ENGLISH

3K, SN’s, Clusters: Hunting the Cosmological Parameters with Precision Cosmology: A JENAM 2002 Workshop Porto, Portugal 3–5 September 2002

By Domingos Barbosa , Sébastien Fabbro (auth.) , António José Da Silva , Ana Maria Mourão (eds.)

Book information

Publisher
Springer Netherlands
Year
2004
ISBN
978-90-481-6546-9, 978-94-017-0559-2
DOI
10.1007/978-94-017-0559-2
Language
english
Format
PDF
Filesize
6 MB (6269927 bytes)
Edition
1
Pages
218\222
Time added
2013-12-12 02:00:00
Classical and Quantum GravitationObservations and TechniquesRelativity Theory;Astrophysics and Astroparticles;

Description

The last few years saw the development of a plethora of experiments and surveys probing the cosmological parameters. The Cosmic Microwave Background (CMB), the Supernovae (SN) searches and galaxy cluster data, namely via X-rays and Sunyaev-Zel'dovich effect, are among the most prolific giving detailed information about the geometry, age and structure formation of the Universe. The program of the WS-HCP workshop was aimed at highlighting the scientific achievements and to discuss the new environment of "precision cosmology" within these three probes. The objective was to analyse different observational strategies, common problems namely foregrounds, and to assess the impact of observational uncertainties in the determination of key cosmological parameters which describe the primordial universe and the large scale structure formation mechanism.

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