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We study the properties of strange quark matter in equilibrium with normalnuclear matter. Instead of using the conventional bag model in quark sector, weachieve the confinement by a density-dependent quark mass derived fromin-medium chiral condensates. In nuclear matter, we adopt the equation of statefrom the Brueckner-Bethe-Goldstone approach with three-body forces. It is foundthat the mixed phase can occur, for a reasonable confinement parameter, nearthe normal nuclear saturation density, and goes over into pure quark matter atabout 5 times the saturation. The onset of mixed and quark phases is compatiblewith the observed class of low-mass neutron stars, but it hinders theoccurrence of kaon condensation.

Deconfinement phase transition in hybrid neutron stars from the Brueckner theory with three-body forces and a quark model with chiral mass scaling