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

被引：0

作者：

Moore, E. ^{[1
,2
]}

Gendre, B. ^{[1
,2
]}

Orange, N. B. ^{[3
,4
]}

Panther, F. H. ^{[1
,2
]}

机构：

[1] Univ Western Australia, Dept Phys, Crawley, WA 6009, Australia

[2] OzGrav ARC Ctr Excellence Gravitat wave Discovery, Crawley, WA 6009, Australia

[3] OrangeWave Innovat Sci LLC, Moncks Corner, SC 29461 USA

[4] Univ Virgin Isl, Etelman Observ Res Ctr, St Thomas, VI 00802 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2024年 / 530卷 / 01期

基金：

澳大利亚研究理事会;

关键词：

methods: statistical; gamma-ray burst: general; cosmic rays; LOW-LUMINOSITY; UNIFIED PICTURE; SHOCK BREAKOUT; SUPERNOVA; ACCELERATION; AFTERGLOW; ASSOCIATION; POPULATION; NEUTRINOS; DISCOVERY;

D O I：

10.1093/mnras/stae873

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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-circle dot of ultra-high energy cosmic rays.

引用

页码：555 / 559

页数：5

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