Stability of strange quark stars with nuclear crusts against radial oscillations

Details Stability of strange quark stars with nuclear crusts against radial oscillations Stability of strange quark stars with nuclear crusts against radial oscillations

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994sqm..symp....1k&link_type=abstract

Presented at the Symposium on Strangeness and Quark Matter, Crete, Greece, 1-5 Sep. 1994

Computer Science

Crusts, Dwarf Stars, Oscillations, Quarks, Stability, Strangeness, Neutron Stars, Unsteady Flow

Scientific paper

This paper investigates the stability of the complete sequence of strange-matter stars with nuclear crusts against radial pulsations (acoustical modes). It is found that a broad class of white dwarf- like strange stars is stable against such pulsations. The same holds for the much denser strange stars, which are the strange counter-parts of neutron stars. All stars possessing still higher central densities (e.g., charm stars) turn out to be unstable.

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