Big Bang Nucleosynthesis, Cosmic Microwave Background Anisotropies and Dark Energy

Details Big Bang Nucleosynthesis, Cosmic Microwave Background Anisotropies and Dark Energy Big Bang Nucleosynthesis, Cosmic Microwave Background Anisotropies and Dark Energy

2001-08-31

arxiv.org/abs/astro-ph/0108515v2

AIP Conf.Proc.616:338-345,2002

Astronomy and Astrophysics

Astrophysics

11 pages, 5 figures, Talk given at 2K1BC Workshop, July 9-12, 2001, Breuil-Cervinia (Italy)

Scientific paper

10.1063/1.1475654

Over the last decade, cosmological observations have attained a level of precision which allows for very detailed comparison with theoretical predictions. We are beginning to learn the answers to some fundamental questions, using information contained in Cosmic Microwave Background Anisotropy (CMBA) data. In this talk, we briefly review some studies of the current and prospected constraints imposed by CMBA measurements on the neutrino physics and on the dark energy. As it was already announced by Scott (1999), we present some possible "new physics" from the Cosmic Microwave Background.

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