Search for Axionlike-Particle-Induced Prompt γ-Ray Emission from Extragalactic Core-Collapse Supernovae with the Fermi Large Area Telescope

Manuel Meyer and Tanja Petrushevska (Fermi-LAT Collaboration)
Phys. Rev. Lett. 124, 231101 – Published 11 June 2020; Erratum Phys. Rev. Lett. 125, 119901 (2020)
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Abstract

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 2.6×1012GeV1 for ALP masses ma3×1010eV, improving previous limits from SN1987A by a factor of 2.

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  • Received 18 February 2020
  • Revised 22 April 2020
  • Accepted 15 May 2020

DOI:https://doi.org/10.1103/PhysRevLett.124.231101

© 2020 American Physical Society

Physics Subject Headings (PhySH)

  1. Physical Systems
Gravitation, Cosmology & AstrophysicsParticles & Fields

Erratum

Authors & Affiliations

Manuel Meyer* (Fermi-LAT Collaboration)

  • Erlangen Centre for Astroparticle Physics, University of Erlangen-Nuremberg, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany and W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, California 94305, USA

Tanja Petrushevska

  • Centre for Astrophysics and Cosmology, University of Nova Gorica, Vipavska 11c, 5270 Ajdovščina, Slovenia

  • *manuel.e.meyer@fau.de
  • tanja.petrushevska@ung.si

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Issue

Vol. 124, Iss. 23 — 12 June 2020

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