Decay photons from the axionlike particles burst of type II supernovae
Financiación H2020 / H2020 Funds
Resumen: 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.
Idioma: Inglés
DOI: 10.1103/PhysRevD.98.055032
Año: 2018
Publicado en: PHYSICAL REVIEW D 98, 5 (2018), 055032 [14 pp]
ISSN: 2470-0010

Factor impacto JCR: 4.368 (2018)
Categ. JCR: ASTRONOMY & ASTROPHYSICS rank: 17 / 69 = 0.246 (2018) - Q1 - T1
Categ. JCR: PHYSICS, PARTICLES & FIELDS rank: 7 / 29 = 0.241 (2018) - Q1 - T1

Factor impacto SCIMAGO: 1.703 - Physics and Astronomy (miscellaneous) (Q1)

Financiación: info:eu-repo/grantAgreement/EC/H2020/674896/EU/The Elusives Enterprise: Asymmetries of the Invisible Universe/ELUSIVES
Financiación: info:eu-repo/grantAgreement/EC/H2020/690575/EU/InvisiblesPlus/InvisiblesPlus
Financiación: info:eu-repo/grantAgreement/ES/MINECO/FPA2015-65745-P
Tipo y forma: Article (Published version)
Área (Departamento): Área Física Teórica (Dpto. Física Teórica)

Rights Reserved All rights reserved by journal editor

Exportado de SIDERAL (2019-12-12-10:13:39)

Este artículo se encuentra en las siguientes colecciones:

 Record created 2018-11-27, last modified 2019-12-12

Versión publicada:
Rate this document:

Rate this document:
(Not yet reviewed)