Cosmology: the homogeneous universe and the evolution of structures
In my course I will first give and introduction to standard cosmology. I discuss the equations of the homogeneous and isotropic universe and I'll briefly summarize its thermal history. After that I want to concentrate on the fluctuations in the universe. We will study anisotropies in the cosmic...
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Lenguaje: | eng |
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2003
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Acceso en línea: | http://cds.cern.ch/record/600181 |
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author | Durrer, Ruth |
author_facet | Durrer, Ruth |
author_sort | Durrer, Ruth |
collection | CERN |
description | In my course I will first give and introduction to standard cosmology. I discuss the equations of the homogeneous and isotropic universe and I'll briefly summarize its thermal history. After that I want to concentrate on the fluctuations in the universe. We will study anisotropies in the cosmic microwave background, fluctuations of the matter density and the velocity field and weak lensing. I want to explain especially new cosmological data which are coming up right now and their implication for the cosmological model.<br><br> N.B. This lecture series will be held in the Auditorium, bldg. 500 on 27, 28, 30, 31 January and in the Council room on 29 January. |
id | cern-600181 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2003 |
record_format | invenio |
spelling | cern-6001812023-10-06T22:03:22Zhttp://cds.cern.ch/record/600181engDurrer, RuthCosmology: the homogeneous universe and the evolution of structuresGeneral Relativity and CosmologyIn my course I will first give and introduction to standard cosmology. I discuss the equations of the homogeneous and isotropic universe and I'll briefly summarize its thermal history. After that I want to concentrate on the fluctuations in the universe. We will study anisotropies in the cosmic microwave background, fluctuations of the matter density and the velocity field and weak lensing. I want to explain especially new cosmological data which are coming up right now and their implication for the cosmological model.<br><br> N.B. This lecture series will be held in the Auditorium, bldg. 500 on 27, 28, 30, 31 January and in the Council room on 29 January.oai:cds.cern.ch:6001812003 |
spellingShingle | General Relativity and Cosmology Durrer, Ruth Cosmology: the homogeneous universe and the evolution of structures |
title | Cosmology: the homogeneous universe and the evolution of structures |
title_full | Cosmology: the homogeneous universe and the evolution of structures |
title_fullStr | Cosmology: the homogeneous universe and the evolution of structures |
title_full_unstemmed | Cosmology: the homogeneous universe and the evolution of structures |
title_short | Cosmology: the homogeneous universe and the evolution of structures |
title_sort | cosmology: the homogeneous universe and the evolution of structures |
topic | General Relativity and Cosmology |
url | http://cds.cern.ch/record/600181 |
work_keys_str_mv | AT durrerruth cosmologythehomogeneousuniverseandtheevolutionofstructures |