Interaction Energy in Geometrostatics
From MaRDI portal
Publication:5727582
DOI10.1103/PhysRev.131.471zbMath0117.23604WikidataQ27348538 ScholiaQ27348538MaRDI QIDQ5727582
Dieter Brill, Richard W. Lindquist
Publication date: 1963
Published in: Physical Review (Search for Journal in Brave)
Related Items
CTTK: a new method to solve the initial data constraints in numerical relativity ⋮ Analytic analysis of irregular discrete universes ⋮ Black-hole binaries, gravitational waves, and numerical relativity ⋮ Physics and initial data for multiple black hole spacetimes ⋮ Malaise and remedy of binary boson-star initial data ⋮ Nonlinear interactions between black holes and Proca fields ⋮ All transverse and TT tensors in flat spaces of any dimension ⋮ Applications of the close-limit approximation: horizonless compact objects and scalar fields ⋮ Solution-generating methods of Einstein’s equations by Hamiltonian reduction ⋮ Gravitational holography and trapped surfaces ⋮ Supersymmetry, attractors and cosmic censorship ⋮ Event and apparent horizon finders for \(3+1\) numerical relativity ⋮ Probing typical black hole microstates ⋮ Numerical Relativity and the Discovery of Gravitational Waves ⋮ Polyhomogeneous expansions from time symmetric initial data ⋮ Initial data for numerical relativity ⋮ A rigidity property of asymptotically simple spacetimes arising from conformally flat data ⋮ Code generation for AMReX with applications to numerical relativity ⋮ Cosmological solutions with charged black holes ⋮ The effects of self-interaction on constructing relativistic point particles ⋮ Recent progress in general relativity ⋮ Multi-localized time-symmetric initial data for the Einstein vacuum equations ⋮ Deformation of horizons during a merger ⋮ Extraction of gravitational-wave energy in higher dimensional numerical relativity using the Weyl tensor ⋮ Dyonic black holes at arbitrary locations ⋮ The closed trapped region and the apparent horizon of two Schwarzschild black holes ⋮ Double-slit interference pattern from single-slit screen and its gravitational analogues ⋮ Numerical initial data deformation exploiting a gluing construction: I. Exterior asymptotic Schwarzschild ⋮ Lie sphere geometry in lattice cosmology ⋮ Super-geometrodynamics ⋮ Black hole gluing in de Sitter space ⋮ Solutions of the Einstein constraint equations with apparent horizon boundaries ⋮ Isolated and dynamical horizons and their applications ⋮ Editorial note to: Ludwig Flamm, Contributions to Einstein's theory of gravitation ⋮ Colliding Black Holes and Gravitational Waves ⋮ Numerical approach for Corvino-type gluing of Brill–Lindquist initial data ⋮ Numerical relativity as a tool for computational astrophysics ⋮ Super-geometrodynamics in higher dimensions ⋮ Orbiting black-hole binaries and apparent horizons in higher dimensions ⋮ Decoupling the momentum constraints in general relativity ⋮ THE EFFICIENCY OF GRAVITATIONAL BREMSSTRAHLUNG PRODUCTION IN THE COLLISION OF TWO SCHWARZSCHILD BLACK HOLES ⋮ Spectral methods for numerical relativity ⋮ Aliasing instabilities in the numerical evolution of the Einstein field equations ⋮ Energy-minimizing two black holes initial data ⋮ Geometry and Regularity of Moving Punctures ⋮ Schwarzschild black hole as moving puncture in isotropic coordinates ⋮ Exact models of charged black holes. I: Geometry of totally geodesic null hypersurface ⋮ Black hole lattices under the microscope ⋮ Black-hole lattices as cosmological models ⋮ The horizons of two Schwarzschild black holes ⋮ Hamiltonian Formalism for Spinning Black Holes in General Relativity ⋮ INITIAL CONDITIONS FOR NUMERICAL RELATIVITY: INTRODUCTION TO NUMERICAL METHODS FOR SOLVING ELLIPTIC PDEs ⋮ A quasi-static approach to structure formation in black hole universes ⋮ Valiente Kroon's obstructions to smoothness at infinity
Cites Work
- Classical Physics as geometry. Gravitation, electromagnetism, unquantized charge, and mass as properties of curved empty space
- On weak time-symmetric gravitational waves
- Dynamics of a Lattice Universe by the Schwarzschild-Cell Method
- Oscillatory Character of Reissner-Nordström Metric for an Ideal Charged Wormhole
- Geometrodynamics and the Problem of Motion
- Maximal Extension of Schwarzschild Metric
- The Particle Problem in the General Theory of Relativity