Diffuse CR, neutrino and gamma-ray fluxes from AGNs
| dc.contributor.author | Giacinti, Gwenael | |
| dc.contributor.author | Kachelriess, Michael | |
| dc.contributor.author | Kalashev, Oleg | |
| dc.contributor.author | Neronov, Andrei | |
| dc.contributor.author | Semikoz, Dimitry | |
| dc.date.accessioned | 2020-03-24T14:08:50Z | |
| dc.date.available | 2020-03-24T14:08:50Z | |
| dc.date.created | 2017-01-19T14:27:37Z | |
| dc.date.issued | 2016 | |
| dc.identifier.citation | PoS - Proceedings of Science. 2016, ICRC2015 . | en_US |
| dc.identifier.issn | 1824-8039 | |
| dc.identifier.uri | https://hdl.handle.net/11250/2648400 | |
| dc.description.abstract | We investigate how the extragalactic proton component derived within the ’escape model’ canbe explained by astrophysical sources. We find that the complete extragalactic proton spectrumcan be explained by a single source population with late time evolution, such as BL Lacs orFR I galaxies. We then calculate the diffuse neutrino andg-ray fluxes produced by these CRprotons interacting with gas inside their sources, their host galaxies and galaxy clusters. For aspectral slope of CRs close toa=2:1 | en_US |
| dc.language.iso | eng | en_US |
| dc.publisher | Sissa Medialab | en_US |
| dc.rights | Navngivelse-Ikkekommersiell-DelPåSammeVilkår 4.0 Internasjonal | * |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/deed.no | * |
| dc.title | Diffuse CR, neutrino and gamma-ray fluxes from AGNs | en_US |
| dc.type | Peer reviewed | en_US |
| dc.type | Journal article | en_US |
| dc.description.version | publishedVersion | en_US |
| dc.source.pagenumber | 8 | en_US |
| dc.source.volume | ICRC2015 | en_US |
| dc.source.journal | PoS - Proceedings of Science | en_US |
| dc.identifier.doi | https://doi.org/10.22323/1.236.1124 | |
| dc.identifier.cristin | 1432424 | |
| dc.description.localcode | Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-ShareAlike. | en_US |
| cristin.ispublished | true | |
| cristin.fulltext | original | |
| cristin.qualitycode | 1 |
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