Date | Tuesday |
Thursday |
Jan 24 |
Overview |
|
Jan 29, 31 |
Linearization of Einstein equations, Lorenz
gauge, transverse-traceless gauge |
Interaction of GWs with freely-falling test
particles, key ideas underlying GW detectors |
Feb 5, 7 |
Effective EMT of GWs, GW energy and
linear-momentum fluxes |
Propagation of GWs in curved spacetime,
geometric optics approximation |
Feb 12, 14 |
Interaction of GWs with matter, gravitational
lensing, absorption and scattering |
Leading-order generation of GWs in the
slow-motion approximation for self-gravitating sources |
Feb 19, 21 |
Quadrupole formula |
GWs from binary systems |
Feb 26, 28 |
Astrophysical predictions for binary coalescing
rates |
Binaries on elliptic orbits |
March 5, 7 |
Basics of PN formalism |
Basics of PN formalism |
March 12,14 |
Numerical relativity | Numerical relativity |
March 26, 28 |
Perturbation theory and black hole quasi-normal modes | Effective-one-body formalism |
April 2, 4 |
Effective-one-body formalism | Inspiraling templates in GR and alternative theories |
April 9, 11 |
Spin effects/tidal effects/EM counterparts | GWs from rotating rigid bodies (pulsars) |
April 16, 18 |
GWs from core-collapse supernovae | GWs from the early Universe |
April 23, 25 |
Data analysis |
Data analysis |
April 30, 2 |
GWs from the early Universe | GWs from the early Universe |
May 7, 9 |
How LIGO works | Quantum-optical noise in GW detectors |
May 14 (?) |
students' presentations |
|