In recent years our understanding of neutron stars has advanced remarkably, thanks to
research converging from many directions. The importance of understanding neutron star …

Formed in the aftermath of gravitational core-collapse supernova explosions, neutron stars
are unique cosmic laboratories for probing the properties of matter under extreme conditions …

In this review article, we discuss selected developments regarding the role of the equation of
state in simulations of core-collapse supernovae. There are no first-principle calculations of …

Compact stars may contain quark matter in their interiors at densities exceeding several
times the nuclear saturation density. We explore models of such compact stars where there …

A two-phase description of the quark–nuclear matter hybrid equation of state that takes into
account the effect of excluded volume in both the hadronic and the quark-matter phases is …

We analyze the effects of chiral symmetry restoration in hadronic matter, including the lowest-
lying baryonic resonance Δ based on the parity doublet model. We study the role of Δ and its …

We show that in the three-polytrope model of Hebeler et al.[Astrophys. J. 773, 11 (2013)
AJLEEY 0004-637X 10.1088/0004-637X/773/1/11] for the neutron star equation of state …

Particles with strangeness content are predicted to populate dense matter, modifying the
equation of state of matter inside neutron stars as well as their structure and evolution. In this …

We investigate the equation of state for the recently developed hybrid quark-meson-nucleon
model under neutron-star conditions of β-equilibrium and charge neutrality. The model has …

As is pointed out in a recent work [Phys. Rev. Lett. 120, 222001 (2018)
10.1103/PhysRevLett. 120.222001], quark matter may not be strange. Inspired by this …