Supernova bound on Axion-Like Particles coupled with electrons
arXiv:2107.12393 · doi:10.1103/PhysRevD.104.103007
Abstract
Axion-Like Particles (ALPs) coupled with electrons would be produced in a Supernova (SN) via electron-proton bremsstrahlung and electron-positron fusion. We evaluate the ALP emissivity from these processes by taking into account the ALP mass and thermal effects on electrons in the strongly degenerate and relativistic SN plasma. Using a state-of-the-art SN simulation, we evaluate the SN 1987A cooling bound on ALPs for masses in the range MeV, which excludes currently unprobed regions down to at MeV.
12 pages, 12 figures. Minor changes to match the version published on PRD
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