Physics
Scientific paper
Apr 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phrvd..23.1715a&link_type=abstract
Physical Review D (Particles and Fields), Volume 23, Issue 8, 15 April 1981, pp.1715-1722
Physics
9
Scientific paper
A calculation is made of the critical density ρt at which it is more favorable for matter to be in the quark phase than in the nuclear phase. The equation of state of the quark phase is obtained assuming that the quantumchromodynamic 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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