Coalescence of Two Spinning Black Holes: An Effective One-Body Approach

Details Coalescence of Two Spinning Black Holes: An Effective One-Body Approach Coalescence of Two Spinning Black Holes: An Effective One-Body Approach

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001stin...0171771d&link_type=abstract

Technical Report, PB2001-105981; IHES/P/01/11

Astronomy and Astrophysics

Astronomy

Deformation, Particle Mass, Black Holes (Astronomy), Coalescing, Binding Energy

Scientific paper

The authors generalize to the case of spinning black holes a recently introduced 'effective one-body' approach to the general relativistic dynamics of binary systems. The authors show how to approximately map the conservative part of the third post-Newtonian (3 PN) dynamics of two spinning black holes of masses m1, m2 and spins S1, S2 onto the dynamics of a non-spinning particle of mass in a certain effective metric which can be viewed either as a spin-deformation.

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