Stable ultracompact objects

DOI10.1023/A:1018807219245zbMath0934.83018OpenAlexW1482421106MaRDI QIDQ1308429

M. C. Durgapa, Pooran Negi

Publication date: 23 November 1999

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

Full work available at URL: https://doi.org/10.1023/a:1018807219245

zbMATH Keywords

existencestability analysisstatic spherically symmetric solutionsultra-compact objects

Mathematics Subject Classification ID

Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)

Related Items (6)

The stability of an isentropic model for a gaseous relativistic star ⋮ Exact solutions of Einstein's field equations ⋮ The stability of relativistic stars and the role of the adiabatic index ⋮ HYDROSTATIC EQUILIBRIUM OF INSULAR, STATIC, SPHERICALLY SYMMETRIC, PERFECT FLUID SOLUTIONS IN GENERAL RELATIVITY ⋮ MAXIMUM MASS OF A CLASS OF COLD COMPACT STARS ⋮ NECESSARY AND SUFFICIENT CONDITION FOR HYDROSTATIC EQUILIBRIUM IN GENERAL RELATIVITY

Cites Work

• Unnamed Item
• Motion of test particles in parabolic density distributions
• General Relativistic Fluid Spheres
• Static Solutions of Einstein's Field Equations for Spheres of Fluid

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