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 …

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 …

In this work we review the role of hyperons on the properties of neutron and proto-neutron
stars. In particular, we revise the so-called “hyperon puzzle”, go over some of the solutions …

Nuclear matter and finite nuclei exhibit the property of superfluidity by forming Cooper pairs.
We review the microscopic theories and methods that are being employed to understand the …

We review the role and properties of hyperons in finite and infinite nuclear systems. In
particular, we present different production mechanisms of hypernuclei, as well as several …

The effects of the ϕ meson on the properties of hyperon stars are studied systematically in
the framework of the density-dependent relativistic mean field (DDRMF) model. The ϕ …

Neutron star models with maximum mass close to 2 M⊙ reach high central densities, which
may activate nucleonic and hyperon direct Urca neutrino emission. To alleviate the tension …

We study the thermal evolution of hypernuclear compact stars constructed from covariant
density functional theory of hypernuclear matter and parametrizations which produce …

We study the resonant tidal excitation of g modes in coalescing superfluid neutron star (NS)
binaries and investigate how such tidal driving impacts the gravitational-wave (GW) signal of …

For core-collapse and neutron star merger simulations, it is important to have adequate
equations of state which describe dense and hot matter as realistically as possible. We …