Getting the most on supernova axions

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 $g_{aN}\gtrsim 10^{-9}$ for ALP masses $m_a\lesssim 1\mathrm{MeV}$. Remarkably, in the case of canonical QCD axion models, the SN bounds exclude all values of $m_a\gtrsim 10^{-2}\mathrm{eV}$. This result prevents the possibility for current and future cosmological surveys to detect any signatures due to hot dark matter QCD axion mass.

Comments: 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