Dark matter bound state formation via emission of a charged scalar

Abstract The formation of stable or meta-stable bound states can dramatically affect the phenomenology of dark matter (DM). Although the capture into bound states via emission of a vector is known to be significant, the capture via scalar emission suffers from cancellations that render it important...

Full description

Bibliographic Details
Main Authors: Ruben Oncala, Kalliopi Petraki
Format: Article
Language:English
Published: SpringerOpen 2020-02-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP02(2020)036
_version_ 1818676731300544512
author Ruben Oncala
Kalliopi Petraki
author_facet Ruben Oncala
Kalliopi Petraki
author_sort Ruben Oncala
collection DOAJ
description Abstract The formation of stable or meta-stable bound states can dramatically affect the phenomenology of dark matter (DM). Although the capture into bound states via emission of a vector is known to be significant, the capture via scalar emission suffers from cancellations that render it important only within narrow parameter space. While this is true for neutral scalar mediators, here we show that bound-state formation via emission of a charged scalar can be extremely significant. To this end, we consider DM charged under a dark U(1) force and coupled also to a light complex scalar that is charged under the same gauge symmetry. We compute the cross-sections for bound-state formation via emission of the charged scalar, and show that they can exceed those for capture via vector emission, as well as annihilation, by orders of magnitude. This holds even for very small values of the DM coupling to the charged scalar, and remains true in the limit of global symmetry. We then compute the DM thermal freeze-out, and find that the capture into meta-stable bound states via emission of a charged scalar can cause a late period of significant DM depletion. Our results include analytical expressions in the Coulomb limit, and are readily generalisable to non-Abelian interactions. We expect them to have implications for Higgs-portal scenarios of multi-TeV WIMP DM, as well as scenarios that feature dark Higgses or (darkly-)charged inert scalars, including models of self-interacting DM.
first_indexed 2024-12-17T08:48:08Z
format Article
id doaj.art-d324d3110760483ba18a2aca1d564801
institution Directory Open Access Journal
issn 1029-8479
language English
last_indexed 2024-12-17T08:48:08Z
publishDate 2020-02-01
publisher SpringerOpen
record_format Article
series Journal of High Energy Physics
spelling doaj.art-d324d3110760483ba18a2aca1d5648012022-12-21T21:56:09ZengSpringerOpenJournal of High Energy Physics1029-84792020-02-012020214010.1007/JHEP02(2020)036Dark matter bound state formation via emission of a charged scalarRuben Oncala0Kalliopi Petraki1NikhefNikhefAbstract The formation of stable or meta-stable bound states can dramatically affect the phenomenology of dark matter (DM). Although the capture into bound states via emission of a vector is known to be significant, the capture via scalar emission suffers from cancellations that render it important only within narrow parameter space. While this is true for neutral scalar mediators, here we show that bound-state formation via emission of a charged scalar can be extremely significant. To this end, we consider DM charged under a dark U(1) force and coupled also to a light complex scalar that is charged under the same gauge symmetry. We compute the cross-sections for bound-state formation via emission of the charged scalar, and show that they can exceed those for capture via vector emission, as well as annihilation, by orders of magnitude. This holds even for very small values of the DM coupling to the charged scalar, and remains true in the limit of global symmetry. We then compute the DM thermal freeze-out, and find that the capture into meta-stable bound states via emission of a charged scalar can cause a late period of significant DM depletion. Our results include analytical expressions in the Coulomb limit, and are readily generalisable to non-Abelian interactions. We expect them to have implications for Higgs-portal scenarios of multi-TeV WIMP DM, as well as scenarios that feature dark Higgses or (darkly-)charged inert scalars, including models of self-interacting DM.https://doi.org/10.1007/JHEP02(2020)036Beyond Standard ModelCosmology of Theories beyond the SMNonperturbative Effects
spellingShingle Ruben Oncala
Kalliopi Petraki
Dark matter bound state formation via emission of a charged scalar
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
Nonperturbative Effects
title Dark matter bound state formation via emission of a charged scalar
title_full Dark matter bound state formation via emission of a charged scalar
title_fullStr Dark matter bound state formation via emission of a charged scalar
title_full_unstemmed Dark matter bound state formation via emission of a charged scalar
title_short Dark matter bound state formation via emission of a charged scalar
title_sort dark matter bound state formation via emission of a charged scalar
topic Beyond Standard Model
Cosmology of Theories beyond the SM
Nonperturbative Effects
url https://doi.org/10.1007/JHEP02(2020)036
work_keys_str_mv AT rubenoncala darkmatterboundstateformationviaemissionofachargedscalar
AT kalliopipetraki darkmatterboundstateformationviaemissionofachargedscalar