Multimessenger Constraints on Radiatively Decaying Axions from GW170817

Fuente: arXiv
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Autores principales: Diamond, Melissa, Fiorillo, Damiano F. G., Marques-Tavares, Gustavo, Tamborra, Irene, Vitagliano, Edoardo
Formato: Preprint
Publicado: 2023
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author Diamond, Melissa
Fiorillo, Damiano F. G.
Marques-Tavares, Gustavo
Tamborra, Irene
Vitagliano, Edoardo
author_facet Diamond, Melissa
Fiorillo, Damiano F. G.
Marques-Tavares, Gustavo
Tamborra, Irene
Vitagliano, Edoardo
contents The metastable hypermassive neutron star produced in the coalescence of two neutron stars can copiously produce axions that radiatively decay into $\mathcal{O}(100)$~MeV photons. These photons can form a fireball with characteristic temperature smaller than $1\rm\, MeV$. By relying on X-ray observations of GW170817/GRB 170817A with CALET CGBM, Konus-Wind, and Insight-HXMT/HE, we present new bounds on the axion-photon coupling for axion masses in the range $1$-$400\,\rm MeV$. We exclude couplings down to $5\times 10^{-11}\,\rm GeV^{-1}$, complementing and surpassing existing constraints. Our approach can be extended to any feebly-interacting particle decaying into photons.
format Preprint
id arxiv_https___arxiv_org_abs_2305_10327
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Multimessenger Constraints on Radiatively Decaying Axions from GW170817
Diamond, Melissa
Fiorillo, Damiano F. G.
Marques-Tavares, Gustavo
Tamborra, Irene
Vitagliano, Edoardo
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
The metastable hypermassive neutron star produced in the coalescence of two neutron stars can copiously produce axions that radiatively decay into $\mathcal{O}(100)$~MeV photons. These photons can form a fireball with characteristic temperature smaller than $1\rm\, MeV$. By relying on X-ray observations of GW170817/GRB 170817A with CALET CGBM, Konus-Wind, and Insight-HXMT/HE, we present new bounds on the axion-photon coupling for axion masses in the range $1$-$400\,\rm MeV$. We exclude couplings down to $5\times 10^{-11}\,\rm GeV^{-1}$, complementing and surpassing existing constraints. Our approach can be extended to any feebly-interacting particle decaying into photons.
title Multimessenger Constraints on Radiatively Decaying Axions from GW170817
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2305.10327