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2024MNRAS.530..555M - Mon. Not. R. Astron. Soc., 530, 555-559 (2024/May-1)

Constraints on the ultra-high energy cosmic ray output of gamma-ray bursts.

MOORE E., GENDRE B., ORANGE N.B. and PANTHER F.H.

Abstract (from CDS):

Ultra-high energy cosmic rays are the most extreme energetic particles detected on Earth, however, their acceleration sites are still mysterious. We explore the contribution of low-luminosity gamma-ray bursts to the ultra-high energy cosmic ray flux, since they form the bulk of the nearby population. We analyse a representative sample of these bursts detected by BeppoSAX, INTEGRAL, and Swift between 1998-2016, and found that in order to reconcile our theoretical flux with the observed flux, these bursts should accelerate at most 10–13 M⊙ of ultra-high energy cosmic rays.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): methods: statistical - gamma-ray burst: general - cosmic rays

Simbad objects: 44

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