A problem of hypothetical emerging of cosmic background radiation photons on horizon in the standard model of universe

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dc.creatorSkalsky, V.
dc.date2000-01-14
dc.date2000-09-25
dc.date.accessioned2026-07-07T12:20:22Z
dc.date.available2026-07-07T12:20:22Z
dc.descriptionThe present temperature of cosmic background radiation and the present number density of photons of cosmic background radiation in the observed expansive and isotropic relativistic Universe is in the standard model of universe explained by the assumption of emergence of the photons of cosmic background radiation on the horizon (of the most remote visibility). However, the physical analysis shows unambiguously that this assumption contradicts the special theory of relativity and the quantum mechanics.
dc.description3 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0001251
dc.identifierhttp://arxiv.org/abs/astro-ph/0001251
dc.identifierSkalsky, V. & Sukenik, M.: Radiation of the cosmic background, Astrophysics and Space Science (ISSN 0004-640X), vol. 187, No 1, pp. 155-158, 01/1992
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/213049
dc.subjectAstrophysics
dc.titleA problem of hypothetical emerging of cosmic background radiation photons on horizon in the standard model of universe
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