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arXiv.org e-Print Archive
Preprint . 1999
Data sources: arXiv.org e-Print Archive
https://dx.doi.org/10.48550/ar...
Article . 1999
License: arXiv Non-Exclusive Distribution
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Article . 1999
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Anisotropies in the CMB

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 1999Embargo end date: 01 Jan 1999Publisher:arXiv
Authors: White, Martin;

doi: 10.48550/arxiv.astro-ph/9903232

arXiv: http://arxiv.org/abs/astro-ph/9903232

Anisotropies in the CMB

Abstract

The ten's of micro-Kelvin variations in the temperature of the cosmic microwave background (CMB) radiation across the sky encode a wealth of information about the Universe. The full-sky, high-resolution maps of the CMB that will be made in the next decade should determine cosmological parameters to unprecedented precision and sharply test inflation and other theories of the early Universe.

7 pages, 7 figures, to appear in proceedings of DPF99

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Keywords

astro-ph, Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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citations
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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