paper

Getting the most on supernova axions

arXiv:2306.01048 · doi:10.1103/PhysRevD.109.023001

Abstract

Axion-like 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.

15 pages, 7 figures. Matches the version published on PRD. Changes: we employed a different benchmark SN model with respect to the previous version, accounting for a 1D treatment of convection. We added a new section to discuss the uncertainties on the SN bounds. We added an additional section to analyze SN bounds on canonical QCD axion models

References in corpus (32)

Cited by in corpus (38)