| Dato | Undervises av | Sted | Tema | Kommentarer / ressurser |
| 24.11.2004 | ?ystein? | ? | Exercise session, final words? | ? |
| 22.11.2004 | ?ystein? | ? | The CMB? | see notes? |
| 17.11.2004 | ?ystein? | ? | Statistics of density perturbations, the CMB? | see notes? |
| 15.11.2004 | ?ystein? | ? | Structure formation? | See notes? |
| 10.11.2004 | ? | ? | No problem session because of home exam 2? | ? |
| 08.11.2004 | ?ystein? | ? | Structure formation? | ? |
| 03.11.2004 | ?ystein? | ? | Structure formation? | Notes will be handed out? |
| 01.11.2004 | ?ystein? | ? | Nucleosynthesis, recombination? | C&L 8.6, 9.3? |
| 27.10.2004 | ?ystein? | ? | Problems 10,11,12,13? | ? |
| 25.10.2004 | ?ystein? | ? | Early universe thermodynamics. Neutrino decoupling. Nucleosynthesis? | C&L 8.4, 8.6? |
| 20.10.2004 | ?ystein? | ? | Problems 8,9 & start of 10 on the problem sheet handed out? | ? |
| 18.10.2004 | ?ystein? | ? | 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 | ?ystein? | ? | Inflation: reheating and density perturbations? | ? |
| 04.10.2004 | ?ystein? | ? | 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 | ?ystein? | ? | Inflation: scalar field models. ? | C&L 7.10+7.11? |
| 20.09.2004 | ?ystein? | 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 | ?ystein? | 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 | ?ystein? | 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 | ?ystein? | 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 | ?ystein? | 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 | ?ystein? | ITA? | Finish intro to GR. Introduce the Friedmann equations? | C&L 1.2,1.3,1.10,1.11? |
| 16.08.2004 | ?ystein? | ITA? | F?rst 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