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Neutron stars and the nuclear equation of state
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 …
and phenomenological models, which are employed to construct the equation of state of …
Neutron-star tidal deformability and equation-of-state constraints
Despite their long history and astrophysical importance, some of the key properties of
neutron stars are still uncertain. The extreme conditions encountered in their interiors …
neutron stars are still uncertain. The extreme conditions encountered in their interiors …
Heavy baryons in compact stars
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 …
covariant density functional approach to the equation of state and composition of dense …
Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
In this article, I introduce ideas and techniques to extract information about the equation of
state of matter at very high densities from gravitational waves emitted before, during and …
state of matter at very high densities from gravitational waves emitted before, during and …
Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections
Gravitational waves emitted from the coalescence of neutron star binaries open a new
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …
Tidal deformability with sharp phase transitions in binary neutron stars
S Han, AW Steiner - Physical Review D, 2019 - APS
The neutron star tidal deformability is a critical parameter which determines the premerger
gravitational-wave signal in a neutron star merger. In this article, we show how neutron star …
gravitational-wave signal in a neutron star merger. In this article, we show how neutron star …
Dark matter effects on the properties of neutron stars: Compactness and tidal deformability
We systematically study the observable properties of dark-matter admixed neutron stars with
arbitrary dark-matter fraction, employing a realistic nuclear equation of state in combination …
arbitrary dark-matter fraction, employing a realistic nuclear equation of state in combination …
[HTML][HTML] Status and perspectives of continuous gravitational wave searches
The birth of gravitational wave astronomy was triggered by the first detection of a signal
produced by the merger of two compact objects (also known as a compact binary …
produced by the merger of two compact objects (also known as a compact binary …
Constraints on the maximum mass of neutron stars with a quark core from GW170817 and NICER PSR J0030+ 0451 data
We perform a Bayesian analysis of the maximum mass M TOV of neutron stars with a quark
core, incorporating the observational data from tidal deformability of the GW170817 binary …
core, incorporating the observational data from tidal deformability of the GW170817 binary …
Dark matter effects on the properties of neutron stars: Optical radii
We study the effects of dark matter on the properties of neutron stars by employing a DM-
admixed model. The Brueckner–Hartree–Fock theory with realistic three-body forces and a …
admixed model. The Brueckner–Hartree–Fock theory with realistic three-body forces and a …