Modeling the horizon-absorbed gravitational flux for equatorial-circular orbits in Kerr spacetime

Modeling the horizon-absorbed gravitational flux for equatorial-circular orbits in Kerr spacetime

We propose an improved analytical model for the horizon-absorbed gravitational-wave energy flux of a small body in circular orbit in the equatorial plane of a Kerr black hole. Post-Newtonian (PN) theory provides an analytical description of the multipolar components of the absorption flux through Ta...

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Bibliographic Details
Main Authors: Taracchini, Andrea (Author), Buonanno, Alessandra (Author), Khanna, Gaurav (Author), Hughes, Scott A (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor), Hughes, Scott A. (Contributor)
Format: Article
Language:English
Published: American Physical Society, 2013-10-16T13:27:55Z.
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