Exploring potential cosmic ray accelerators with neutrinos: what do we learn by injecting nuclei in Gamma-Ray Bursts?

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00550818" target="_blank" >RIV/68378271:_____/18:00550818 - isvavai.cz</a>

Result on the web

<a href="https://pos.sissa.it/301/1064/pdf" target="_blank" >https://pos.sissa.it/301/1064/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.301.1064" target="_blank" >10.22323/1.301.1064</a>

Result language

angličtina

Original language name

Exploring potential cosmic ray accelerators with neutrinos: what do we learn by injecting nuclei in Gamma-Ray Bursts?

Original language description

Neutrino stacking analysis constrains the paradigm that Gamma-Ray Bursts (GRBs) are the sources of the Ultra-High Energy Cosmic Rays (UHECRs). However, most of the literature has focused on a pure proton composition of UHECRs, which has been disfavored by recent composition measurements of the Pierre Auger Observatory. The injection of nuclei in the sources is here considered by simulating the nuclear cascade in the photon field of a GRB within the (one-zone) internal shock model. We demonstrate that the prompt neutrino flux hardly depends on the injected composition and is potentially able to strongly constrain UHECR models.n

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

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OECD FORD branch

10303 - Particles and field physics

Project

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Continuities

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Publication year

2018

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Proceedings of Science

ISBN

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ISSN

1824-8039

e-ISSN

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Number of pages

8

Pages from-to

1-8

Publisher name

Sissa Medilab srl

Place of publication

Trieste

Event location

Busan

Event date

Jul 10, 2017

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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