Effect of extragalactic magnetic field on cascade gamma-ray emission
- Authors: Uryson A.V.1
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Affiliations:
- Lebedev Physical Institute of the Russian Academy of Sciences
- Issue: Vol 88, No 3 (2024)
- Pages: 495-497
- Section: Physics of Cosmic Rays
- URL: https://jdigitaldiagnostics.com/0367-6765/article/view/654740
- DOI: https://doi.org/10.31857/S0367676524030216
- EDN: https://elibrary.ru/QKWBDN
- ID: 654740
Cite item
Abstract
The intensity of diffuse cascade gamma-ray emission produced in electromagnetic cascades when ultra-high energy cosmic rays propagate in extragalactic space is discussed. It is obtained that in the range of ~107—109 eV diffuse cascade gamma-ray spectra weakly depends on extragalactic magnetic field value. Thus, there is no need to refine extragalactic magnetic field models to estimate the intensity of cascade emission in this energy range.
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About the authors
A. V. Uryson
Lebedev Physical Institute of the Russian Academy of Sciences
Author for correspondence.
Email: uryson@sci.lebedev.ru
Russian Federation, Moscow
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Supplementary files
Supplementary Files
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JATS XML
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Fig. 1. Model spectra of diffuse cascade gamma-ray emission near the Earth at B = 10-6, 10-12 Gs. The spectra at B < 10-12 and B = 10-12 Gs coincide
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