Speaker
Jinbiao Wei
(INFN - National Institute for Nuclear Physics)
Description
The appearance of quark matter may show a different property with traditional NS in the cooling process. With this purpose, we investigate the cooling of hybrid star. For the hadronic sector, we use a microscopic EOS derived within the Brueckner-Hartree-Fock many-body theory with realistic two-body and three-body forces. For the description of quark matter, we employ the Dyson-Schwinger quark model. We also consider the MIT bag model and field correlator method for the comparison. We find that once the quark matter appears, the hybrid star initiates a fast cooling again even the hadronic sector is suppressed by the pairing gaps.
Authors
Jinbiao Wei
(INFN - National Institute for Nuclear Physics)
Fiorella Burgio
(INFN Sezione di Catania)
Dr
Hans Schulze
(INFN-Catania)
