Publication: Gamma-ray counterpart of the IceCube neutrinos
Дата
2019
Авторы
Kachelriess, M.
Neronov, A.
Semikoz, D. V.
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Аннотация
© Published under licence by IOP Publishing Ltd. A γ-ray excess at high Galactic latitudes starting at energies 300 GeV was recently discovered in the data of the Fermi telescope. The multi-TeV γ-ray emission found has spectral characteristics at both low and high Galactic latitudes compatible with those of the IceCube neutrinos in the same sky regions. This suggests that these γ-rays are the counterpart of the IceCube neutrino signal, implying that a sizeable part of the IceCube neutrino flux originates from the Milky Way. The diffuse neutrino and γ-ray signal at high Galactic latitudes may originate either from a nearby cosmic ray "PeVatron" cosmic ray source, an extended Galactic cosmic ray halo or from decays of heavy dark matter particles.
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Цитирование
Kachelriess, M. Gamma-ray counterpart of the IceCube neutrinos / Kachelriess, M., Neronov, A., Semikoz, D.V. // Journal of Physics: Conference Series. - 2019. - 1181. - № 1. - 10.1088/1742-6596/1181/1/012052
URI
https://www.doi.org/10.1088/1742-6596/1181/1/012052
https://www.scopus.com/record/display.uri?eid=2-s2.0-85064349427&origin=resultslist
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000556332900052
https://openrepository.mephi.ru/handle/123456789/16902
https://www.scopus.com/record/display.uri?eid=2-s2.0-85064349427&origin=resultslist
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000556332900052
https://openrepository.mephi.ru/handle/123456789/16902