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 1MeV. 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 1-400MeV. We exclude couplings down to 5×10−11GeV−1, complementing and surpassing existing constraints. Our approach can be extended to any feebly-interacting particle decaying into photons.
@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