CMBR distortion concerned with recombination of the primordial hydrogen plasma

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dc.creatorKholupenko, E. E.
dc.creatorIvanchik, A. V.
dc.creatorVarshalovich, D. A.
dc.date2005-09-27
dc.date.accessioned2026-07-07T06:20:15Z
dc.date.available2026-07-07T06:20:15Z
dc.descriptionCMBR distortion concerned with recombination of the primordial plasma is calculated in frequency band from 1 GHz to 100 GHz in the frame of the standard cosmological model for different values of cosmological density parameters: nonrelativistic matter density $Ω_m$ and baryonic matter density $Ω_b$. Comparison of these results with observational data which will be obtained from planned experiments may be used for independent determination of the cosmological parameters $Ω_m$ and $Ω_b$.
dc.description6 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0509807
dc.identifierhttp://arxiv.org/abs/astro-ph/0509807
dc.identifierGrav.Cosmol. 11 (2005) 161-165
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/95277
dc.subjectAstrophysics
dc.titleCMBR distortion concerned with recombination of the primordial hydrogen plasma
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