CMB Temperature Anisotropy from Broken Spatial Isotropy due to an Homogeneous Cosmological Magnetic Field

Simple item page
dc.creatorKahniashvili, Tina
dc.creatorLavrelashvili, George
dc.creatorRatra, Bharat
dc.date2008-07-26
dc.date2008-09-09
dc.date.accessioned2026-07-07T11:45:06Z
dc.date.available2026-07-07T11:45:06Z
dc.descriptionWe derive the cosmic microwave background temperature anisotropy two-point correlation function (including off-diagonal correlations) from broken spatial isotropy due to an arbitrarily oriented homogeneous cosmological magnetic field.
dc.description16 pages, references added, PRD accepted
dc.identifierhttps://arxiv.org/abs/0807.4239
dc.identifierhttp://arxiv.org/abs/0807.4239
dc.identifierPhys.Rev.D78:063012,2008
dc.identifierdoi:10.1103/PhysRevD.78.063012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201773
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleCMB Temperature Anisotropy from Broken Spatial Isotropy due to an Homogeneous Cosmological Magnetic Field
dc.typetext

Files

Collections

arXiv