On spherically symmetric stellar models in general relativity (Q1290847)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: On spherically symmetric stellar models in general relativity |
scientific article; zbMATH DE number 1295041
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | On spherically symmetric stellar models in general relativity |
scientific article; zbMATH DE number 1295041 |
Statements
On spherically symmetric stellar models in general relativity (English)
0 references
3 June 1999
0 references
The non-relativistic theory of stellar structure investigates the linearized equation for small perturbations near spherically symmetric equilibria of a self-gravitating gas sphere. These results are extended and carried to the corresponding problem in general relativity. The investigation starts with the so-called Tolman-Oppenheimer-Volkoff equation describing spherically symmetric equilibrium configurations in general relativity.
0 references
relativistic stellar structure
0 references
Tolman-Oppenheimer-Volkoff equation
0 references
spherically symmetric equilibrium configurations
0 references