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Talk1 h 6 min

Cosmology : the homogeneous universe and the evolution of structures

Ruth Durrer · CERN

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About

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.

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..

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The talk

  1. Cosmology : the homogeneous universe and the evolution of structures 2003-01-30 · 1 h 6 min · CERN's player

Credits and licence

Institution
CERN
Department
CERN Academic Training Lecture
Speaker
Ruth Durrer
Year
2003
Level
Graduate
Language
English
Subjects
Physics, Astronomy and space
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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