Perturbation of the Kerr Metric
arXiv:1401.0866
Abstract
A new Kerr-like metric with quadrupole moment is obtained by means of perturbing the Kerr spacetime. By comparison with the exterior Hartle-Thorne metric, it is showed that it could be matched to an interior solution. This metric may represent the spacetime of an astrophysical object.
References in corpus (5)
- Global General Relativistic MHD Simulation of a Tilted Black-Hole Accretion Disk
- Realistic Exact Solution for the Exterior Field of a Rotating Neutron Star
- Gravitational field of compact objects in general relativity
- Exterior and interior metrics with quadrupole moment
- Wavefronts and Light Cones for Kerr Spacetimes