Combination and interpretation of observables in Cosmology

The standard cosmological model has deep theoretical foundations but need the introduction of two major unknown components, dark matter and dark energy, to be in agreement with various observations. Dark matter describes a non-relativistic collisionless fluid of (non baryonic) matter which amount...

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Main Author: Virey Jean-Marc
Format: Article
Language:English
Published: EDP Sciences 2010-04-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20100403001
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spelling doaj-735439342f3e46cdaa831adc5cf32d102021-08-02T04:04:46ZengEDP SciencesEPJ Web of Conferences2100-014X2010-04-0140300110.1051/epjconf/20100403001Combination and interpretation of observables in CosmologyVirey Jean-MarcThe standard cosmological model has deep theoretical foundations but need the introduction of two major unknown components, dark matter and dark energy, to be in agreement with various observations. Dark matter describes a non-relativistic collisionless fluid of (non baryonic) matter which amount to 25% of the total density of the universe. Dark energy is a new kind of fluid not of matter type, representing 70% of the total density which should explain the recent acceleration of the expansion of the universe. Alternatively, one can reject this idea of adding one or two new components but argue that the equations used to make the interpretation should be modified consmological scales. Instead of dark matter one can invoke a failure of Newton's laws. Instead of dark energy, two approaches are proposed : general relativity (in term of the Einstein equation) should be modified, or the cosmological principle which fixes the metric used for cosmology should be abandonned. One of the main objective of the community is to find the path of the relevant interpretations thanks to the next generation of experiments which should provide large statistics of observationnal data. Unfortunately, cosmological in formations are difficult to pin down directly fromt he measurements, and it is mandatory to combine the various observables to get the cosmological parameters. This is not problematic from the statistical point of view, but assumptions and approximations made for the analysis may bias our interprettion of the data. Consequently, a strong attention should be paied to the statistical methods used to make parameters estimation and for model testing. After a review of the basics of cosmology where the cosmological parameters are introduced, we discuss the various cosmological probes and their associated observables used to extract cosmological informations. We present the results obtained from several statistical analyses combining data of diferent nature but we insist on the main drawbaks that can falsify our final interpretation. http://dx.doi.org/10.1051/epjconf/20100403001
collection DOAJ
language English
format Article
sources DOAJ
author Virey Jean-Marc
spellingShingle Virey Jean-Marc
Combination and interpretation of observables in Cosmology
EPJ Web of Conferences
author_facet Virey Jean-Marc
author_sort Virey Jean-Marc
title Combination and interpretation of observables in Cosmology
title_short Combination and interpretation of observables in Cosmology
title_full Combination and interpretation of observables in Cosmology
title_fullStr Combination and interpretation of observables in Cosmology
title_full_unstemmed Combination and interpretation of observables in Cosmology
title_sort combination and interpretation of observables in cosmology
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2010-04-01
description The standard cosmological model has deep theoretical foundations but need the introduction of two major unknown components, dark matter and dark energy, to be in agreement with various observations. Dark matter describes a non-relativistic collisionless fluid of (non baryonic) matter which amount to 25% of the total density of the universe. Dark energy is a new kind of fluid not of matter type, representing 70% of the total density which should explain the recent acceleration of the expansion of the universe. Alternatively, one can reject this idea of adding one or two new components but argue that the equations used to make the interpretation should be modified consmological scales. Instead of dark matter one can invoke a failure of Newton's laws. Instead of dark energy, two approaches are proposed : general relativity (in term of the Einstein equation) should be modified, or the cosmological principle which fixes the metric used for cosmology should be abandonned. One of the main objective of the community is to find the path of the relevant interpretations thanks to the next generation of experiments which should provide large statistics of observationnal data. Unfortunately, cosmological in formations are difficult to pin down directly fromt he measurements, and it is mandatory to combine the various observables to get the cosmological parameters. This is not problematic from the statistical point of view, but assumptions and approximations made for the analysis may bias our interprettion of the data. Consequently, a strong attention should be paied to the statistical methods used to make parameters estimation and for model testing. After a review of the basics of cosmology where the cosmological parameters are introduced, we discuss the various cosmological probes and their associated observables used to extract cosmological informations. We present the results obtained from several statistical analyses combining data of diferent nature but we insist on the main drawbaks that can falsify our final interpretation.
url http://dx.doi.org/10.1051/epjconf/20100403001
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