The VHE anomaly in blazar spectra and related phenomena
Most of the recent research on extragalactic γ-ray propagation focused on the study of the γγ * e+e− absorption process (“absorption-only model”). Starting from a possible anomaly at very high energies (VHE, E > 100 GeV), we briefly review several existing deviations from this model. The exotic i...
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2017-01-01
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Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201614517002 |
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doaj-62ce4a6d155740d4a8ed323e536476d22021-08-02T14:37:18ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011451700210.1051/epjconf/201614517002epjconf-isvhecri2016_17002The VHE anomaly in blazar spectra and related phenomenaDzhatdoev Timur0Khalikov Emil1Kircheva Anna2Lyukshin Alexander3Federal State Budget Educational Institution of Higher Education M.V. Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)Federal State Budget Educational Institution of Higher Education M.V. Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics (SINP MSU)Federal State Budget Educational Institution of Higher Education M.V. Lomonosov Moscow State University, Department of PhysicsFederal State Budget Educational Institution of Higher Education M.V. Lomonosov Moscow State University, Department of PhysicsMost of the recent research on extragalactic γ-ray propagation focused on the study of the γγ * e+e− absorption process (“absorption-only model”). Starting from a possible anomaly at very high energies (VHE, E > 100 GeV), we briefly review several existing deviations from this model. The exotic interpretation of the VHE anomaly is not supported by the recent works. On the other hand, the process of intergalactic electromagnetic cascade development naturally explains these effects. We discuss phenomenology of intergalactic cascades and the main spectral signatures of the electromagnetic cascade model. We also briefly consider the hadronic cascade model; it also may explain the data, but requires low strength of magnetic field around the source of primary protons or nuclei.https://doi.org/10.1051/epjconf/201614517002 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Dzhatdoev Timur Khalikov Emil Kircheva Anna Lyukshin Alexander |
spellingShingle |
Dzhatdoev Timur Khalikov Emil Kircheva Anna Lyukshin Alexander The VHE anomaly in blazar spectra and related phenomena EPJ Web of Conferences |
author_facet |
Dzhatdoev Timur Khalikov Emil Kircheva Anna Lyukshin Alexander |
author_sort |
Dzhatdoev Timur |
title |
The VHE anomaly in blazar spectra and related phenomena |
title_short |
The VHE anomaly in blazar spectra and related phenomena |
title_full |
The VHE anomaly in blazar spectra and related phenomena |
title_fullStr |
The VHE anomaly in blazar spectra and related phenomena |
title_full_unstemmed |
The VHE anomaly in blazar spectra and related phenomena |
title_sort |
vhe anomaly in blazar spectra and related phenomena |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2017-01-01 |
description |
Most of the recent research on extragalactic γ-ray propagation focused on the study of the γγ * e+e− absorption process (“absorption-only model”). Starting from a possible anomaly at very high energies (VHE, E > 100 GeV), we briefly review several existing deviations from this model. The exotic interpretation of the VHE anomaly is not supported by the recent works. On the other hand, the process of intergalactic electromagnetic cascade development naturally explains these effects. We discuss phenomenology of intergalactic cascades and the main spectral signatures of the electromagnetic cascade model. We also briefly consider the hadronic cascade model; it also may explain the data, but requires low strength of magnetic field around the source of primary protons or nuclei. |
url |
https://doi.org/10.1051/epjconf/201614517002 |
work_keys_str_mv |
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