3K, SN's, Clusters: Hunting the Cosmological Parameters with Precision Cosmology / Edition 1

by Domingos Barbosa, Antïnio da Silva, Ana Mourïo

Overview

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."

Product Details

ISBN-13:	9781402019401
Publisher:	Springer Netherlands
Publication date:	05/31/2004
Series:	Cell Engineering
Edition description:	2004
Pages:	218
Product dimensions:	6.10(w) x 9.25(h) x 0.02(d)

Table of Contents

Probing dark energy with supernova searches.- Type Ia supernova models: Latest developments.- Are Type Ia supernovae standard candles?.- Cosmology with supernovae.- Intensive supernovae searches.- Cosmic structures, parameters & temperature anisotropies: Status and perspectives.- Measuring CMB polarisation with the Planck mission.- The Sunyaev-Zel’dovich effect and its uses.- An update on Archeops: Flights and data products.- Cosmological parameters: Where are we?.- Cosmological parameter estimation with the galaxy cluster abundance.- Investigating clusters of galaxies with Planck and Herschel.- SZ scaling relations in galaxy clusters: Results from hydrodynamical N-body simulations.- The gas mass fraction in local and z > 0.7 galaxy clusters: constraints on cosmology.- Deep slices and the supercluster-void network.- Testing cosmological models using the kinematics of high redshift galaxies.- Cosmological constraints from the redshift distribution of galaxy clusters.- The topology of the 2-degree field galaxy redshift survey.