Implications of strong intergalactic magnetic fields for ultrahigh-energy cosmic-ray astronomy-Reference-Cited by-同舟云学术

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Implications of strong intergalactic magnetic fields for ultrahigh-energy cosmic-ray astronomy

Published:2017-07-25 Issue:2 Volume:96 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Alves Batista Rafael,Shin Min-Su,Devriendt Julien,Semikoz Dmitri,Sigl Guenter

Funder

Fondazione Internazionale Premio Balzan

Deutsche Forschungsgemeinschaft

Bundesministerium für Bildung und Forschung

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.96.023010/fulltext

Reference72 articles.

1. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above1017.8 eV

2. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications

3. Study of Ultra-High Energy Cosmic Ray composition using Telescope Array’s Middle Drum detector and surface array in hybrid mode

4. Report of the Working Group on the Composition of Ultra High Energy Cosmic Rays

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1. Ultra-high-energy Cosmic-Ray Sources Can Be Gamma-Ray Dim;The Astrophysical Journal Letters;2024-05-01

2. The unprecedented flaring activities around Mrk 421 in 2012 and 2013: The test for neutrino and UHECR event connection;Journal of High Energy Astrophysics;2023-11

3. Nearby active galactic nuclei and starburst galaxies as sources of the measured UHECRs anisotropy signal;Journal of Cosmology and Astroparticle Physics;2023-07-01

4. Ultra high energy cosmic rays The intersection of the Cosmic and Energy Frontiers;Astroparticle Physics;2023-07

5. Effects of large-scale magnetic fields on the observed composition of ultrahigh-energy cosmic rays;Physical Review D;2023-05-15

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