Cosmic ray models

dc.contributor.author	Kachelriess, Michael
dc.contributor.author	Semikoz, DV
dc.date.accessioned	2020-08-24T08:35:11Z
dc.date.available	2020-08-24T08:35:11Z
dc.date.created	2019-08-28T11:29:21Z
dc.date.issued	2019
dc.identifier.issn	0146-6410
dc.identifier.uri	https://hdl.handle.net/11250/2673524
dc.description.abstract	We review progress in high-energy cosmic ray physics focusing on recent experimental results and models developed for their interpretation. Emphasis is put on the propagation of charged cosmic rays, covering the whole range from (20–50) GV, i.e. the rigidity when solar modulations can be neglected, up to the highest energies observed. We discuss models aiming to explain the anomalies in Galactic cosmic rays, the knee, and the transition from Galactic to extragalactic cosmic rays.	en_US
dc.language.iso	eng	en_US
dc.publisher	Elsevier	en_US
dc.title	Cosmic ray models	en_US
dc.type	Journal article	en_US
dc.description.version	submittedVersion	en_US
dc.source.journal	Progress in Particle and Nuclear Physics	en_US
dc.identifier.doi	10.1016/j.ppnp.2019.07.002
dc.identifier.cristin	1719501
dc.description.localcode	© 2019. This is the authors' manuscript to the article.	en_US
cristin.unitcode	194,66,20,0
cristin.unitname	Institutt for fysikk
cristin.ispublished	true
cristin.fulltext	preprint
cristin.qualitycode	1