Peters cycle at the end of the cosmic ray spectrum?

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F24%3A00604948" target="_blank" >RIV/68378271:90232/24:00604948 - isvavai.cz</a>

Result on the web

<a href="https://doi.org/10.1103/PhysRevD.109.023006" target="_blank" >https://doi.org/10.1103/PhysRevD.109.023006</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1103/PhysRevD.109.023006" target="_blank" >10.1103/PhysRevD.109.023006</a>

Result language

angličtina

Original language name

Peters cycle at the end of the cosmic ray spectrum?

Original language description

We investigate the degree to which current ultrahigh-energy cosmic ray observations above the ankle support a common maximum rigidity for all nuclei, often called a Peters cycle, over alternative scenarios for the cosmic ray spectra escaping sources. We show that a Peters cycle is not generally supported by the data when compared with these alternatives for the scenarios studied. We explore the observational signatures of non-Peters cycle scenarios, and the opportunities to explore both ultrahigh-energy cosmic ray source conditions, as well as physics beyond the Standard Model they present.n

Czech name

—

Czech description

—

Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

—

OECD FORD branch

10303 - Particles and field physics

Project

—

Continuities

—

Publication year

2024

Confidentiality

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

Name of the periodical

Physical Review D

ISSN

2470-0010

e-ISSN

2470-0029

Volume of the periodical

109

Issue of the periodical within the volume

2

Country of publishing house

US - UNITED STATES

Number of pages

10

Pages from-to

023006

UT code for WoS article

001172661500001

EID of the result in the Scopus database

2-s2.0-85181879992