Criterion for the Instability of a Uniformly Rotating Configuration in General Relativity

Details Criterion for the Instability of a Uniformly Rotating Configuration in General Relativity Criterion for the Instability of a Uniformly Rotating Configuration in General Relativity

Apr 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971phrvl..26.1047c&link_type=abstract

Physical Review Letters, vol. 26, Issue 17, pp. 1047-1050

Physics

5

Scientific paper

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.

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