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

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==== Indirect detection =======Channelvcs[cm^3/s]~o1,~o1 > b B 2.25E29~o1,~o1 > t T 2.55E29~o1,~o1 > l L 5.37E29~o1,~o1 > W+ W 2.95E31~o1,~o1 > l L 5.37E29~o1,~o1 > t T 2.55E29~o1,~o1 > b B 2.25E29~o1,~o1 > W+ W 2.95E31sigmav=1.02E28[cm^3/s]Photon flux for angle of sight f=0.00[rad]and spherical region described by cone with angle 0.0349[rad]Photon flux = 7.53E16[cm^2 s GeV]^{1} for E=103.0[GeV]Positron flux = 3.50E14[cm^2 sr s GeV]^{1} for E=103.0[GeV]Antiproton flux = 1.99E15[cm^2 sr s GeV]^{1} for E=103.0[GeV]==== Calculation of CDMnucleons amplitudes =====CDMnucleon micrOMEGAs amplitudes:proton: SI 1.316E09 SD 1.575E08neutron: SI 1.333E09 SD 1.984E08CDMnucleon cross sections[pb]:proton SI 7.502E10 SD 3.223E07neutron SI 7.696E10 SD 5.113E0718
Free parameters of the model.Free model parameters are presented in MODEL/work/models/vars1.mdlFor example:Inert Doublet ModelVariablesName | Value |> Comment
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 and 8: C) Solar neutrinos. In some sense t
Page 9 and 10: To Downloadhttp://lapth.in2p3.fr/mi
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: ==== Physical Constraints: =====del
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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