ar X iv : g r - qc / 0 11 10 01 v 3 1 4 Fe b 20 02 OU - TAP - 167 Calculating the gravitational self force in Schwarzschild spacetime
نویسندگان
چکیده
Leor Barack, Yasushi Mino, Hiroyuki Nakano, Amos Ori, and Misao Sasaki Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, Am Mühlenberg 1, D-14476 Golm, Germany Theoretical Astrophysics, California institute of Technology, Pasadena, California 91125 Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan Department of Physics, Technion—Israel Institute of Technology, Haifa, 32000, Israel (February 7, 2008)
منابع مشابه
ar X iv : g r - qc / 0 50 20 46 v 2 1 1 Fe b 20 05 Gravitational quasinormal modes for Kerr Anti - de Sitter black holes
We investigate the quasinormal modes for gravitational perturbations of rotating black holes in four dimensional Anti-de Sitter (AdS) spacetime. The study of the quasinormal frequencies related to these modes is relevant to the AdS/CFT correspondence. Although results have been obtained for Schwarzschild and Reissner-Nordstrom AdS black holes, quasinormal frequencies of Kerr-AdS black holes are...
متن کاملar X iv : g r - qc / 0 70 20 29 v 1 5 Fe b 20 07 Papapetrou Energy - Momentum Tensor for Chern - Simons Modified Gravity
We construct a conserved, symmetric energy-momentum (pseudo-)tensor for Chern-Simons modified gravity, thus demonstrating that the theory is Lorentz invariant. The tensor is discussed in relation to other gravitational energy-momentum tensors and analyzed for the Schwarzschild, Reissner-Nordstrom, and FRW solutions. To our knowledge this is the first confirmation that the Reissner-Nordstrom and...
متن کاملar X iv : g r - qc / 0 60 30 86 v 3 1 6 Fe b 20 07 A statistical mechanical problem in Schwarzschild space - time
Abstract We use Fermi coordinates to calculate the canonical partition function for an ideal gas in a circular geodesic orbit in Schwarzschild spacetime. To test the validity of the results we prove theorems for limiting cases. We recover the Newtonian gas law subject only to tidal forces in the Newtonian limit. Additionally we recover the special relativistic gas law as the radius of the orbit...
متن کاملar X iv : h ep - t h / 05 02 10 9 v 1 1 1 Fe b 20 05 The Self - Gravitational Corrections as the Source for Stiff Matter on the Brane in SAdS 5 Bulk
A D3− brane with non-zero energy density is considered as the boundary of a five dimensional Schwarzschild anti de Sitter bulk background. Taking into account the semi-classical corrections to the black hole entropy that arise as a result of the self-gravitational effect, and employing the AdS/CFT correspondence, we obtain the self-gravitational correction to the first Friedmann-like equation. ...
متن کاملar X iv : g r - qc / 9 90 20 08 v 1 2 F eb 1 99 9 The Inner Structure of Black Holes
We study the gravitational collapse of a self-gravitating charged scalar-field. Starting with a regular spacetime, we follow the evolution through the formation of an apparent horizon, a Cauchy horizon and a final central singularity. We find a null, weak, mass-inflation singularity along the Cauchy horizon, which is a precursor of a strong, spacelike singularity along the r = 0 hypersurface. T...
متن کامل