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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Online Access: | http://dx.doi.org/10.1051/epjconf/20100403001 |
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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 |
work_keys_str_mv |
AT vireyjeanmarc combinationandinterpretationofobservablesincosmology |
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