A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

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 explore in a parameterized manner a very large range of physically plausible equations
of state (EOSs) for compact stars for matter that is either purely hadronic or that exhibits a …

A whole decades research collated, organised and synthesised into one single book!
Following a 60-page review of the seminal treatises of Misner, Thorne, Wheeler and …

The structure of neutron stars is considered from theoretical and observational perspectives.
We demonstrate an important aspect of neutron star structure: the neutron star radius is …

An equation of state for hot, dense matter is presented in a form that is sufficiently rapid to
use directly in hydrodynamical simulations, for example, in stellar collapse calculations. It …

A radiative model for the soft gamma repeaters and the energetic 1979 March 5 burst is
presented. We identify the sources of these bursts with neutron stars the external magnetic …

Matter at high density and low temperature is expected to be a color superconductor, which
is a degenerate Fermi gas of quarks with a condensate of Cooper pairs near the Fermi …

Investigations of deconfined quark matter within NJL-type models are reviewed, focusing on
the regime of low temperatures and “moderate” densities, which is not accessible by …

The historical first detection of a binary neutron star merger by the LIGO-Virgo Collaboration
[BP Abbott et al., Phys. Rev. Lett. 119, 161101 (2017) PRLTAO 0031-9007 …