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Anisotropy and polarization of cosmic microwave background: state of the art


Lomonosov Moscow State University, Shternberg State Astronomical Institute, Universitetskii prosp. 13, Moscow, 119889, Russian Federation

The anisotropy and polarization of cosmic microwave background radiation provide the most powerful tools for modern cosmology. At present, many experiments for observing these phenomena are either being conducted or prepared, which holds promise for yielding the fundamental parameters of the present and early universe; for shedding light on the crucial current problem of the existence of gravitational waves; and for solidly contributing to elementary particle and high energy physics. In the present paper the formation mechanisms of anisotropy and polarization are briefly discussed. The latest experiments in the field, in particular the WMAP experiment aboard a special spacecraft, are given particular attention.

Fulltext pdf (353 KB)
Fulltext is also available at DOI: 10.1070/PU2004v047n02ABEH001630
PACS: 95.85.Bh, 98.70.Vc, 98.80.−k (all)
DOI: 10.1070/PU2004v047n02ABEH001630
URL: https://ufn.ru/en/articles/2004/2/f/
000222400000006
2004PhyU...47..187S
Citation: Sazhin M V "Anisotropy and polarization of cosmic microwave background: state of the art" Phys. Usp. 47 187–194 (2004)
BibTexBibNote ® (generic)BibNote ® (RIS)Medline RefWorks
RT Journal
T1 Anisotropy and polarization of cosmic microwave background: state of the art
A1 Sazhin,M.V.
PB Physics-Uspekhi
PY 2004
FD 10 Feb, 2004
JF Physics-Uspekhi
JO Phys. Usp.
VO 47
IS 2
SP 187-194
DO 10.1070/PU2004v047n02ABEH001630
LK https://ufn.ru/en/articles/2004/2/f/

Оригинал: Сажин М В «Анизотропия и поляризация реликтового излучения. Последние данные» УФН 174 197–205 (2004); DOI: 10.3367/UFNr.0174.200402g.0197

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