CMB Spectral Distortions from an Axion-Dark Photon-Photon Interaction

Fuente: arXiv
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Main Authors: Hook, Anson, Marques-Tavares, Gustavo, Ristow, Clayton
Format: Preprint
Published: 2023
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author Hook, Anson
Marques-Tavares, Gustavo
Ristow, Clayton
author_facet Hook, Anson
Marques-Tavares, Gustavo
Ristow, Clayton
contents The presence of a plethora of light spin 0 and spin 1 fields is motivated in a number of BSM scenarios, such as the axiverse. The study of the interactions of such light bosonic fields with the Standard Model has focused mostly on interactions involving only one such field, such as the axion ($ϕ$) coupling to photons, $ϕF \tilde F$, or the kinetic mixing between photon and the dark photon, $ F F_D$. In this work, we continue the exploration of interactions involving two light BSM fields and the standard model, focusing on the mixed axion-photon-dark-photon interaction $ϕF \tilde F_D$. If either the axion or dark photon are dark matter, we show that this interaction leads to conversion of the CMB photons into a dark sector particle, leading to a distortion in the CMB spectrum. We present the details of these unique distortion signatures and the resulting constraints on the $ϕF \tilde F_D$ coupling. In particular, we find that for a wide range of masses, the constraints from these effect are stronger than on the more widely studied axion-photon coupling.
format Preprint
id arxiv_https___arxiv_org_abs_2306_13135
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle CMB Spectral Distortions from an Axion-Dark Photon-Photon Interaction
Hook, Anson
Marques-Tavares, Gustavo
Ristow, Clayton
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
The presence of a plethora of light spin 0 and spin 1 fields is motivated in a number of BSM scenarios, such as the axiverse. The study of the interactions of such light bosonic fields with the Standard Model has focused mostly on interactions involving only one such field, such as the axion ($ϕ$) coupling to photons, $ϕF \tilde F$, or the kinetic mixing between photon and the dark photon, $ F F_D$. In this work, we continue the exploration of interactions involving two light BSM fields and the standard model, focusing on the mixed axion-photon-dark-photon interaction $ϕF \tilde F_D$. If either the axion or dark photon are dark matter, we show that this interaction leads to conversion of the CMB photons into a dark sector particle, leading to a distortion in the CMB spectrum. We present the details of these unique distortion signatures and the resulting constraints on the $ϕF \tilde F_D$ coupling. In particular, we find that for a wide range of masses, the constraints from these effect are stronger than on the more widely studied axion-photon coupling.
title CMB Spectral Distortions from an Axion-Dark Photon-Photon Interaction
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2306.13135