Origin of the heaviest elements: The rapid neutron-capture process
JJ Cowan, C Sneden, JE Lawler, A Aprahamian… - Reviews of Modern …, 2021 - APS
The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
Kilonovae
BD Metzger - Living reviews in relativity, 2017 - Springer
The mergers of double neutron star (NS–NS) and black hole (BH)–NS binaries are
promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The …
promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The …
INTEGRAL detection of the first prompt gamma-ray signal coincident with the gravitational-wave event GW170817
V Savchenko, C Ferrigno, E Kuulkers… - The Astrophysical …, 2017 - iopscience.iop.org
Abstract We report the INTernational Gamma-ray Astrophysics Laboratory (INTEGRAL)
detection of the short gamma-ray burst GRB 170817A (discovered by Fermi-GBM) with a …
detection of the short gamma-ray burst GRB 170817A (discovered by Fermi-GBM) with a …
Modeling GW170817 based on numerical relativity and its implications
Gravitational-wave observation together with a large number of electromagnetic
observations shows that the source of the latest gravitational-wave event, GW170817 …
observations shows that the source of the latest gravitational-wave event, GW170817 …
Constraint on the maximum mass of neutron stars using GW170817 event
We revisit the constraint on the maximum mass of cold spherical neutron stars coming from
the observational results of GW170817. We develop a new framework for the analysis by …
the observational results of GW170817. We develop a new framework for the analysis by …
Binary neutron star mergers: a review of Einstein's richest laboratory
L Baiotti, L Rezzolla - Reports on Progress in Physics, 2017 - iopscience.iop.org
In a single process, the merger of binary neutron star systems combines extreme gravity, the
copious emission of gravitational waves, complex microphysics and electromagnetic …
copious emission of gravitational waves, complex microphysics and electromagnetic …
Kilonovae
BD Metzger - Living Reviews in Relativity, 2020 - Springer
The coalescence of double neutron star (NS–NS) and black hole (BH)–NS binaries are
prime sources of gravitational waves (GW) for Advanced LIGO/Virgo and future ground …
prime sources of gravitational waves (GW) for Advanced LIGO/Virgo and future ground …
Kilonova from post-merger ejecta as an optical and near-Infrared counterpart of GW170817
M Tanaka, Y Utsumi, PA Mazzali… - Publications of the …, 2017 - academic.oup.com
Recent detection of gravitational waves from a neutron star (NS) merger event GW170817
and identification of an electromagnetic counterpart provide a unique opportunity to study …
and identification of an electromagnetic counterpart provide a unique opportunity to study …
Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
L Baiotti - Progress in Particle and Nuclear Physics, 2019 - Elsevier
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 …
Merger and mass ejection of neutron star binaries
M Shibata, K Hotokezaka - Annual Review of Nuclear and …, 2019 - annualreviews.org
Mergers of binary neutron stars and black hole–neutron star binaries are among the most
promising sources for ground-based gravitational-wave (GW) detectors and are also high …
promising sources for ground-based gravitational-wave (GW) detectors and are also high …