Decay photons from the axionlike particles burst of type II supernovae

We determine limits from SN 1987A on massive axionlike particles with masses in the 10 keV-100 MeV range and purely coupled to two photons. Axionlike particles produced in the core collapse escape from the star and decay into photons that can be observed as a delayed and diffuse burst. We discuss th...

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Hauptverfasser: Jaeckel, Joerg (VerfasserIn) , Cavalcanti Malta, Pedro (VerfasserIn) , Redondo, Javier (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 27 September 2018
In: Physical review
Year: 2018, Jahrgang: 98, Heft: 5
ISSN:2470-0029
DOI:10.1103/PhysRevD.98.055032
Online-Zugang:Verlag, Volltext: https://doi.org/10.1103/PhysRevD.98.055032
Verlag: https://link.aps.org/doi/10.1103/PhysRevD.98.055032
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Verfasserangaben:J. Jaeckel, P.C. Malta, J. Redondo
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Zusammenfassung:We determine limits from SN 1987A on massive axionlike particles with masses in the 10 keV-100 MeV range and purely coupled to two photons. Axionlike particles produced in the core collapse escape from the star and decay into photons that can be observed as a delayed and diffuse burst. We discuss the time and angular distribution of such a signal. Looking into the future, we also estimate the possible improvements caused by better gamma-ray detectors or the explosion of the red supergiant Betelgeuse in a supernova event.
Beschreibung:Gesehen am 26.02.2020
Beschreibung:Online Resource
ISSN:2470-0029
DOI:10.1103/PhysRevD.98.055032