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Publicação:
The Cosmic Microwave Background Radiation (CMBR) Anisotropy

dc.contributor.authorNăstase, Horaţiu [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2020-12-12T02:07:29Z
dc.date.available2020-12-12T02:07:29Z
dc.date.issued2019-01-01
dc.description.abstractIn this chapter we will describe the Cosmic Microwave Background Radiation and its anisotropy. After describing the CMBR kinematics, we will see how primordial perturbations, in particular curvature perturbations, that were already observed, are described and propagate, and how they influence the CMBR.en
dc.description.affiliationInstituto de Física Teórica UNESP
dc.description.affiliationUnespInstituto de Física Teórica UNESP
dc.format.extent77-93
dc.identifierhttp://dx.doi.org/10.1007/978-3-030-15077-8_7
dc.identifier.citationFundamental Theories of Physics, v. 197, p. 77-93.
dc.identifier.doi10.1007/978-3-030-15077-8_7
dc.identifier.issn2365-6425
dc.identifier.issn0168-1222
dc.identifier.scopus2-s2.0-85085178214
dc.identifier.urihttp://hdl.handle.net/11449/200469
dc.language.isoeng
dc.relation.ispartofFundamental Theories of Physics
dc.sourceScopus
dc.titleThe Cosmic Microwave Background Radiation (CMBR) Anisotropyen
dc.typeCapítulo de livro
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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