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.

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