
 
  
 | 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 | |