Forbidden scalar dark matter and dark Higgses

Abstract As experimental searches for WIMP dark matter continue to yield null results, models beyond the WIMP paradigm have proliferated in order to elude ever improving observational constraints, among them that of sub-GeV dark matter mediated by a massive vector portal (a dark photon) associated w...

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Main Authors: George N. Wojcik, Thomas G. Rizzo
Format: Article
Language:English
Published: SpringerOpen 2022-04-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP04(2022)033
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author George N. Wojcik
Thomas G. Rizzo
author_facet George N. Wojcik
Thomas G. Rizzo
author_sort George N. Wojcik
collection DOAJ
description Abstract As experimental searches for WIMP dark matter continue to yield null results, models beyond the WIMP paradigm have proliferated in order to elude ever improving observational constraints, among them that of sub-GeV dark matter mediated by a massive vector portal (a dark photon) associated with a new dark U(1) gauge symmetry. It has been previously noted that for a significant range of the parameter space of this class of models, the annihilation of dark matter particles into a pair of dark photons can dominate the freeze-out process even when this process is kinematically forbidden for dark matter at rest — this is known as the “forbidden dark matter” (FDM) regime. Prior studies of this regime, however, assume that any “dark Higgs” associated with breaking the dark U(1) and imparting mass to the dark photon is decoupled from the dark matter and as such plays no role in the freeze-out process. In this paper, we explore the effects of a dark Higgs on sub-GeV dark matter phenomenology in this FDM regime by considering the simplest possible construction in which there exist non-trivial dark matter-dark Higgs couplings: a model with a single complex scalar DM candidate coupled directly to the dark Higgs field. We find that for a wide range of parameter space, the dark Higgs can alter the resulting relic abundance by many orders of magnitude, and that this effect can remain significant even for a small dark matter-dark Higgs coupling constant. Considering measurements from direct detection and measurements of the CMB, we further find that points in this model’s parameter space which recreate the appropriate dark matter relic abundance suffer only mild constraints from other sources at present, but may become accessible in near-future direct detection experiments.
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spelling doaj.art-a7e127420e014be58ddf09b441ec7f2b2023-03-22T10:11:34ZengSpringerOpenJournal of High Energy Physics1029-84792022-04-012022413710.1007/JHEP04(2022)033Forbidden scalar dark matter and dark HiggsesGeorge N. Wojcik0Thomas G. Rizzo1SLAC National Accelerator LaboratorySLAC National Accelerator LaboratoryAbstract As experimental searches for WIMP dark matter continue to yield null results, models beyond the WIMP paradigm have proliferated in order to elude ever improving observational constraints, among them that of sub-GeV dark matter mediated by a massive vector portal (a dark photon) associated with a new dark U(1) gauge symmetry. It has been previously noted that for a significant range of the parameter space of this class of models, the annihilation of dark matter particles into a pair of dark photons can dominate the freeze-out process even when this process is kinematically forbidden for dark matter at rest — this is known as the “forbidden dark matter” (FDM) regime. Prior studies of this regime, however, assume that any “dark Higgs” associated with breaking the dark U(1) and imparting mass to the dark photon is decoupled from the dark matter and as such plays no role in the freeze-out process. In this paper, we explore the effects of a dark Higgs on sub-GeV dark matter phenomenology in this FDM regime by considering the simplest possible construction in which there exist non-trivial dark matter-dark Higgs couplings: a model with a single complex scalar DM candidate coupled directly to the dark Higgs field. We find that for a wide range of parameter space, the dark Higgs can alter the resulting relic abundance by many orders of magnitude, and that this effect can remain significant even for a small dark matter-dark Higgs coupling constant. Considering measurements from direct detection and measurements of the CMB, we further find that points in this model’s parameter space which recreate the appropriate dark matter relic abundance suffer only mild constraints from other sources at present, but may become accessible in near-future direct detection experiments.https://doi.org/10.1007/JHEP04(2022)033Beyond Standard ModelCosmology of Theories beyond the SM
spellingShingle George N. Wojcik
Thomas G. Rizzo
Forbidden scalar dark matter and dark Higgses
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
title Forbidden scalar dark matter and dark Higgses
title_full Forbidden scalar dark matter and dark Higgses
title_fullStr Forbidden scalar dark matter and dark Higgses
title_full_unstemmed Forbidden scalar dark matter and dark Higgses
title_short Forbidden scalar dark matter and dark Higgses
title_sort forbidden scalar dark matter and dark higgses
topic Beyond Standard Model
Cosmology of Theories beyond the SM
url https://doi.org/10.1007/JHEP04(2022)033
work_keys_str_mv AT georgenwojcik forbiddenscalardarkmatteranddarkhiggses
AT thomasgrizzo forbiddenscalardarkmatteranddarkhiggses