Isolated Newtonian dust stars are unstable but can be stabilized by exterior matter

DOI10.1023/A:1010230204300zbMath0989.83022MaRDI QIDQ5947423

Urs M. Schaudt, Herbert Pfister

Publication date: 16 October 2001

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

zbMATH Keywords

Newtonian gravitydust starsrotating dust stars

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (1)

The interior solution of axially symmetric, stationary and rigidly rotating dust configurations

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• On uniformly rotating stars
• On the Dirichlet problem for the stationary and axisymmetric Einstein equations
• Newtonian potential theory for unbounded sources and applications to free boundary problems
• Elliptic partial differential equations of second order
• A constraint on the pressure in static stellar models
• General Relativistic Gravitational Field of a Rigidly Rotating Disk of Dust: Solution in Terms of Ultraelliptic Functions
• Null geodesics in a rotating dust cloud
• IX.—The Gravitational Field of a Distribution of Particles Rotating about an Axis of Symmetry

This page was built for publication: Isolated Newtonian dust stars are unstable but can be stabilized by exterior matter