After the successful measurements of many ground based, balloon-borne and satellite experiments, which started the era of "Precision Cosmology", Cosmic Microwave Background (CMB) observations are now focusing on two targets: the precision measurement of B-modes in the polarization field, and the measurement of the Sunyaev-Zeldovich effect in distant clusters of galaxies. Polarization measurements represent the best way to probe the very early universe, and the energy scale of inflation. Fine-scale anisotropy measurements, possibly with spectral capabilities, can provide important information on (lark matter and dark energy. Here we describe original approaches to these measurements.

Science with future cosmic microwave background observations / DE BERNARDIS, Paolo; Calvo, Martino; Giordano, Claudia; Masi, Silvia; Nati, Federico; Piacentini, Francesco; Schillaci, Alessandro. - In: NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS. - ISSN 0920-5632. - STAMPA. - 194:C(2009), pp. 350-356. ((Intervento presentato al convegno Galileo-Galilei-Institute Conference on Dark Matter and Dark Energy tenutosi a Florence; Italy [10.1016/j.nuclphysbps.2009.07.097].

Science with future cosmic microwave background observations

DE BERNARDIS, Paolo;CALVO, MARTINO;GIORDANO, CLAUDIA;MASI, Silvia;NATI, FEDERICO;PIACENTINI, Francesco;SCHILLACI, ALESSANDRO
2009

Abstract

After the successful measurements of many ground based, balloon-borne and satellite experiments, which started the era of "Precision Cosmology", Cosmic Microwave Background (CMB) observations are now focusing on two targets: the precision measurement of B-modes in the polarization field, and the measurement of the Sunyaev-Zeldovich effect in distant clusters of galaxies. Polarization measurements represent the best way to probe the very early universe, and the energy scale of inflation. Fine-scale anisotropy measurements, possibly with spectral capabilities, can provide important information on (lark matter and dark energy. Here we describe original approaches to these measurements.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11573/55377
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