Cosmic Background Radiation Due to Photon Condensation

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dc.creatorSidharth, B. G.
dc.date1998-06-10
dc.date.accessioned2026-07-07T02:27:10Z
dc.date.available2026-07-07T02:27:10Z
dc.descriptionIt is shown that a collection of photons with nearly the same frequency exhibits a Bose "condensation" type of phenomenon at about 3 degrees K corresponding to a peak intensity at a wave length of about 0.4cm. This could give a mechanism for the observed Cosmic Background Radiation, and also explain some curious features.
dc.description3 pages, TeX
dc.identifierhttps://arxiv.org/abs/astro-ph/9806142
dc.identifierhttp://arxiv.org/abs/astro-ph/9806142
dc.identifierChaos Solitons Fractals 11 (2000) 1471-1472
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12577
dc.subjectAstrophysics
dc.titleCosmic Background Radiation Due to Photon Condensation
dc.typetext

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