activity
20132023
most citedQuark matter in Neutron Stars within the Field Correlator Method

30 citations · 69 across the 6 of their papers we have counts for

collaborators

6 papers

hep-ph2023

Functional Renormalization Group Study of Thermodynamic Geometry Around the Phase Transition of Quantum Chromodynamic

Fabrizio Murgana, Vincenzo Greco, Marco Ruggieri +1

We investigate the thermodynamic geometry of the quark-meson model at finite temperature, , and quark number chemical potential, . We extend previous works by the inclusion o…

hep-th2023

The conformal sector of Quantum Einstein Gravity beyond the local potential approximation

Alfio Bonanno, Maria Conti, Dario Zappalà

The anomalous scaling of Newton's constant around the Reuter fixed point is dynamically computed using the functional flow equation approach. Specifically, we thoroughly analyze th…

nucl-th2020★ 16 cited

Cooling of hybrid neutron stars with microscopic equations of state

J. -B. Wei, G. F. Burgio, H. -J. Schulze +1

We model the cooling of hybrid neutron stars combining a microscopic nuclear equation of state in the Brueckner-Hartree-Fock approach with different quark models. We then analyze t…

nucl-th2015★ 22 cited

Hybrid star structure with the Field Correlator Method

G. F. Burgio, D. Zappala'

We explore the relevance of the color-flavor locking phase in the equation of state (EoS) built with the Field Correlator Method (FCM) for the description of the quark matter core…

hep-ph2013★ 1 cited

Neutron Star masses from the Field Correlator Method Equation of State

D. Zappala, G. F. Burgio, V. Greco +1

We analyse the hadron-quark phase transition in neutron stars by confronting the hadronic Equation of State (EoS) obtained according to the microscopic Brueckner-Hartree-Fock many…

hep-ph2013★ 30 cited

Quark matter in Neutron Stars within the Field Correlator Method

S. Plumari, G. F. Burgio, V. Greco +1

We discuss the appearance of quark matter in neutron star cores', focussing on the possibility that the recent observation of a very heavy neutron star could constrain free paramet…