The Axion-Higgs Portal

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autores principales: Bauer, Martin, Rostagni, Guillaume, Spinner, Jonas
Formato: Preprint
Publicado: 2022
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866915348561788928
author Bauer, Martin
Rostagni, Guillaume
Spinner, Jonas
author_facet Bauer, Martin
Rostagni, Guillaume
Spinner, Jonas
contents The phenomenology of axions and axion-like particles strongly depends on their couplings to Standard Model particles. The focus of this paper is the phenomenology of the unique dimension six operator respecting the shift symmetry: the axion-Higgs portal. We compare constraints from Higgs physics, flavor violating and radiative meson decays, bounds from atomic spectroscopy searching for fifth forces and astrophysical observables. In contrast to the QCD axion, axions interacting through the axion-Higgs portal are stable and can provide a dark matter candidate for any axion mass. We derive the parameter space for which freeze-out and freeze-in production as well as the misalignment mechanism can reproduce the observed relic abundance and compare the results with the phenomenological constraints. For comparison we also derive Higgs, flavor and spectroscopy constraints and the parameter space for which the scalar Higgs portal without derivative interactions can explain dark matter.
format Preprint
id arxiv_https___arxiv_org_abs_2207_05762
institution arXiv
publishDate 2022
record_format arxiv
spellingShingle The Axion-Higgs Portal
Bauer, Martin
Rostagni, Guillaume
Spinner, Jonas
High Energy Physics - Phenomenology
The phenomenology of axions and axion-like particles strongly depends on their couplings to Standard Model particles. The focus of this paper is the phenomenology of the unique dimension six operator respecting the shift symmetry: the axion-Higgs portal. We compare constraints from Higgs physics, flavor violating and radiative meson decays, bounds from atomic spectroscopy searching for fifth forces and astrophysical observables. In contrast to the QCD axion, axions interacting through the axion-Higgs portal are stable and can provide a dark matter candidate for any axion mass. We derive the parameter space for which freeze-out and freeze-in production as well as the misalignment mechanism can reproduce the observed relic abundance and compare the results with the phenomenological constraints. For comparison we also derive Higgs, flavor and spectroscopy constraints and the parameter space for which the scalar Higgs portal without derivative interactions can explain dark matter.
title The Axion-Higgs Portal
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2207.05762