SIMP dark matter and its cosmic abundances

We give a review on the thermal average of the annihilation cross-sections for 3 → 2 and general higher-order processes. Thermal average of higher order annihilations highly depend on the velocity of dark matter, especially, for the case with resonance poles. We show such examples for scalar dark ma...

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Main Authors: Choi Soo-Min, Lee Hyun Min, Seo Min-Seok
Format: Article
Language:English
Published: EDP Sciences 2018-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201816806009
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spelling doaj-74afe80186994b8f880ab7d0c2dbdcb62021-08-02T06:18:00ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011680600910.1051/epjconf/201816806009epjconf_icgaxiii-ik2018_06009SIMP dark matter and its cosmic abundancesChoi Soo-MinLee Hyun MinSeo Min-SeokWe give a review on the thermal average of the annihilation cross-sections for 3 → 2 and general higher-order processes. Thermal average of higher order annihilations highly depend on the velocity of dark matter, especially, for the case with resonance poles. We show such examples for scalar dark matter in gauged Z3 models.https://doi.org/10.1051/epjconf/201816806009
collection DOAJ
language English
format Article
sources DOAJ
author Choi Soo-Min
Lee Hyun Min
Seo Min-Seok
spellingShingle Choi Soo-Min
Lee Hyun Min
Seo Min-Seok
SIMP dark matter and its cosmic abundances
EPJ Web of Conferences
author_facet Choi Soo-Min
Lee Hyun Min
Seo Min-Seok
author_sort Choi Soo-Min
title SIMP dark matter and its cosmic abundances
title_short SIMP dark matter and its cosmic abundances
title_full SIMP dark matter and its cosmic abundances
title_fullStr SIMP dark matter and its cosmic abundances
title_full_unstemmed SIMP dark matter and its cosmic abundances
title_sort simp dark matter and its cosmic abundances
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2018-01-01
description We give a review on the thermal average of the annihilation cross-sections for 3 → 2 and general higher-order processes. Thermal average of higher order annihilations highly depend on the velocity of dark matter, especially, for the case with resonance poles. We show such examples for scalar dark matter in gauged Z3 models.
url https://doi.org/10.1051/epjconf/201816806009
work_keys_str_mv AT choisoomin simpdarkmatteranditscosmicabundances
AT leehyunmin simpdarkmatteranditscosmicabundances
AT seominseok simpdarkmatteranditscosmicabundances
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