We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

Because of the development of many-body theories of nuclear matter, the long-standing,
open problem of the equation of state (EOS) of dense matter may be understood in the near …

Ages and thermal luminosities of neutron stars, inferred from observations, can be
interpreted with the aid of the neutron star cooling theory to gain information on the …

Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Thermal emission of neutron stars in soft X-ray transients (SXTs) in a quiescent state is
believed to be powered by the heat deposited in the stellar crust due to nuclear reactions …

A set of unified relativistic mean-field equations of state for hyperonic compact stars recently
built in [M. Fortin, Ad. R. Raduta, S. Avancini, and C. Providência, Phys. Rev. D 101, 034017 …

The prediction of the equation of state of hot, dense nuclear matter is one of the most
complicated and interesting problems in nuclear astrophysics. At the same time, knowledge …

Aims. We study the long-term thermal evolution of neutron stars in soft X-ray transients
(SXTs), taking the deep crustal heating into account consistently with the changes of the …

In the present study we analyse the effect of the density dependence of the symmetry energy
on the hyperonic content of neutron stars within a relativistic mean field description of stellar …

We study the properties of hot β-stable nuclear matter using equations of state derived within
the Brueckner-Hartree-Fock approach at finite temperature including consistent three-body …