Masses, radii, and the equation of state of neutron stars
We summarize our current knowledge of neutron-star masses and radii. Recent
instrumentation and computational advances have resulted in a rapid increase in the …
instrumentation and computational advances have resulted in a rapid increase in the …
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 …
GWTC-3: Compact binary coalescences observed by LIGO and Virgo during the second part of the third observing run
R Abbott, TD Abbott, F Acernese, K Ackley, C Adams… - Physical Review X, 2023 - APS
The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals detected with
Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the …
Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the …
[HTML][HTML] GW190425: Observation of a compact binary coalescence with total mass∼ 3.4 M⊙
BP Abbott, R Abbott, TD Abbott… - The Astrophysical …, 2020 - iopscience.iop.org
The first observation of gravitational waves from the inspiral of a binary neutron star (BNS)
200 system on 2017 August 17 (Abbott et al. 2017b) was a major landmark in multi …
200 system on 2017 August 17 (Abbott et al. 2017b) was a major landmark in multi …
Formation of double neutron star systems
Double neutron star (DNS) systems represent extreme physical objects and the endpoint of
an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems …
an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems …
The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations
A Burrows, D Radice, D Vartanyan… - Monthly Notices of …, 2020 - academic.oup.com
We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …
broad range of progenitor masses. This is the largest collection of sophisticated 3D …
The NANOGrav nine-year data set: mass and geometric measurements of binary millisecond pulsars
We analyze 24 binary radio pulsars in the North American Nanohertz Observatory for
Gravitational Waves (NANOGrav) nine-year data set. We make 14 significant measurements …
Gravitational Waves (NANOGrav) nine-year data set. We make 14 significant measurements …
Progenitors of gravitational wave mergers: binary evolution with the stellar grid-based code ComBinE
MU Kruckow, TM Tauris, N Langer… - Monthly Notices of …, 2018 - academic.oup.com
The first gravitational wave detections of mergers between black holes and neutron stars
represent a remarkable new regime of high-energy transient astrophysics. The signals …
represent a remarkable new regime of high-energy transient astrophysics. The signals …
On the formation history of Galactic double neutron stars
A Vigna-Gómez, CJ Neijssel… - Monthly Notices of …, 2018 - academic.oup.com
Double neutron stars (DNSs) have been observed as Galactic radio pulsars, and the recent
discovery of gravitational waves from the DNS merger GW170817 adds to the known DNS …
discovery of gravitational waves from the DNS merger GW170817 adds to the known DNS …
[HTML][HTML] 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 …