Difference between revisions of "MSUGRA scan"
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== Checking one susy point == | == Checking one susy point == | ||
− | The macro susygen.py checkes the compatibility of one specific SUSY point to a certain number of individual constraints. The results of these constaints are written to file. susygen.py is called with: susygen.py <m0> <m12> <A0> <tan(beta)> <sign(mu)> <name resultfile> | + | The macro susygen.py checkes the compatibility of one specific SUSY point to a certain number of individual constraints. The results of these constaints are written to file. susygen.py is called with: susygen.py <m0> <m12> <A0> <tan(beta)> <sign(mu)> <name resultfile>. masses should be given in GeV. |
− | + | Under current form 13 number are written to the result file, in the following order: <m0> <m12> <A0> <tan(beta)> <sign(mu)> <theory> <mass neutralino> <mass higgs> <LSP> <BR(B->s gamma)> <relic dencity (omega h^2)> <BR(Bs->mu mu)> The masses are given in GeV. | |
− | The | + | The value for theory is 0 if the susypoint is theoretically allowed and 1 otherwise. This can easily be changed to give different values for different theoretical constraints. |
− | The | + | The value for LSP is equal to the particle number (as used by HERWIG) of the lightest superpartner. 450 = neutralino, 429 = stau. |
Revision as of 15:47, 24 January 2008
Main goal
The macros on this page can be used to scan any part of the mSUGRA phacespace to determine wich part of the phacespace is still currently allowed by both experiment and theory.
Checking one susy point
The macro susygen.py checkes the compatibility of one specific SUSY point to a certain number of individual constraints. The results of these constaints are written to file. susygen.py is called with: susygen.py <m0> <m12> <A0> <tan(beta)> <sign(mu)> <name resultfile>. masses should be given in GeV.
Under current form 13 number are written to the result file, in the following order: <m0> <m12> <A0> <tan(beta)> <sign(mu)> <theory> <mass neutralino> <mass higgs> <LSP> <BR(B->s gamma)> <relic dencity (omega h^2)> <BR(Bs->mu mu)> The masses are given in GeV.
The value for theory is 0 if the susypoint is theoretically allowed and 1 otherwise. This can easily be changed to give different values for different theoretical constraints.
The value for LSP is equal to the particle number (as used by HERWIG) of the lightest superpartner. 450 = neutralino, 429 = stau.