Tensor-virial equations for post-Newtonian relativistic stellar dynamics

DOI10.1007/BF00762632zbMath0427.70017MaRDI QIDQ1136504

S. H. Smith

Publication date: 1977

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

zbMATH Keywords

post-Newtonian relativistic stellar dynamicstensor-virial equation, virial theorem

Mathematics Subject Classification ID

Celestial mechanics (70F15) (n)-body problems (70F10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items

On the energy in relativistic stellar dynamics, Relativistic equations of motion of extended bodies, Relativistic effects in many-body systems of finite size, internal structure, and internal motions: I. Self-acceleration of astrophysical systems, Post-Newtonian spin and angular momentum of bounded systems, The force law for the dynamic two-body problem in the second post- Newtonian approximation of general relativity, Relativistic celestial mechanics of binary stars, Celestial coordinate reference systems in curved space-time, Newtonian dynamics of systems of extended bodies, Spin precession in the relativistic two-body problem, Post-Newtonian gravitational radiation from binary stars

Cites Work

• On the energy in relativistic stellar dynamics
• Dynamics of extended bodies in general relativity center-of-mass description and quasirigidity
• The gravitational equations and the problem of motion
• THE HYDRODYNAMIC STABILITY OF INVISCID FLOW BETWEEN COAXIAL CYLINDERS
• THE VIRAL THEOREM IN GENERAL RELATIVITY IN THE POST-NEWTONIAN APPROXIMATION
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