Numerical Simulations of Black Hole Formation
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Publication:3627809
DOI10.1007/978-3-540-88460-6_5zbMath1163.83310OpenAlexW1674613445WikidataQ63410515 ScholiaQ63410515MaRDI QIDQ3627809
Publication date: 13 May 2009
Published in: Physics of Black Holes (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/978-3-540-88460-6_5
Black holes (83C57) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Software, source code, etc. for problems pertaining to relativity and gravitational theory (83-04)
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Cites Work
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- The piecewise parabolic method (PPM) for gas-dynamical simulations
- Adaptive mesh refinement for hyperbolic partial differential equations
- Uniformly high order accurate essentially non-oscillatory schemes. III
- An efficient implementation of flux formulae in multidimensional relativistic hydrodynamical codes
- The formation of supermassive black holes and the evolution of supermassive stars
- Critical collapse of the massless scalar field in axisymmetry
- Formation of Supermassive Black Holes through Fragmentation of Torodial Supermassive Stars
- Numerical stability of a new conformal-traceless 3 $plus$ 1 formulation of the Einstein equation
- Evolution of three-dimensional gravitational waves: Harmonic slicing case
- Numerical integration of Einstein’s field equations
- Normal modes of Bardeen discs - II. A sequence of n = 2 polytropes
- On Upstream Differencing and Godunov-Type Schemes for Hyperbolic Conservation Laws
- Computational Gasdynamics
- A new general purpose event horizon finder for 3D numerical spacetimes
- Evolutions in 3D numerical relativity using fixed mesh refinement
- A fast apparent horizon finder for three-dimensional Cartesian grids in numerical relativity
- Coordinate conditions in three-dimensional numerical relativity
- On the gravitational radiation from the collapse of neutron stars to rotating black holes
- Grazing Collisions of Black Holes via the Excision of Singularities
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Rotating stars in relativity
- Numerical hydrodynamics in general relativity
