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Gauge conditions for long-term numerical black hole evolutions without excision

Gauge conditions for long-term numerical black hole evolutions without excision

http://www.wikidata.org/entity/Q27345273

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Introduction to dynamical horizons in numerical relativity Spin flips and precession in black-hole-binary mergers Accurate Evolutions of Orbiting Black-Hole Binaries without Excision Evolving a puncture black hole with fixed mesh refinement Foundations of multiple-black-hole evolutions Wave zone extraction of gravitational radiation in three-dimensional numerical relativity Numerical simulation of orbiting black holes Maximum Gravitational Recoil Continuum and Discrete Initial-Boundary Value Problems and Einstein's Field Equations.Exploring New Physics Frontiers Through Numerical Relativity.End Point of the Ultraspinning Instability and Violation of Cosmic Censorship.End Point of Black Ring Instabilities and the Weak Cosmic Censorship Conjecture.Black-hole universe: time evolution.Orbital evolution of extreme-mass-ratio black-hole binaries with numerical relativity.Accurate evolution of orbiting binary black holes.Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity.Numerical Hydrodynamics in General Relativity Last orbit of binary black holes Numerical simulations with a first-order BSSN formulation of Einstein’s field equations Generalized harmonic equations in3+1form Trumpet slices of the Schwarzschild-Tangherlini spacetime Generalized harmonic spatial coordinates and hyperbolic shift conditions Hyperbolicity of the Kidder-Scheel-Teukolsky formulation of Einstein’s equations coupled to a modified Bona-Masso slicing condition Numerical relativity in spherical polar coordinates: Evolution calculations with the BSSN formulation BSSN equations in spherical coordinates without regularization: Vacuum and nonvacuum spherically symmetric spacetimes Gravitational waves in dynamical spacetimes with matter content in the fully constrained formulation Matter effects on binary neutron star waveforms

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Gauge conditions for long-term numerical black hole evolutions without excision

http://www.wikidata.org/entity/Q27345273

description

2003 nî lūn-bûn

@nan

2003 թուականի Ապրիլին հրատարակուած գիտական յօդուած

@hyw

2003 թվականի ապրիլին հրատարակված գիտական հոդված

@hy

2003年の論文

@ja

2003年学术文章

@wuu

2003年学术文章

@zh-cn

2003年学术文章

@zh-hans

2003年学术文章

@zh-my

2003年学术文章

@zh-sg

2003年學術文章

@yue

name

Gauge conditions for long-term numerical black hole evolutions without excision

@ast

Gauge conditions for long-term numerical black hole evolutions without excision

@en

Gauge conditions for long-term numerical black hole evolutions without excision

@nl

type

label

Gauge conditions for long-term numerical black hole evolutions without excision

@ast

Gauge conditions for long-term numerical black hole evolutions without excision

@en

Gauge conditions for long-term numerical black hole evolutions without excision

@nl

prefLabel

Gauge conditions for long-term numerical black hole evolutions without excision

@ast

Gauge conditions for long-term numerical black hole evolutions without excision

@en

Gauge conditions for long-term numerical black hole evolutions without excision

@nl

P1433

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P356

PHYSREVD.67.084023

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Physical Review D

P1476

Gauge conditions for long-term numerical black hole evolutions without excision

@en

P2093

Bernd Brügmann

http://www.w3.org/2001/XMLSchema#string

Denis Pollney

http://www.w3.org/2001/XMLSchema#string

Edward Seidel

http://www.w3.org/2001/XMLSchema#string

Michael Koppitz

http://www.w3.org/2001/XMLSchema#string

Miguel Alcubierre

http://www.w3.org/2001/XMLSchema#string

Peter Diener

http://www.w3.org/2001/XMLSchema#string

Ryoji Takahashi

http://www.w3.org/2001/XMLSchema#string

P2860

Kinematical conditions in the construction of spacetime

The Lazarus project: A pragmatic approach to binary black hole evolutions

Modeling gravitational radiation from coalescing binary black holes

Plunge Waveforms from Inspiralling Binary Black Holes

Three-dimensional numerical relativity: The evolution of black holes

Interaction Energy in Geometrostatics

Grazing Collisions of Black Holes via the Excision of Singularities

Simple excision of a black hole in 3 + 1 numerical relativity

New Formalism for Numerical Relativity

A Simple Construction of Initial Data for Multiple Black Holes

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scholarly article

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10.1103/PHYSREVD.67.084023

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8

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67

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2003-04-24T00:00:00Z

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gr-qc/0206072

http://www.w3.org/2001/XMLSchema#string

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