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We study the hadron-quark phase transition in the interior of neutron stars(NS). For the hadronic sector, we use a microscopic equation of state (EOS)involving nucleons and hyperons derived within the Brueckner-Bethe-Goldstonemany-body theory, with realistic two-body and three-body forces. For thedescription of quark matter, we employ both the MIT bag model with a densitydependent bag constant, and the color dielectric model. We calculate thestructure of NS interiors with the EOS comprising both phases, and we find thatthe NS maximum masses are never larger than 1.7 solar masses, no matter themodel chosen for describing the pure quark phase.Comment: 11 pages, 5 figures, submitted to Phys. Rev.

Hybrid stars with the color dielectric and the MIT bag models