Mathematical Research Data Initiative
Main page
Recent changes
Random page
Help about MediaWiki
Create a new Item
Create a new Property
Create a new EntitySchema
Merge two items
In other projects
Discussion
View source
View history
Purge
English
Log in

On the energy in relativistic stellar dynamics

From MaRDI portal
Publication:1136505
Jump to:navigation, search

DOI10.1007/BF00762633zbMath0427.70018MaRDI QIDQ1136505

S. H. Smith

Publication date: 1977

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



Mathematics Subject Classification ID

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


Related Items

Tensor-virial equations for post-Newtonian 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, Relativistic celestial mechanics of binary stars, Newtonian dynamics of systems of extended bodies



Cites Work

  • Unnamed Item
  • Tensor-virial equations for post-Newtonian relativistic stellar dynamics
  • THE VIRAL THEOREM IN GENERAL RELATIVITY IN THE POST-NEWTONIAN APPROXIMATION
Retrieved from "https://portal.mardi4nfdi.de/w/index.php?title=Publication:1136505&oldid=13186957"
Tools
What links here
Related changes
Special pages
Printable version
Permanent link
Page information
MaRDI portal item
This page was last edited on 31 January 2024, at 04:37.
Privacy policy
About MaRDI portal
Disclaimers
Imprint
Powered by MediaWiki