On the collapse of a spherically symmetric star

DOI10.1063/1.530990zbMath0841.76099OpenAlexW2165636437MaRDI QIDQ4873525

Marcus Kriele

Publication date: 16 April 1996

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.530990

zbMATH Keywords

initial value problemgeneral equation of statearea of spheres of symmetryinitial energy density

Mathematics Subject Classification ID

PDEs in connection with relativity and gravitational theory (35Q75) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Galactic and stellar dynamics (85A05)

Related Items (1)

On the critical mass of the collapse of a gaseous star in spherically symmetric and isentropic motion

Cites Work

• Black holes without singularities
• The collapse of a spherically symmetric star with linear equation of state
• A generalization of the singularity theorem of Hawking & Penrose to space-times with causality violations
• Existence and properties of spherically symmetric static fluid bodies with a given equation of state
• The formation of black holes and singularities in spherically symmetric gravitational collapse
• The initial value problem for a class of general relativistic fluid bodies
• The Maximum Mass of Ideal White Dwarfs
• On Continued Gravitational Contraction

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