Energy spectrum and mass composition of primary cosmic rays around the `knee' in the framework of the model with two types of sources

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dc.creatorLagutin, A. A.
dc.creatorTyumentsev, A. G.
dc.creatorYushkov, A. V.
dc.date2006-10-21
dc.date.accessioned2026-07-07T11:26:13Z
dc.date.available2026-07-07T11:26:13Z
dc.descriptionAnalysis of the experimental data on cosmic ray spectra in the framework of the proposed model with two types of sources leads to conclusion, that sources with particle generation spectral exponent $p\sim 2.85$ give the major contribution to the all-particle spectrum in the energy range $10^5-10^7$ GeV. `Fine structure' of spectrum around the `knee' may arise due to presence of nearby supernova type source, accelerating particles up to the energies $\sim3\cdot 10^4 Z$ GeV, if the energy output of such source is $\sim2\cdot10^{48}$ erg/source.
dc.descriptionPrepared for XIVth ISVHECRI, Weihai, China
dc.identifierhttps://arxiv.org/abs/astro-ph/0610654
dc.identifierhttp://arxiv.org/abs/astro-ph/0610654
dc.identifierNucl.Phys.Proc.Suppl.175-176:555-558,2008
dc.identifierdoi:10.1016/j.nuclphysbps.2007.11.070
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195757
dc.subjectAstrophysics
dc.titleEnergy spectrum and mass composition of primary cosmic rays around the `knee' in the framework of the model with two types of sources
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