Search for Axionlike-Particle-Induced Prompt γ -Ray Emission from Extragalactic Core-Collapse Supernovae with the Fermi Large Area Telescope
During a core-collapse supernova (SN), axionlike particles (ALPs) could be produced through the Primakoff process and subsequently convert into γ rays in the magnetic field of the Milky Way. We do not find evidence for such a γ-ray burst in observations of extragalactic SNe with the Fermi Large Area Telescope (LAT). The SN explosion times are estimated from optical light curves and we find a probability of about ∼90% that the LAT observed at least one SN at the time of the core collapse. Under the assumption that at least one SN was contained within the LAT field of view, we exclude photon-ALP couplings ≳2.6×10−12 GeV−1 for ALP masses ma≲3×10−10 eV, improving previous limits from SN1987A by a factor of 2.
2020
2020-06-11 16:46:34
1033
darn matter, axions, axion-like particles, core-collapse supernovae
r6
Manuel
Meyer
70
Tanja
Petrushevska
70
COBISS_ID
3
19315459
DOI
15
10.1103/PhysRevLett.124.231101
NUK URN
18
URN:SI:UNG:REP:PMCTVWMJ
SNALPs-2.pdf
31945140
Predstavitvena datoteka
2020-06-11 16:47:46
0
Izvorni URL
2020-06-11 16:46:35