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LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas
Part of book or chapter of book . 2020
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https://doi.org/10.1007/978-3-...
Part of book or chapter of book . 2019 . Peer-reviewed
License: Springer TDM
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https://dx.doi.org/10.1007/978...
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Universidade Estadual Paulista São Paulo: Repositório Institucional UNESP
Part of book or chapter of book . 2019
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The Cosmic Microwave Background Radiation (CMBR) Anisotropy

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 01 Jan 2019 Brazil English Publisher:Springer International Publishing
Authors: Năstase, Horaţiu;

doi: 10.1007/978-3-030-15077-8_7

handle: 11449/200469

The Cosmic Microwave Background Radiation (CMBR) Anisotropy

Abstract

In 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.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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