Phase transition to quark matter in neutron stars

Details Phase transition to quark matter in neutron stars Phase transition to quark matter in neutron stars

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phlb...98..140a&link_type=abstract

Physics Letters B, Volume 98, Issue 1-2, p. 140-144.

Physics

6

Scientific paper

A calculation is made of the critical density ϱt at which it is more favorable for the matter to be in the quark phase than in the nuclear one. The equation of state of the quark phase is obtained assuming that the QCD effective lagrangian satisfactorily describes the interaction at all energies, and by making a relativistic Hartree-Fock approximation. The main result we get is that ϱt > ϱm, the maximum central density of stable neutron stars.

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