For seminars and other local announcements, please subscribe to sfu-cosmo mailing list.
Thursday, 23 February 2012, 14:00 in P8445B
Prof. Jonathan Thornburg (Indiana University)
Modelling extreme mass ratio binary black hole inspirals for eLISA
Consider a stellar-mass black hole (mass ∼ 10 solar masses) in a close orbit around a supermassive black hole (mass ∼ 106 solar masses). In this talk I'll discuss the challenge of trying to model the orbital dynamics and gravitational-wave (GW) emission of such an "EMRI" system as it evolves under the influence of the gravitational radiation-reaction "self-force". Because of the highly asymmetric mass ratio the orbital-decay timescale is much longer than the orbital period, so a direct "numerical relativity" solution of the Einstein equations would be both impractically expensive and insufficiently accurate. Instead, we can use methods based on black hole perturbation theory, treating the small black hole as a perturbation of a background (Schwarzschild or Kerr) spacetime. I'll outline some of the analytical and computational challenges of these analyses, describe recent progress in surmounting these challenges, and discuss EMRI systems as potential GW sources for the proposed eLISA/NGO space-based GW observatory.
Seminars in 2011:
[ See complete seminar archives | iCal feed ]
Modified by Andrei Frolov <frolov@sfu.ca> on 2023-11-01