
 
 | 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 | 
          |