Indirect search for dark matter with micrOMEGAs_2.4

Abstract
We present a new module of micrOMEGAs devoted to the computation of indirect signals from dark matter annihilation in any new model with a stable weakly interacting particle. The code provides the mass spectrum, cross-sections, relic density and exotic fluxes of gamma rays, positrons and antiprotons. The propagation of charged particles in the Galactic halo is handled with a new module that allows to easily modify the propagation parameters.

Title of program: micrOMEGAs2.4
Catalogue Id: ADQR_v2_3

Nature of problem
Calculation of the relic density and detection rates of the lightest stable particle in a generic new model of particle physics.

Versions of this program held in the CPC repository in Mendeley Data
ADQR_v1_0; micrOMEGAs; 10.1016/S0010-4655(02)00596-9
ADQR_v1_3; micrOMEGAs1.3; 10.1016/j.cpc.2005.12.005
ADQR_v2_0; micrOMEGAs2.0; 10.1016/j.cpc.2006.11.008
ADQR_v2_1; micrOMEGAs2.1; 10.1016/j.cpc.2007.08.002
ADQR_v2_2; micrOMEGAs2.2; 10.1016/j.cpc.2008.11.019
ADQR_v2_3; micrOMEGAs2.4; 10.1016/j.cpc.2010.11.033
ADQR_v3_0; micrOMEGAs3; 10.1016/j.cpc.2013.10.016
ADQR_v4_0; MicrOMEGAs4.1; 10.1016/j.cpc.2015.03.003

This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)