Gravitational radiation from Schwarzschild black holes: the second-order perturbation formalism
نویسندگان
چکیده
منابع مشابه
Gravitational Radiation from Intermediate-Mass Black Holes
Recent X-ray observations of galaxies with ROSAT, ASCA, and Chandra have revealed numerous bright off-center point sources which, if isotropic emitters, are likely to be intermediate-mass black holes, with M ∼ 102−4 M⊙. The origin of these objects is under debate, but observations suggest that a significant number of them currently reside in young high-density stellar clusters. There is also gr...
متن کاملSchwarzschild Black Holes and Propagation of Electromagnetic and Gravitational Waves. *
Disturbing of a spacetime geometry may result in the appearance of an oscillating and damped radiation the so-called quasinormal modes. Their periods of oscillations and damping coefficients carry unique information about the mass and the angular momentum, that would allow one to identify the source of the gravitational field. In this talk we present recent bounds on the diffused energy, applic...
متن کاملGravitational shock waves for Schwarzschild and Kerr black holes.
The metrics of gravitational shock waves for a Schwarzschild black hole in ordinary coordinates and for a Kerr black hole in BoyerLindquist coordinates are derived. The Kerr metric is discussed for two cases: the case of a Kerr black hole moving parallel to the rotational axis, and moving perpendicular to the rotational axis. Then, two properties from the derived metrics are investigated: the s...
متن کاملBack Reaction of Gravitational Radiation on the Schwarzschild Black Hole
We address some of the issues that appear in the study of back reaction in Schwarzschild backgrounds. Our main object is the effective energymomentum tensor (EEMT) of gravitational perturbations. It is commonly held that only asymptotically flat or radiation gauges can be employed for these purposes. We show that the traditional Regge-Wheeler gauge for the perturbations of the Schwarszchild met...
متن کاملSchwarzschild Black Holes from Matrix Theory
We consider Matrix theory compactified on T 3 and show that it correctly describes the properties of Schwarzschild black holes in 7 + 1 dimensions, including the energy–entropy relation, the Hawking temperature and the physical size, up to numerical factors of order unity. The most economical description involves setting the cut-off N in the discretized light-cone quantization to be of order th...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Physics Reports
سال: 2000
ISSN: 0370-1573
DOI: 10.1016/s0370-1573(99)00048-4