About this document
Gravitational Radiation from Kerr Black Holes by Célio Lima is a document available to read on EtoBox.
1) Two collapsing objects like black holes merging can emit gravitational radiation. 2) For two equal mass objects with zero spin merging, the maximum energy released as gravitational radiation is (2-v2) times the mass of each object. 3) This places an upper limit on how efficiently mass can be converted to gravitational waves during mergers, helping understand mass loss from galaxy centers over time.
- Author
- Célio Lima
- Language
- EN