Chandrasekhar, S. ; Friedman, John L. (1971) Criterion for the instability of a uniformly rotating configuration in general relativity Physical Review Letters, 26 (17). pp. 1047-1050. ISSN 0031-9007
Full text not available from this repository.
Official URL: http://prl.aps.org/abstract/PRL/v26/i17/p1047_1
Related URL: http://dx.doi.org/10.1103/PhysRevLett.26.1047
Abstract
Uniformly rotating configurations in general relativity are considered, and a condition is obtained that they can be quasistatically deformed without violating any of the requirements for equilibrium. This condition extends, into the domain of the rotating stars, the criterion for the onset of dynamical instability (via a neutral mode of oscillation) that occurs by radial pulsations in nonrotating stars.
Item Type: | Article |
---|---|
Source: | Copyright of this article belongs to The American Physical Society. |
ID Code: | 70308 |
Deposited On: | 16 Nov 2011 04:16 |
Last Modified: | 16 Nov 2011 04:16 |
Repository Staff Only: item control page