On the stability of fluid configurations having a phase transition

Details On the stability of fluid configurations having a phase transition On the stability of fluid configurations having a phase transition

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..110o&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, Jan.-Feb. 1983, p. 110-113) Soviet Astronomy (ISSN 0038-5301), vol. 27, Jan.-Feb. 1983, p. 6

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Flow Stability, Neutron Stars, Relativistic Theory, Stellar Models, Density Distribution, Incompressible Fluids, Phase Transformations, Stellar Mass

Scientific paper

The stability of stratified general-relativistic configurations is investigated in the context of configurations having a phase transition as part of a study to determine whether a phase transition can occur in neutron star material. The regions of stability are determined for the simplest case of two incompressible fluids in each of two states (one state with a density discontinuity at the surface and the other state with a density discontinuity inside the star at the phase boundary). The relativity correction is shown to expand their region of stability. Numemrical estimates are obtained for the case of rhoc/rho = 7 (where c refers to the core).

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