Showing 2000 · gr-qcShow all

31 papers · 2 filters

gr-qc2000★ 50 cited

Hairy Black Holes, Horizon Mass and Solitons

Abhay Ashtekar, Alejandro Corichi, Daniel Sudarsky

Properties of the horizon mass of hairy black holes are discussed with emphasis on certain subtle and initially unexpected features. A key property suggests that hairy black holes…

gr-qc2000★ 62 cited

Distorted Black Holes with Charge

Stephen Fairhurst, Badri Krishnan

We present new solutions to the Einstein-Maxwell equations representing a class of charged distorted black holes. These solutions are static-axisymmetric and are generalizations of…

gr-qc2000★ 80 cited

Aperture synthesis for gravitational-wave data analysis: Deterministic Sources

Lee Samuel Finn

Gravitational wave detectors now under construction are sensitive to the phase of the incident gravitational waves. Correspondingly, the signals from the different detectors can be…

gr-qc2000★ 26 cited

Perturbations of the Kerr spacetime in horizon penetrating coordinates

Manuela Campanelli, Gaurav Khanna, Pablo Laguna +2

We derive the Teukolsky equation for perturbations of a Kerr spacetime when the spacetime metric is written in either ingoing or outgoing Kerr-Schild form. We also write explicit f…

gr-qc2000★ 106 cited

Grazing Collisions of Black Holes via the Excision of Singularities

Steve Brandt, Randall Correll, Roberto Gomez +10

We present the first simulations of non-headon (grazing) collisions of binary black holes in which the black hole singularities have been excised from the computational domain. Ini…

gr-qc2000★ 29 cited

Data conditioning for gravitational wave detectors: A Kalman filter for regressing suspension violin mode

Lee Samuel Finn, Soma Mukherjee

Interferometric gravitational wave detectors operate by sensing the differential light travel time between free test masses. Correspondingly, they are sensitive to anything that ch…

gr-qc2000★ 130 cited

Loop Quantum Cosmology IV: Discrete Time Evolution

Martin Bojowald

Using general features of recent quantizations of the Hamiltonian constraint in loop quantum gravity and loop quantum cosmology, a dynamical interpretation of the constraint equati…

gr-qc2000★ 84 cited

Loop Quantum Cosmology III: Wheeler-DeWitt Operators

Martin Bojowald

In the framework of loop quantum cosmology anomaly free quantizations of the Hamiltonian constraint for Bianchi class A, locally rotationally symmetric and isotropic models are giv…

gr-qc2000★ 9 cited

The large cosmological constant approximation to classical and quantum gravity: model examples

Rodolfo Gambini, Jorge Pullin

We have recently introduced an approach for studying perturbatively classical and quantum canonical general relativity. The perturbative technique appears to preserve many of the a…

gr-qc2000★ 13 cited

Making classical and quantum canonical general relativity computable through a power series expansion in the inverse cosmological constant

Rodolfo Gambini, Jorge Pullin

We consider general relativity with a cosmological constant as a perturbative expansion around a completely solvable diffeomorphism invariant field theory. This theory is the $Λ\to…

gr-qc2000★ 100 cited

The rotational modes of relativistic stars: Analytic results

Keith H. Lockitch, Nils Andersson, John L. Friedman

We study the r-modes and rotational ``hybrid'' modes of relativistic stars. As in Newtonian gravity, the spectrum of low-frequency rotational modes is highly sensitive to the stell…

gr-qc2000★ 11 cited

Quasi-spherical approximation for rotating black holes

Hisa-aki Shinkai, Sean A. Hayward

We numerically implement a quasi-spherical approximation scheme for computing gravitational waveforms for coalescing black holes, testing it against angular momentum by applying it…

gr-qc2000★ 240 cited

Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA

Lee Samuel Finn, Kip S. Thorne

Results are presented from high-precision computations of the orbital evolution and emitted gravitational waves for a stellar-mass object spiraling into a massive black hole in a s…

gr-qc2000★ 14 cited

Three-dimensional adaptive evolution of gravitational waves in numerical relativity

Kimberly C. B. New, Dae-Il Choi, Joan M. Centrella +3

Adaptive techniques are crucial for successful numerical modeling of gravitational waves from astrophysical sources such as coalescing compact binaries, since the radiation typical…

gr-qc2000★ 24 cited

Hyperbolic formulations and numerical relativity II: Asymptotically constrained systems of the Einstein equations

Gen Yoneda, Hisa-aki Shinkai

We study asymptotically constrained systems for numerical integration of the Einstein equations, which are intended to be robust against perturbative errors for the free evolution…

gr-qc2000★ 45 cited

Suspensions Thermal Noise in the LIGO Gravitational Wave Detector

Gabriela González

We present a calculation of the maximum sensitivity achievable by the LIGO Gravitational wave detector in construction, due to limiting thermal noise of its suspensions. We present…

gr-qc2000★ 278 cited

Generic Isolated Horizons and their Applications

Abhay Ashtekar, Christopher Beetle, Olaf Dreyer +4

Boundary conditions defining a generic isolated horizon are introduced. They generalize the notion available in the existing literature by allowing the horizon to have distortion a…

gr-qc2000★ 8 cited

Quantum Geometry of Isolated Horizons and Black Hole Entropy

A. Ashtekar, J. Baez, K. Krasnov

Using the earlier developed classical Hamiltonian framework as the point of departure, we carry out a non-perturbative quantization of the sector of general relativity, coupled to…

gr-qc2000★ 21 cited

operator for canonical quantum gravity

Yongge Ma, Yi Ling

We study the properties of operator on the kinematical Hilbert space for canonical quantum gravity. Its complete spectrum with respect to the spin network b…

gr-qc2000★ 23 cited

Constant Crunch Coordinates for Black Hole Simulations

Adrian P. Gentle, Daniel E. Holz, Arkady Kheyfets +3

We reinvestigate the utility of time-independent constant mean curvature foliations for the numerical simulation of a single spherically-symmetric black hole. Each spacelike hypers…

gr-qc2000★ 365 cited

Isolated Horizons: Hamiltonian Evolution and the First Law

Abhay Ashtekar, Stephen Fairhurst, Badri Krishnan

A framework was recently introduced to generalize black hole mechanics by replacing stationary event horizons with isolated horizons. That framework is significantly extended. The…

gr-qc2000★ 27 cited

Hyperbolic formulations and numerical relativity: Experiments using Ashtekar's connection variables

Hisa-aki Shinkai, Gen Yoneda

In order to perform accurate and stable long-time numerical integration of the Einstein equation, several hyperbolic systems have been proposed. We here present numerical compariso…

gr-qc2000★ 26 cited

Excitation of Neutron Star Oscillations by an Orbiting Particle

Johannes Ruoff, Pablo Laguna, Jorge Pullin

The excitation of neutron stars is expected to be an important source of gravitational radiation. Of fundamental importance is then to investigate mechanisms that trigger oscillati…

gr-qc2000★ 24 cited

Generic Tracking of Multiple Apparent Horizons with Level Flow

Deirdre M. Shoemaker, Mijan F. Huq, Richard A. Matzner

We report the development of the first apparent horizon locator capable of finding multiple apparent horizons in a ``generic'' numerical black hole spacetime. We use a level-flow m…