30 citations · 30 across the 1 of their papers we have counts for
6 papers
Phase structure of hadronic and Polyakov-loop extended NJL model at finite isospin density
Rafael Cavagnoli, Debora P. Menezes, Constança Providência
It is believed that there exists a rich phase structure of quantum chromodynamics (QCD) at finite temperature and baryon density, namely, the deconfinement process from hadron gas…
Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars
Constança Providência, Sidney S. Avancini, Rafael Cavagnoli +7
In this work we study the effect of the symmetry energy on several properties of neutron stars. First, we discuss its effect on the density, proton fraction and pressure of the neu…
Neutron star properties and the symmetry energy
Rafael Cavagnoli, Constança Providência, Debora P. Menezes
The effect of the symmetry energy on the properties of compact stars is discussed. It is shown that, for stars with masses above 1 , the radius of the star varies linearly…
Hadron-quark phase transition in asymmetric matter with boson condensation
Rafael Cavagnoli, Constança Providência, Debora P. Menezes
In the present work we study the hadron-quark phase transition with boson condensation in asymmetric matter by investigating the binodal surface and extending it to finite temperat…
Radiatively Induced Non Linearity in the Walecka Model
Rafael Cavagnoli, Marcus Benghi Pinto
We evaluate the effective potential for the conventional linear Walecka non perturbatively up to one loop. This quantity is then renormalized with a prescription which allows finit…
The importance of strange mesons in neutron star properties
Rafael Cavagnoli, Debora Peres Menezes
In order to obtain the properties of compact stellar objects, appropriate equations of state have to be used. In the literature, strange meson fields, namely the scalar meson field…