Upper mass limit for neutron star stability against black hole formation
| Data(s) |
1978
|
|---|---|
| Resumo |
Starting from the exact general relativistic expression for the total energy of selfgravitating spherically distributed matter and using the minimum energy priciple, we calculate the upper mass limit for a neutron star to be 3.1 solar masses. |
| Formato |
application/pdf |
| Identificador |
http://eprints.iisc.ernet.in/33497/1/mass.pdf Krishan, V and Kumar, N (1978) Upper mass limit for neutron star stability against black hole formation. In: Astrophysics and Space Science, 57 (1). 241-243 . |
| Publicador |
Springer |
| Relação |
http://www.springerlink.com/content/q6643516702g321g/ http://eprints.iisc.ernet.in/33497/ |
| Palavras-Chave | #Physics |
| Tipo |
Journal Article PeerReviewed |
