A numerical model for the propagation of ultra-high energy cosmic rays through extragalactic magnetic fields

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00549821" target="_blank" >RIV/68378271:_____/18:00549821 - isvavai.cz</a>

Result on the web

<a href="https://pos.sissa.it/301/477/pdf" target="_blank" >https://pos.sissa.it/301/477/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.301.0477" target="_blank" >10.22323/1.301.0477</a>

Result language

angličtina

Original language name

A numerical model for the propagation of ultra-high energy cosmic rays through extragalactic magnetic fields

Original language description

We present a novel numerical model for the propagation of ultra-high energy charged particles in the intergalactic medium, assumed to have a cellular structure of coherent magnetic fields. We take into account the diffusion of ultrarelativistic particles under the influence of the extragalactic magnetic fields and their energy losses. The fields are considered to have random orientations of their vector components within the cells with smooth transitions between them. The propagator presents a very high accuracy on calculating the particle tracking, on the order of ≲10−33 of relative error in energy, and 10−5 in Larmor radius.

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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