We analyze and quantify how the color-flavor locked (CFL) phase in dense matter enhances
the parameter space for absolute stability (strange matter). We find that the “CFL strange …

Using the solutions of the gap equations of the magnetic-color-flavor-locked (MCFL) phase
of paired quark matter in a magnetic field, and taking into consideration the separation …

The distribution of masses for neutron stars is analysed using the Bayesian statistical inference,
evaluating the likelihood of the proposed Gaussian peaks by using 54 measured points …

Strange quark matter in a color flavor locked (CFL) state can be the true ground state of
hadronic matter for a much wider range of the parameters of the model (the gap of the QCD …

We calculate the evolution of close binary systems (CBSs) formed by a neutron star (behaving
as a radio pulsar) and a normal donor star, which evolve either to a helium white dwarf (…

We used the statistical measurements of information entropy, disequilibrium and complexity
to infer a hierarchy of equations of state for two types of compact stars from the broad class …

We investigate the rates of production and thermalization of ν μ and ν τ neutrinos at temperatures
and densities relevant to core-collapse supernovae and protoneutron stars. Included …

The conjecture of Bodmer–Witten–Terazawa suggesting a form of quark matter (Strange
Quark Matter) as the ground state of hadronic interactions has been studied in laboratory and …

The existence of millisecond pulsars with planet-mass companions in close orbits is
challenging from the stellar evolution point of view. We calculate in detail the evolution of binary …

The method developed by Raffelt (1990a,b,c) to estimate a possible increase in the standard
values of the helium-core mass at the tip of the red giant branch, $\Mc$, from properties of …