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...
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
27 September 2018
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| 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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| 520 | |a 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. | ||
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