Phase transition of superdense neutron star matter

Details Phase transition of superdense neutron star matter Phase transition of superdense neutron star matter

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phlb..147..157z&link_type=abstract

Physics Letters B, Volume 147, Issue 1-3, p. 157-161.

Physics

Scientific paper

We present a lagrangian leading to a quark linear-potential model in the
static case and, using many-body theory to calculate the equation of
state, point out that the first order phase transition may occur for
superdense neutron star matter, which is important to phase transition
dynamics and shock wave formation in stellar collapse.

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