Ultraviolet running constraints on low mass dark sectors
Abstract We analyze the UV breakdown of Sub-GeV dark matter models that live in a new, dark U(1) sector. Many of these models include a scalar field, which is either the dark matter itself or a dark Higgs field that generates mass terms for the dark matter particle via spontaneous symmetry breaking....
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Format: | Article |
Language: | English |
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SpringerOpen
2024-01-01
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Series: | Journal of High Energy Physics |
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Online Access: | https://doi.org/10.1007/JHEP01(2024)089 |
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author | Aidan Reilly Natalia Toro |
author_facet | Aidan Reilly Natalia Toro |
author_sort | Aidan Reilly |
collection | DOAJ |
description | Abstract We analyze the UV breakdown of Sub-GeV dark matter models that live in a new, dark U(1) sector. Many of these models include a scalar field, which is either the dark matter itself or a dark Higgs field that generates mass terms for the dark matter particle via spontaneous symmetry breaking. A quartic self coupling of this scalar field is generically allowed, and we show that its running is largely governed by the strength of the U(1) gauge field, α D . Furthermore, it consistently has a lower Landau pole than the gauge coupling. Link fields, which couple to both the dark sector and the Standard Model (SM), connect these Landau poles to constraints on SM charged particles. Current LHC constraints on link fields are compatible with α D ≲ 0.5 − 1 for most of the mass range in most models, while smaller values, α D ≲ 0.15, are favored for Majorana DM. |
first_indexed | 2024-03-08T12:41:33Z |
format | Article |
id | doaj.art-a7f0faaa3e9c4f2398c18d856746be0a |
institution | Directory Open Access Journal |
issn | 1029-8479 |
language | English |
last_indexed | 2024-03-08T12:41:33Z |
publishDate | 2024-01-01 |
publisher | SpringerOpen |
record_format | Article |
series | Journal of High Energy Physics |
spelling | doaj.art-a7f0faaa3e9c4f2398c18d856746be0a2024-01-21T12:07:42ZengSpringerOpenJournal of High Energy Physics1029-84792024-01-012024113110.1007/JHEP01(2024)089Ultraviolet running constraints on low mass dark sectorsAidan Reilly0Natalia Toro1SLAC National Accelerator LaboratorySLAC National Accelerator LaboratoryAbstract We analyze the UV breakdown of Sub-GeV dark matter models that live in a new, dark U(1) sector. Many of these models include a scalar field, which is either the dark matter itself or a dark Higgs field that generates mass terms for the dark matter particle via spontaneous symmetry breaking. A quartic self coupling of this scalar field is generically allowed, and we show that its running is largely governed by the strength of the U(1) gauge field, α D . Furthermore, it consistently has a lower Landau pole than the gauge coupling. Link fields, which couple to both the dark sector and the Standard Model (SM), connect these Landau poles to constraints on SM charged particles. Current LHC constraints on link fields are compatible with α D ≲ 0.5 − 1 for most of the mass range in most models, while smaller values, α D ≲ 0.15, are favored for Majorana DM.https://doi.org/10.1007/JHEP01(2024)089Models for Dark MatterNew Gauge InteractionsDark Matter at CollidersNew Light Particles |
spellingShingle | Aidan Reilly Natalia Toro Ultraviolet running constraints on low mass dark sectors Journal of High Energy Physics Models for Dark Matter New Gauge Interactions Dark Matter at Colliders New Light Particles |
title | Ultraviolet running constraints on low mass dark sectors |
title_full | Ultraviolet running constraints on low mass dark sectors |
title_fullStr | Ultraviolet running constraints on low mass dark sectors |
title_full_unstemmed | Ultraviolet running constraints on low mass dark sectors |
title_short | Ultraviolet running constraints on low mass dark sectors |
title_sort | ultraviolet running constraints on low mass dark sectors |
topic | Models for Dark Matter New Gauge Interactions Dark Matter at Colliders New Light Particles |
url | https://doi.org/10.1007/JHEP01(2024)089 |
work_keys_str_mv | AT aidanreilly ultravioletrunningconstraintsonlowmassdarksectors AT nataliatoro ultravioletrunningconstraintsonlowmassdarksectors |