The evolution of binary neutron star post-merger remnants: a review
Two neutron stars merge somewhere in the Universe approximately every 10 to 100 s,
creating violent explosions potentially observable in gravitational waves and across the …
creating violent explosions potentially observable in gravitational waves and across the …
QCD equations of state and speed of sound in neutron stars
T Kojo - AAPPS Bulletin, 2021 - Springer
Neutron stars are cosmic laboratories to study dense matter in quantum chromodynamics
(QCD). The observable mass-radius relations of neutron stars are determined by QCD …
(QCD). The observable mass-radius relations of neutron stars are determined by QCD …
Science with the Einstein Telescope: a comparison of different designs
M Branchesi, M Maggiore, D Alonso… - … of Cosmology and …, 2023 - iopscience.iop.org
Abstract The Einstein Telescope (ET), the European project for a third-generation
gravitational-wave detector, has a reference configuration based on a triangular shape …
gravitational-wave detector, has a reference configuration based on a triangular shape …
Model comparison from LIGO–Virgo data on GW170817's binary components and consequences for the merger remnant
BP Abbott, R Abbott, TD Abbott… - … and Quantum Gravity, 2020 - iopscience.iop.org
GW170817 is the very first observation of gravitational waves originating from the
coalescence of two compact objects in the mass range of neutron stars, accompanied by …
coalescence of two compact objects in the mass range of neutron stars, accompanied by …
RAPID: early classification of explosive transients using deep learning
D Muthukrishna, G Narayan, KS Mandel… - Publications of the …, 2019 - iopscience.iop.org
Abstract We present Real-time Automated Photometric IDentification (RAPID), a novel time
series classification tool capable of automatically identifying transients from within a day of …
series classification tool capable of automatically identifying transients from within a day of …
A long-lived neutron star merger remnant in GW170817: constraints and clues from X-ray observations
Multimessenger observations of GW170817 have not conclusively established whether the
merger remnant is a black hole (BH) or a neutron star (NS). We show that a long-lived …
merger remnant is a black hole (BH) or a neutron star (NS). We show that a long-lived …
Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817
BP Abbott, R Abbott, TD Abbott… - The Astrophysical …, 2019 - iopscience.iop.org
The binary neutron star (BNS) observation GW170817 (Abbott et al. 2017d) was the first
multimessenger astronomy event to be jointly detected in gravitational waves (GWs) and at …
multimessenger astronomy event to be jointly detected in gravitational waves (GWs) and at …
The afterglow and kilonova of the short GRB 160821B
E Troja, AJ Castro-Tirado… - Monthly Notices of …, 2019 - academic.oup.com
ABSTRACT GRB 160821B is a short duration gamma-ray burst (GRB) detected and
localized by the Neil Gehrels Swift Observatory in the outskirts of a spiral galaxy at z …
localized by the Neil Gehrels Swift Observatory in the outskirts of a spiral galaxy at z …
A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger
Mergers of neutron stars are known to be associated with short γ-ray bursts,,–. If the neutron-
star equation of state is sufficiently stiff (that is, the pressure increases sharply as the density …
star equation of state is sufficiently stiff (that is, the pressure increases sharply as the density …
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 …