Spinning solutions in general relativity with infinite central density

DOI10.1007/S10714-018-2371-7zbMath1392.83013arXiv1606.04343OpenAlexW2427211083MaRDI QIDQ725367

P. D. Flammer

Publication date: 1 August 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1606.04343

zbMATH Keywords

gravitationgeneral relativityneutron starsnumerical relativityinfinite central densityspinning solutions

Mathematics Subject Classification ID

Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

On the asymptotic behavior of static perfect fluids

Cites Work

• Numerical Relativity
• Rapidly rotating general relativistic stars - II. Differentially rotating polytropes
• Rapidly rotating general relativistic stars - I. Numerical method and its application to uniformly rotating polytropes
• Dynamical non-axisymmetric instabilities in rotating relativistic stars
• General Relativistic Polytropic Fluid Spheres.
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
• On Massive Neutron Cores

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