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Multimessenger Constraints on Radiatively Decaying Axions from GW170817

High Energy Physics - Phenomenology 2024-03-11 v2 High Energy Astrophysical Phenomena

Abstract

The metastable hypermassive neutron star produced in the coalescence of two neutron stars can copiously produce axions that radiatively decay into O(100)\mathcal{O}(100)~MeV photons. These photons can form a fireball with characteristic temperature smaller than 1MeV1\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 11-400MeV400\,\rm MeV. We exclude couplings down to 5×1011GeV15\times 10^{-11}\,\rm GeV^{-1}, complementing and surpassing existing constraints. Our approach can be extended to any feebly-interacting particle decaying into photons.

Keywords

Cite

@article{arxiv.2305.10327,
  title  = {Multimessenger Constraints on Radiatively Decaying Axions from GW170817},
  author = {Melissa Diamond and Damiano F. G. Fiorillo and Gustavo Marques-Tavares and Irene Tamborra and Edoardo Vitagliano},
  journal= {arXiv preprint arXiv:2305.10327},
  year   = {2024}
}

Comments

Version accepted at Phys. Rev. Lett.; 5 pages, 3 figures + 5 pages, 3 figures