We review the physics of hyperons and Δ-resonances in dense matter in compact stars. The
covariant density functional approach to the equation of state and composition of dense …

We investigate how current and proposed observations of neutron stars can lead to an
understanding of the state of their interiors and the key unknowns: the typical neutron star …

There has recently been growing evidence for the existence of neutron stars possessing
magnetic fields with strengths that exceed the quantum critical field strength of 4.4× 10 13 G …

We discuss neutron stars with strong magnetic mean fields in the framework of Extended
Theories of Gravity. In particular, we take into account models derived from f (R) and f (Script …

The properties of matter are drastically modified by strong magnetic fields, B≫ me 2 e 3 c/ħ
3= 2.35× 10 9 G (1 G= 10− 4 T), as are typically found on the surfaces of neutron stars. In …

Over the last decade, numerical solutions of Quantum Chromodynamics (QCD) using the
technique of lattice QCD have developed to a point where they are beginning to connect …

The equation of state of a system of fermions in a uniform magnetic field is obtained in terms
of the thermodynamic quantities of the theory by using functional methods. It is shown that …

We study static neutron stars with poloidal magnetic fields and a simple class of electric
current distributions consistent with the requirement of stationarity. For this class of electric …

Observations of thermal radiation from neutron stars can potentially provide information
about the states of supranuclear matter in the interiors of these stars with the aid of the …

In the present work we use the large-N c approximation to investigate quark matter
described by the SU (2) Nambu–Jona-Lasinio model subject to a strong magnetic field. The …