|
|||
MASS 2026 Course: Gravitation and Cosmology |
|||
Lecture |
Presentation |
||
|---|---|---|---|
| Syllabus: course overview | odp | ||
Part 1: General Relativity |
|||
| 01. | General Relativity as a geometric theory of gravitation, spacetime, manifolds, scalars, vectors and dual vectors: contravariant and covariant transformation rules |
odp | |
| 02. | Tensors: transformation rules, metric (fundamental) tensor and tensor algebra |
odp | |
| 03. | Reference frames, basics of Special Relativity, Minkowski spacetime, Lorentz transformations, energy-momentum tensor and perfect fluid |
odp | |
| 04. | Basic principles of General Relativity: principle of equivalence and principle of general covariance, locally inertial frame, affine connection, geodesic equation |
odp | |
| 05. | Covariant differentiation, parallel transport, minimal-coupling principle, Riemann-Christoffel curvature tensor, Ricci tensor and scalar curvature |
odp | |
| 06. | Lagrangian, action, Hamilton's principle of least action, Einstein-Hilbert action, matter action, calculus of variations, Einstein field equations |
odp | |
| 07. | Vacuum solutions: Schwarzschild, Kerr, Reissner-Nordström and Kerr-Newman metric, classic Solar System tests of GR and Lense-Thirring effect |
zip | |
| 08. | Other experimental tests: black holes, single and binary supermassive black holes, their shadows, relativistically broadened spectral lines and gravitational waves |
zip | |
Part 2: Cosmology |
|||
| 09. | Cosmological principle, Friedmann-Lemaître-Robertson-Walker metric, Friedmann equations, cosmological parameters, standard ΛCDM cosmological model |
zip | |
| 10. | Distance measures in cosmology: proper and comoving distance, angular diameter distance, luminosity distance, distance-duality relation |
zip | |
| 11. | Observational cosmology: determination of cosmological parameters using Type Ia supernovae and cosmic microwave background radiation |
zip | |
| 12. | Gravitational lenses (basic principles, types and cosmological applications), problems of the ΛCDM model: Hubble tension and cosmological constant problem |
zip | |