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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Main Authors: Aidan Reilly, Natalia Toro
Format: Article
Language:English
Published: SpringerOpen 2024-01-01
Series:Journal of High Energy Physics
Subjects:
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.
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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