Analytic Properties of High Spin & Large Mass-ratio Coalescences

I will review the derivation of gravitational waveforms for binaries with large mass ratios based on conformal symmetry methods. I will first motivate the astrophysics of intermediate mass ratio inspirals and black holes with very high spin. I will then turn to review the near-horizon properties of the high spin Kerr black hole and I will outline the conformal symmetry methods to derive gravitational waveforms. I will derive the key signatures of such waveforms. I will end by extending the point particle limit to finite size corrections using the Mathisson-Papapetrou-Dixon formalism.


Mardi, 12 février, 2019 - 14:00

Localisation / Location: 


Salle / Local: 

646A - Mondrian

Nom/Prénom // Last name/First name: 

G. Compère


ULB, Bruxelles

Equipe(s) organisatrice(s) / Organizing team(s): 

  • Théorie