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The hadron-quark phase transition in neutron stars

G. F. Burgio
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Abstract

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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G. F. Burgio. 2004-10-08. The hadron-quark phase transition in neutron stars. https://doi.org/10.1016/j.nuclphysa.2004.12.064

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