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

Fuente: arXiv
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Main Authors: Moore, Eloise, Gendre, Bruce, Orange, N. Brice, Panther, Fiona H.
Format: Preprint
Published: 2023
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author Moore, Eloise
Gendre, Bruce
Orange, N. Brice
Panther, Fiona H.
author_facet Moore, Eloise
Gendre, Bruce
Orange, N. Brice
Panther, Fiona H.
contents 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$_\odot$ of ultra-high energy cosmic rays.
format Preprint
id arxiv_https___arxiv_org_abs_2303_13781
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Constraints on the ultra-high energy cosmic ray output of gamma-ray bursts
Moore, Eloise
Gendre, Bruce
Orange, N. Brice
Panther, Fiona H.
High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
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$_\odot$ of ultra-high energy cosmic rays.
title Constraints on the ultra-high energy cosmic ray output of gamma-ray bursts
topic High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2303.13781