This review aims at providing an extensive discussion of modern constraints relevant for
dense and hot strongly interacting matter. It includes theoretical first-principle results from …

Massive (hypermassive and supramassive) neutron stars are likely to be often formed after
the merger of binary neutron stars. We explore the evolution process of the remnant massive …

We construct the equation of state (EOS) of dense matter covering a wide range of
temperature, proton fraction, and density for the use of core-collapse supernova simulations …

Background: The recent accurate measurement of the mass of two pulsars close to or above
2 M⊙ has raised the question of whether such large pulsar masses allow for the existence …

Within the covariant density functional theory of hypernuclear matter we build a series of
equations of state for hypernuclear compact stars, by calibrating the coupling constants of …

The shapes of light normal nuclei and Λ hypernuclei are investigated in the (β, γ)
deformation plane by using a newly developed constrained relativistic mean field (RMF) …

Numerical simulations for the merger of binary neutron stars are performed in full general
relativity incorporating both nucleonic and hyperonic finite-temperature equations of state …

The properties of Λ hypernuclei in a broad mass region are studied by using a deformed
Hartree-Fock approach using realistic nucleonic Skyrme forces, pairing correlations, and a …

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 deformation property of Λ hypernuclei using the relativistic mean-field (RMF)
method. We find that Λ 29 Si and Λ 13 C hypernuclei have a spherical shape as a …