Dark QCD matters

Abstract We investigate the nightmare scenario of dark sectors that are made of non-abelian gauge theories with fermions, gravitationally coupled to the Standard Model (SM). While testing these scenarios is experimentally challenging, they are strongly motivated by the accidental stability of dark b...

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Main Authors: Raghuveer Garani, Michele Redi, Andrea Tesi
Format: Article
Language:English
Published: SpringerOpen 2021-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2021)139
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author Raghuveer Garani
Michele Redi
Andrea Tesi
author_facet Raghuveer Garani
Michele Redi
Andrea Tesi
author_sort Raghuveer Garani
collection DOAJ
description Abstract We investigate the nightmare scenario of dark sectors that are made of non-abelian gauge theories with fermions, gravitationally coupled to the Standard Model (SM). While testing these scenarios is experimentally challenging, they are strongly motivated by the accidental stability of dark baryons and pions, that explain the cosmological stability of dark matter (DM). We study the production of these sectors which are minimally populated through gravitational freeze-in, leading to a dark sector temperature much lower than the SM, or through inflaton decay, or renormalizable interactions producing warmer DM. Despite having only gravitational couplings with the SM these scenarios turn out to be rather predictive depending roughly on three parameters: the dark sector temperature, the confinement scale and the dark pion mass. In particular, when the initial temperature is comparable to the SM one these scenarios are very constrained by structure formation, ∆N eff and limits on DM self-interactions. Dark sectors with same temperature or warmer than SM are typically excluded.
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spelling doaj.art-857e72b42b5e404085a65419dd5b34dd2022-12-21T18:43:07ZengSpringerOpenJournal of High Energy Physics1029-84792021-12-0120211213210.1007/JHEP12(2021)139Dark QCD mattersRaghuveer Garani0Michele Redi1Andrea Tesi2INFN Sezione di FirenzeINFN Sezione di FirenzeINFN Sezione di FirenzeAbstract We investigate the nightmare scenario of dark sectors that are made of non-abelian gauge theories with fermions, gravitationally coupled to the Standard Model (SM). While testing these scenarios is experimentally challenging, they are strongly motivated by the accidental stability of dark baryons and pions, that explain the cosmological stability of dark matter (DM). We study the production of these sectors which are minimally populated through gravitational freeze-in, leading to a dark sector temperature much lower than the SM, or through inflaton decay, or renormalizable interactions producing warmer DM. Despite having only gravitational couplings with the SM these scenarios turn out to be rather predictive depending roughly on three parameters: the dark sector temperature, the confinement scale and the dark pion mass. In particular, when the initial temperature is comparable to the SM one these scenarios are very constrained by structure formation, ∆N eff and limits on DM self-interactions. Dark sectors with same temperature or warmer than SM are typically excluded.https://doi.org/10.1007/JHEP12(2021)139Beyond Standard ModelCosmology of Theories beyond the SM
spellingShingle Raghuveer Garani
Michele Redi
Andrea Tesi
Dark QCD matters
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
title Dark QCD matters
title_full Dark QCD matters
title_fullStr Dark QCD matters
title_full_unstemmed Dark QCD matters
title_short Dark QCD matters
title_sort dark qcd matters
topic Beyond Standard Model
Cosmology of Theories beyond the SM
url https://doi.org/10.1007/JHEP12(2021)139
work_keys_str_mv AT raghuveergarani darkqcdmatters
AT micheleredi darkqcdmatters
AT andreatesi darkqcdmatters