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Cosmic ray models

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Nov 2019Embargo end date: 01 Jan 2019 France English Publisher:Elsevier BVJournal:Progress in Particle and Nuclear Physics, volume 109, page 103,710 (issn: 0146-6410,

Authors: Kachelriess, M.; Semikoz, D.V.;

doi: 10.1016/j.ppnp.2019.07.002 , 10.48550/arxiv.1904.08160

arXiv: http://arxiv.org/abs/1904.08160

handle: 11250/2673524

Cosmic ray models

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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 $\sim (20-50)$ 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.

89 pages, 56 figures; v2: minor additions, version to appear

Country

France

Related Organizations

French National Centre for Scientific Research
France
CEA LETI
France
PSL Research University
France
University of Paris
France
NTNU
Norway

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Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), anomaly, FOS: Physical sciences, High-energy cosmic rays, 530, UHE, solar, modulation, Cosmic ray propagation, Magnetic fields, cosmic radiation: galaxy, propagation, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Astrophysics - High Energy Astrophysical Phenomena, Cosmic ray secondaries, cosmic radiation: model, experimental results

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	56
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Top 1%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 1%