Dato | Undervises av | Sted | Tema | Kommentarer / ressurser |
24.11.2004 | Øystein | Exercise session, final words | ||
22.11.2004 | Øystein | The CMB | see notes | |
17.11.2004 | Øystein | Statistics of density perturbations, the CMB | see notes | |
15.11.2004 | Øystein | Structure formation | See notes | |
10.11.2004 | No problem session because of home exam 2 | |||
08.11.2004 | Øystein | Structure formation | ||
03.11.2004 | Øystein | Structure formation | Notes will be handed out | |
01.11.2004 | Øystein | Nucleosynthesis, recombination | C&L 8.6, 9.3 | |
27.10.2004 | Øystein | Problems 10,11,12,13 | ||
25.10.2004 | Øystein | Early universe thermodynamics. Neutrino decoupling. Nucleosynthesis | C&L 8.4, 8.6 | |
20.10.2004 | Øystein | Problems 8,9 & start of 10 on the problem sheet handed out | ||
18.10.2004 | Øystein | Particles of the Standard Model, thermodynamics in the early universe | C&L 8.1,8.2,8.3 | |
13.10.2004 | No lectures this week | |||
11.10.2004 | No lectures this week | |||
06.01.2004 | Øystein | Inflation: reheating and density perturbations | ||
04.10.2004 | Øystein | The slow-roll approximation. A worked example | ||
29.09.2004 | Kathinka | Solution of home exam | ||
27.09.2004 | No lectures this week | |||
22.09.2004 | Øystein | Inflation: scalar field models. | C&L 7.10+7.11 | |
20.09.2004 | Øystein | ITA | Horizons in cosmology (C&L 2.8). Motivation for inflation: the flatness problem and the horizon problem (C&L 7.8.1, 7.9.1). Inflation: the basic idea (C&L 7.8.2) | |
15.09.2004 | Everyone | ITA | Problems 6 & 7 on the problem sheets | |
13.09.2004 | Øystein | ITA | Classical cosmological models continued: models with curvature (C&L 2.3, 2.4, 2.5) | |
08.09.2004 | Everyone | ITA | Problems 4 & 5 on the problem sheets | |
06.09.2004 | Øystein | ITA | Density parameters (C&L 1.13), the Hubble parameter as a function of redshift (C&L 2.1), classical cosmological models (C&L 2.2) | |
01.09.2004 | Everyone | Problem 2 & 3 on the problem sheets | ||
30.08.2004 | Øystein | ITA | Proper distance, Hubble's law (C&L 1.4), redshift (C&L 1.5), the deceleration parameter (C&L 1.6), distances (C&L 1.7), density parameters (C&L 1.13) | |
25.08.2004 | Øystein | ITA | Lecture+problem solving session | The continuity equation (C&L 1.10), the cosmological constant (C&L 1.12). The solution of problem 1 in the problem set, which involved solving the Friedmann equation for flat universe models with matter, radiation, or a cosmological constant. |
18.08.2004 | Øystein | ITA | Finish intro to GR. Introduce the Friedmann equations | C&L 1.2,1.3,1.10,1.11 |
16.08.2004 | Øystein | ITA | Først info om kurset og litt peptalk. Deretter: GR med harelabb | Coles & Lucchin (C&L) 1.2, 1.3 |
Undervisningsplan
Publisert 10. aug. 2004 18:51
- Sist endret 17. nov. 2004 10:27