurements in the hydrogen molecule, and its isotopomers. The work aims at testing the QED calculations of energy levels in H2, D2, T2, HD, etc. with the most precise measurements, where all kind of experimental laser techniques play a role (cw and pulsed lasers, atomic clocks, frequency combs, molecular beams). Also a target of studies is the connection to the "Proton size puzzle", which may be solved through studies in the hydrogen molecular isotopes.

In the past half year we have produced a number of important results that are described in the following papers:

  • Frequency comb (Ramsey type) electronic excitations in the H2 molecule:

see: Deep-ultraviolet frequency metrology of H2 for tests of molecular quantum theory http://www.nat.vu.nl/~wimu/Publications/Altmann-PRL-2018.pdf

  • Precision measurement of an infrared transition in the HD molecule

see: Sub-Doppler frequency metrology in HD for tests of fundamental physics: https://arxiv.org/abs/1712.08438

  • The first precision study in molecular tritium T2

see: Relativistic and QED effects in the fundamental vibration of T2: http://arxiv.org/abs/1803.03161

  • Dissociation energy of the hydrogen molecule at 10^-9 accuracy paper submitted to Phys. Rev. Lett.
  • Probing QED and fundamental constants through laser spectroscopy of vibrational transitions in HD+

This is also a study of the hydrogen molecular ion HD+, where important results were obtained not so long ago, and where we have a strong activity: http://www.nat.vu.nl/~wimu/Publications/ncomms10385.pdf

These five results mark the various directions we are pursuing, and in all directions we aim at obtaining improvements. Specific projects with students can be defined; those are mostly experimental, although there might be some theoretical tasks, like performing calculations of hyperfine structures. Contact: Wim Ubachs Kjeld Eikema Rick Bethlem


Last year's MSc Projects

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