Descriptif
Lecturer: David LANGLOIS
1. Homogeneous cosmology (Friedmann equations, cosmological parameters)
2. Thermal history (nucleosynthesis, recombination, neutrinos, dark matter)
3. Inflation
4. Theory of cosmological perturbations
5. Initial conditions from inflation
6. Cosmic Microwave Background
7. Large scale structures
Bibliography:
- "Inflation, quantum fluctuations and cosmological perturbations", D. Langlois, arXiv:hep-th/0405053
Lectures given at Cargese School of Particle Physics and Cosmology: the Interface,
Cargese, Cosica, France, 4-16 Aug 2003
- "Lectures on inflation and cosmological perturbations", D. Langlois, arXiv:1001.5259 [astro-ph.CO],
Second TRR33 Winter School on cosmology, "Theory for observers & Observations for theorists",
Passo del Tonale (Italy) 7 - 12 December 2008
- "Modern cosmology", S. Dodelson
- "Physical Foundations of Cosmology", V. Mukhanov
Requirements : A knowledge of general relativity is a prerequisite for this course.
ECTS credits: 4
Diplôme(s) concerné(s)
Format des notes
Numérique sur 20Littérale/grade réduitPour les étudiants du diplôme M2 PBR - Physique par Recherche
Vos modalités d'acquisition :
Modalités/Modalities : Examen Ecrit/Written Exam.
L'UE est acquise si Note finale >= 10- Crédits ECTS acquis : 4 ECTS
Pour les étudiants du diplôme M2 HEP - Physique des Hautes Energies
Vos modalités d'acquisition :
Modalités/Modalities : Examen Ecrit/Written Exam.
Le rattrapage est autorisé (Note de rattrapage conservée)- Crédits ECTS acquis : 4 ECTS
