Coscattering in next-to-minimal dark matter and split supersymmetry

Abstract In some models of thermal relic dark matter, the relic abundance may be set by inelastic scattering processes (rather than annihilations) becoming inefficient as the universe cools down. This effect has been called coscattering. We present a procedure to numerically solve the full momentum-...

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Main Author: F. Brümmer
Format: Article
Language:English
Published: SpringerOpen 2020-01-01
Series:Journal of High Energy Physics
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Online Access:https://doi.org/10.1007/JHEP01(2020)113
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author F. Brümmer
author_facet F. Brümmer
author_sort F. Brümmer
collection DOAJ
description Abstract In some models of thermal relic dark matter, the relic abundance may be set by inelastic scattering processes (rather than annihilations) becoming inefficient as the universe cools down. This effect has been called coscattering. We present a procedure to numerically solve the full momentum-dependent Boltzmann equations in coscattering, which allows for a precise calculation of the dark matter relic density including the effects of early kinetic decoupling. We apply our method to a simple model, containing a fermionic SU(2) triplet and a fermionic singlet with electroweak-scale masses, at small triplet-singlet mixing. The relic density can be set by either coannihilation or, at values of the mixing angle θ ≲ 10−5, by coscattering. We identify the parameter ranges which give rise to the observed relic abundance. As a special case, we study bino-like dark matter in split supersymmetry at large μ.
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spelling doaj-art-b7a6b49364ce475987e95122e9f5a5642025-01-26T12:11:12ZengSpringerOpenJournal of High Energy Physics1029-84792020-01-012020112010.1007/JHEP01(2020)113Coscattering in next-to-minimal dark matter and split supersymmetryF. Brümmer0LUPM, UMR5299, Université de Montpellier and CNRSAbstract In some models of thermal relic dark matter, the relic abundance may be set by inelastic scattering processes (rather than annihilations) becoming inefficient as the universe cools down. This effect has been called coscattering. We present a procedure to numerically solve the full momentum-dependent Boltzmann equations in coscattering, which allows for a precise calculation of the dark matter relic density including the effects of early kinetic decoupling. We apply our method to a simple model, containing a fermionic SU(2) triplet and a fermionic singlet with electroweak-scale masses, at small triplet-singlet mixing. The relic density can be set by either coannihilation or, at values of the mixing angle θ ≲ 10−5, by coscattering. We identify the parameter ranges which give rise to the observed relic abundance. As a special case, we study bino-like dark matter in split supersymmetry at large μ.https://doi.org/10.1007/JHEP01(2020)113Cosmology of Theories beyond the SMSupersymmetric Standard Model
spellingShingle F. Brümmer
Coscattering in next-to-minimal dark matter and split supersymmetry
Journal of High Energy Physics
Cosmology of Theories beyond the SM
Supersymmetric Standard Model
title Coscattering in next-to-minimal dark matter and split supersymmetry
title_full Coscattering in next-to-minimal dark matter and split supersymmetry
title_fullStr Coscattering in next-to-minimal dark matter and split supersymmetry
title_full_unstemmed Coscattering in next-to-minimal dark matter and split supersymmetry
title_short Coscattering in next-to-minimal dark matter and split supersymmetry
title_sort coscattering in next to minimal dark matter and split supersymmetry
topic Cosmology of Theories beyond the SM
Supersymmetric Standard Model
url https://doi.org/10.1007/JHEP01(2020)113
work_keys_str_mv AT fbrummer coscatteringinnexttominimaldarkmatterandsplitsupersymmetry