Isotherms clustering in cosmic microwave background

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dc.creatorBershadskii, A.
dc.date2006-07-17
dc.date2006-08-21
dc.date.accessioned2026-07-07T07:15:42Z
dc.date.available2026-07-07T07:15:42Z
dc.descriptionSince the strong clustering of luminous matter in the observable universe is a consequence of an initial non-uniformity of the baryon-photon fluid in the last scattering surface, an investigation of clustering of the isotherms in the cosmic microwave background has been performed. The isotherms clustering has been related to the baryon-photon fluid dynamics and the Taylor-microscale Reynolds number of this motion is estimated to be $10^2$. 3-year WMAP cosmic microwave background map has been used in this investigation.
dc.identifierhttps://arxiv.org/abs/astro-ph/0607370
dc.identifierhttp://arxiv.org/abs/astro-ph/0607370
dc.identifierPhys.Lett. A360 (2006) 210-216
dc.identifierdoi:10.1016/j.physleta.2006.08.026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/113309
dc.subjectAstrophysics
dc.subjectStatistical Mechanics
dc.subjectChaotic Dynamics
dc.titleIsotherms clustering in cosmic microwave background
dc.typetext

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