An approach to obtain high-quality data of the early universe was presented by using cosmic microwave background (CMB) anisotropy method. CMB observations concentrated on precise polarization measurements and deep sub-arcmin imaging searching for secondary anisotropies. Both ballon-borne and ground-based experiments independently demonstrated the acoustic pattern of the angular power spectrum.

Anisotropies of the cosmic microwave background / M. Bersanelli, D. Maino, A. Mennella. - In: LA RIVISTA DEL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. - ISSN 0393-697X. - 25:9(2002), pp. 1-82.

Anisotropies of the cosmic microwave background

M. Bersanelli
Primo
;
D. Maino
Secondo
;
A. Mennella
Ultimo
2002

Abstract

An approach to obtain high-quality data of the early universe was presented by using cosmic microwave background (CMB) anisotropy method. CMB observations concentrated on precise polarization measurements and deep sub-arcmin imaging searching for secondary anisotropies. Both ballon-borne and ground-based experiments independently demonstrated the acoustic pattern of the angular power spectrum.
Settore FIS/05 - Astronomia e Astrofisica
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/2434/204245
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