Abstract
Axionlike particles (ALPs) coupled to nucleons might be copiously emitted from a supernova (SN) core. We extend existing bounds on free-streaming ALPs to the case in which these are so strongly interacting with the nuclear matter to be trapped in the SN core. For strongly interacting ALPs, we also extend the bound from the absence of an ALP-induced signal in Kamiokande-II neutrino detector at the time of SN 1987A. We find that combining the different arguments, SNe exclude values of ALP-nucleon coupling for ALP masses . Remarkably, in the case of canonical QCD axion models, the SN bounds exclude all values of . This result prevents the possibility for current and future cosmological surveys to detect any signatures due to hot dark matter QCD axion mass.
- Received 10 July 2023
- Accepted 6 December 2023
DOI:https://doi.org/10.1103/PhysRevD.109.023001
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Published by the American Physical Society
