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Determination of Cosmological Parameters from Cosmic Microwave Background Anisotropies

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Data Analysis in Cosmology

Part of the book series: Lecture Notes in Physics ((LNP,volume 665))

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Abstract

New cosmic microwave background anisotropies data are increasingly improving our understanding of the evolution and formation of structures in the universe. Here we briefly discuss the cosmological parameters extraction methods, review the latest results and comment about possible modifications to the standard model.

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  1. Dipartimento di Fisica and Sezione INFN Roma, Universita di Roma “La Sapienza”, Ple Aldo Moro 5, 00185, Rome, Italy

    A. Melchiorri, C. Odman & P. Serra

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  1. A. Melchiorri
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    Melchiorri, A., Odman, C., Serra, P. (2008). Determination of Cosmological Parameters from Cosmic Microwave Background Anisotropies. In: Martinez, V., Saar, E., Gonzales, E., Pons-Borderia, M. (eds) Data Analysis in Cosmology. Lecture Notes in Physics, vol 665. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-44767-2_8

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