Study of gravitational radiation using quasi-local energy.
arXiv research
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Paper develops a new geometric framework for Kerr stability.
Derives equations for gravitational and electromagnetic perturbations of Reissner-Nordström spacetime.
Scattering theory developed for linearised gravity near Schwarzschild black hole.
We study the ellipticity and the ``Nekhoroshev stability'' (stability properties for finite, but very long, time scales) of the Riemann ellipsoids. We provide numerical evidence that the regions of ellipticity of the ellipsoids of types II and III are larger than those found by Chandrasekhar in the 60's and that all Ri…
We prove that, in the non-extreme Kerr-Newman black hole geometry, the Dirac equation has no normalizable, time-periodic solutions. A key tool is Chandrasekhar's separation of the Dirac equation in this geometry. A similar non-existence theorem is established in a more general class of stationary, axisymmetric metrics …
We consider the Cauchy problem for the massive Dirac equation in the non-extreme Kerr-Newman geometry outside the event horizon. We derive an integral representation for the Dirac propagator involving the solutions of the ODEs which arise in Chandrasekhar's separation of variables. It is proved that for initial data in…
Maxwell equations decay to Coulomb solutions on black hole spacetimes.
Carter tensor analysis aids wave equation on Kerr-Newman spacetime.