micrOMEGAs2.0: a program to calculate the relic density of dark matter in a generic model

dc.creatorBelanger, G.
dc.creatorBoudjema, F.
dc.creatorPukhov, A.
dc.creatorSemenov, A.
dc.date2006-07-05
dc.date.accessioned2026-07-07T11:27:01Z
dc.date.available2026-07-07T11:27:01Z
dc.descriptionmicrOMEGAs2.0 is a code which calculates the relic density of a stable massive particle in an arbitrary model. The underlying assumption is that there is a conservation law like R-parity in supersymmetry which guarantees the stability of the lightest odd particle. The new physics model must be incorporated in the notation of CalcHEP, a package for the automatic generation of squared matrix elements. Once this is done, all annihilation and coannihilation channels are included automatically in any model. Cross-sections at $v=0$, relevant for indirect detection of dark matter, are also computed automatically. The package includes three sample models: the minimal supersymmetric standard model (MSSM), the MSSM with complex phases and the NMSSM. Extension to other models, including non supersymmetric models, is described.
dc.description23 pages
dc.identifierhttps://arxiv.org/abs/hep-ph/0607059
dc.identifierhttp://arxiv.org/abs/hep-ph/0607059
dc.identifierComput.Phys.Commun.176:367-382,2007
dc.identifierdoi:10.1016/j.cpc.2006.11.008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196017
dc.subjectHigh Energy Physics - Phenomenology
dc.titlemicrOMEGAs2.0: a program to calculate the relic density of dark matter in a generic model
dc.typetext

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