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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EDP Sciences
2018-01-01
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Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201816806009 |
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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 |
_version_ |
1721240400583196672 |