Vela as the Source of Galactic Cosmic Rays above 100 TeV

dc.contributor.author	Kachelriess, Michael
dc.contributor.author	Semikoz, Dmitri
dc.contributor.author	Bouyahiaoui, Makarim
dc.date.accessioned	2022-10-03T12:55:32Z
dc.date.available	2022-10-03T12:55:32Z
dc.date.created	2021-01-11T21:04:08Z
dc.date.issued	2020
dc.identifier.issn	1824-8039
dc.identifier.uri	https://hdl.handle.net/11250/3023389
dc.description.abstract	We modeled the contribution of the young supernova remant Vela to the local cosmic rays taking into account the effect of the Local superBubble and an anistropic diffusion. We recovered the knee observed in the CR spectrum at energy of 3-5 PeV. By the contribution of Vela and an older local source of 2-3 Myr supernova we were able to explain the CR spectrum from TeV to 100 PeV.	en_US
dc.language.iso	eng	en_US
dc.publisher	Sissa Medialab	en_US
dc.rights	Attribution-NonCommercial-NoDerivatives 4.0 Internasjonal	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/4.0/deed.no	*
dc.title	Vela as the Source of Galactic Cosmic Rays above 100 TeV	en_US
dc.title.alternative	Vela as the Source of Galactic Cosmic Rays above 100 TeV	en_US
dc.type	Peer reviewed	en_US
dc.type	Journal article	en_US
dc.description.version	publishedVersion	en_US
dc.source.volume	ICRC2019	en_US
dc.source.journal	Proceedings of Science (PoS)	en_US
dc.source.issue	039	en_US
dc.identifier.doi	10.22323/1.358.0039
dc.identifier.cristin	1869419
cristin.ispublished	true
cristin.fulltext	original
cristin.qualitycode	1

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