Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2011-06-02
Class. Quantum Grav. 28 175006, 2011
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
27 pages, 4 figures
Scientific paper
10.1088/0264-9381/28/17/175006
A description of the event horizon of a perturbed Schwarzschild black hole is provided in terms of the intrinsic and extrinsic geometries of the null hypersurface. This description relies on a Gauss-Codazzi theory of null hypersurfaces embedded in spacetime, which extends the standard theory of spacelike and timelike hypersurfaces involving the first and second fundamental forms. We show that the intrinsic geometry of the event horizon is invariant under a reparameterization of the null generators, and that the extrinsic geometry depends on the parameterization. Stated differently, we show that while the extrinsic geometry depends on the choice of gauge, the intrinsic geometry is gauge invariant. We apply the formalism to solutions to the vacuum field equations that describe a tidally deformed black hole. In a first instance we consider a slowly-varying, quadrupolar tidal field imposed on the black hole, and in a second instance we examine the tide raised during a close parabolic encounter between the black hole and a small orbiting body.
Massey Ryan
Poisson Eric
Vega Ian
No associations
LandOfFree
Intrinsic and extrinsic geometries of a tidally deformed black hole does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Intrinsic and extrinsic geometries of a tidally deformed black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Intrinsic and extrinsic geometries of a tidally deformed black hole will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-222735