The hadron-quark phase transition in neutron stars

Details The hadron-quark phase transition in neutron stars The hadron-quark phase transition in neutron stars

2004-10-08

arxiv.org/abs/nucl-th/0410040v1

Nucl.Phys. A749 (2005) 337-340

Physics

Nuclear Physics

Nuclear Theory

Talk given at the 18th International Nuclear Physics Divisional Conference of the EPS, Prague, 23-29 August, 2004. To be publi

Scientific paper

10.1016/j.nuclphysa.2004.12.064

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-Hartree-Fock approach. For the quark sector, we employ the MIT bag model, as well as the Nambu--Jona-Lasinio (NJL) and the Color Dielectric (CD) models, and find that the NS maximum masses lie in the interval between 1.5 and 1.8 solar masses.

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