Vacuum polarization energy losses of high energy cosmic rays

dc.creatorMaisheev, V. A.
dc.date2002-06-20
dc.date2002-07-30
dc.date.accessioned2026-07-07T03:47:17Z
dc.date.available2026-07-07T03:47:17Z
dc.descriptionThe process of the vacuum polarization energy losses of high energy cosmic rays propagating in the extragalactic space is considered. The process is due to the polarization of Cosmic Background Radiation by a moving charged particle. With the goal of the description of the process, the photon mass, refractive indices and permittivity function for low and high energy photons are found. Calculations show the rather noticeable level of the energy losses for propagating protons with the enegies more than 10^6 - 10^7 GeV. The influence of the polarization energy losses on propagation of cosmic rays is discussed.
dc.description10 pages, 3 eps figures, Latex, epsfig.sty misprints corrected, mistake in Eqs(7-8) corrected, Eqs(4-5) rewrited in equiv. form, references added, main results not changed
dc.identifierhttps://arxiv.org/abs/hep-ph/0206185
dc.identifierhttp://arxiv.org/abs/hep-ph/0206185
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41604
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleVacuum polarization energy losses of high energy cosmic rays
dc.typetext

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