On the instability of an isentropic model for a gaseous relativistic star

DOI10.1007/BF00758956zbMath0636.76135MaRDI QIDQ1098745

Henning Knutsen

Publication date: 1988

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

zbMATH Keywords

exact solutiongaseous relativistic starisentropic perfect fluid

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Galactic and stellar dynamics (85A05)

Related Items (4)

The stability of an isentropic model for a gaseous relativistic star ⋮ General relativistic effects in the structure of massive white dwarfs ⋮ Exact solutions of Einstein's field equations ⋮ The stability of relativistic stars and the role of the adiabatic index

Cites Work

• General Relativistic 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
• Unnamed Item
• Unnamed Item
• Unnamed Item

This page was built for publication: On the instability of an isentropic model for a gaseous relativistic star