Introduction In the last 30 years we have made great progress both ...

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MicrOMEGAs uses CalcHEP to generate codes for matrixelements. It makes micrOMEGAs flexible for new modelimplementation.MicrOMEGAs is written in C but user program can be writtenin C, C++, FORTRANPlatforms are Linux, MacOther code for DM business:DarkSUSY: http://www.physto.se/~edsjo/darksusySuperISO : http://superiso.in2p3.frIsaJet : http://www.nhn.ou.edu/~isajetThere is a good agreement between these codes.8
To Downloadhttp://lapth.in2p3.fr/micromegasThe name of file should bemicromegas_2.4.X.tgzUnpack it bytar -xvzf micromegas_2.4.X.tgzIt should create directory micromegas_2.4.X/ which occupies about 40Mb of disk space. You will need more disk space after compilation of specificmodels and generation of matrix elements .In case of problems and questionsemail: micro.omegas@lapp.in2p3.frFor current lecture downloadhttp://theory.sinp.msu.ru/~pukhov/micromegas_2.2.tgz9
Page 1 and 2: MicrOMEGAs - a package for calculat
Page 3 and 4: Massive Stable ParticleTo describe
Page 5 and 6: In the framework of a given model o
Page 7: C) Solar neutrinos. In some sense t
Page 11 and 12: Compilation of CalcHEP and micromeg
Page 13 and 14: Module structure of main programs.m
Page 15 and 16: Parameters of main programs.Default
Page 17 and 18: ==== Physical Constraints: =====del
Page 19 and 20: Free parameters of the model.Free m
Page 21 and 22: Constrained parameter of the model.
Page 23 and 24: err = sortOddParticles( stext)This
Page 25 and 26: Shared libraries of matrix elements
Page 27 and 28: Calculation of particle widths in m
Page 29 and 30: Coannihilation and Beps parameterAs
Page 31 and 32: We define abundance Y=N/s to remove
Page 33 and 34: Ω = M cdm [GeV] * Y * (2.889 10 9
Page 36 and 37: vSigma[pb] & Yeqfor MSUGRA modelM0

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