Black holes, star clusters, and naked singularities: numerical solution of Einstein’s equations

DOI10.1098/rsta.1992.0073zbMath0777.70011OpenAlexW2086612671MaRDI QIDQ4697071

Stuart L. Shapiro, Saul A. Teukolsky

Publication date: 29 June 1993

Published in: Philosophical Transactions of the Royal Society of London. Series A: Physical and Engineering Sciences (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1098/rsta.1992.0073

zbMATH Keywords

singularityspherical symmetryaxial symmetrycollisionless gasnon-rotating gas spheroidThorne's hoop conjecture

Mathematics Subject Classification ID

Black holes (83C57) Computational methods for problems pertaining to mechanics of particles and systems (70-08) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40)

Related Items (5)

General relativistic cosmological N-body simulations. Part I. Time integration ⋮ P1–Nonconforming Polyhedral Finite Elements in High Dimensions ⋮ Dynamics of gravitational collapse in the axisymmetric Einstein–Vlasov system ⋮ An approach to stability analyses in general relativity via symplectic geometry ⋮ Repulsive gravity effects in horizon formation. Horizon remnants in naked singularities

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