Indirect search for dark matter with micrOMEGAs_2.4

Published: 01-03-2011| Version 1 | DOI: 10.17632/cbkj3xxy85.1
Contributors:
Genevieve Belanger,
F. Boudjema,
P. Brun,
A. Pukhov,
S. Rosier-Lees,
P. Salati,
A. Semenov

Description

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)

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