Published March 5, 2024 | Version v1
Journal article Open

Multimessenger Constraints on Radiatively Decaying Axions from GW170817

  • 1. Arthur B. McDonald Canadian Astropartical Physics Institute, Queens University, Kingston, Ontario K7L 3N6, Canada
  • 2. Niels Bohr International Academy, Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, 2100 Copenhagen, Denmark
  • 3. Maryland Center for Fundamental Physics, Department of Physics, University of Maryland, College Park, Maryland 20742, USA
  • 4. DARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 128, 2200 Copenhagen, Denmark
  • 5. Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel

Description

The metastable hypermassive neutron star produced in the coalescence of two neutron stars can copiously produce axions that radiatively decay into O(100)MeV photons. These photons can form a fireball with characteristic temperature smaller than 1 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 MeV. We exclude couplings down to 5×1011GeV1, complementing and surpassing existing constraints. Our approach can be extended to any feebly interacting particle decaying into photons.

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10.1103_PhysRevLett.132.101004.pdf

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Additional details

Identifiers

DOI
10.1103/PhysRevLett.132.101004;
arXiv
arXiv:2305.10327;
Crossref Funder ID
10.13039/501100000038; 10.13039/100008398; 10.13039/100010661; 10.13039/100018694; 10.13039/100000001; 10.13039/501100001742; 10.13039/501100002808; 10.13039/501100001659; 10.13039/100010663;

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
132
Journal Issue
10
Journal Page Range
8 pgs.
ISSN
0031-9007