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 …
Compact binary coalescences: Astrophysical processes and lessons learned
On 11 February 2016, the LIGO and Virgo scientific collaborations announced the first direct
detection of gravitational waves, a signal caught by the LIGO interferometers on 14 …
detection of gravitational waves, a signal caught by the LIGO interferometers on 14 …
Fast flavor instability in hypermassive neutron star disk outflows
R Fernández, S Richers, N Mulyk, S Fahlman - Physical Review D, 2022 - APS
We examine the effect of neutrino flavor transformation by the fast flavor instability (FFI) on
long-term mass ejection from accretion disks formed after neutron star mergers. Neutrino …
long-term mass ejection from accretion disks formed after neutron star mergers. Neutrino …
Dark photon superradiance: Electrodynamics and multimessenger signals
N Siemonsen, C Mondino, D Egana-Ugrinovic… - Physical Review D, 2023 - APS
We study the electrodynamics of a kinetically mixed dark photon cloud that forms through
superradiance around a spinning black hole, and design strategies to search for the …
superradiance around a spinning black hole, and design strategies to search for the …
Black-hole–Neutron-star Mergers Are Unlikely Multimessenger Sources
G Fragione - The Astrophysical Journal Letters, 2021 - iopscience.iop.org
The promise by the LIGO/Virgo/Kagra (LVK) collaboration to detect black-hole–neutron-star
(BH–NS) mergers via gravitational wave (GW) emission has recently been fulfilled with the …
(BH–NS) mergers via gravitational wave (GW) emission has recently been fulfilled with the …
A broad grid of 2D kilonova emission models
Depending upon the properties of their compact remnants and the physics included in the
models, simulations of neutron star mergers can produce a broad range of ejecta properties …
models, simulations of neutron star mergers can produce a broad range of ejecta properties …
Kilonova detectability with wide-field instruments
Kilonovae are ultraviolet, optical, and infrared transients powered by the radioactive decay
of heavy elements following a neutron star merger. Joint observations of kilonovae and …
of heavy elements following a neutron star merger. Joint observations of kilonovae and …
Target-of-opportunity observations of gravitational-wave events with Vera C. Rubin observatory
I Andreoni, R Margutti, OS Salafia… - The Astrophysical …, 2022 - iopscience.iop.org
The discovery of the electromagnetic counterpart to the binary neutron star (NS) merger
GW170817 has opened the era of gravitational-wave multimessenger astronomy. Rapid …
GW170817 has opened the era of gravitational-wave multimessenger astronomy. Rapid …
No detectable kilonova counterpart is expected for o3 neutron star–black hole candidates
We analyze the tidal disruption probability of potential neutron star–black hole (NSBH)
merger gravitational-wave (GW) events, including GW190426_152155, GW190814 …
merger gravitational-wave (GW) events, including GW190426_152155, GW190814 …
A tale of two mergers: constraints on kilonova detection in two short GRBs at z ∼ 0.5
B O'Connor, E Troja, S Dichiara… - Monthly Notices of …, 2021 - academic.oup.com
We present a detailed multiwavelength analysis of two short gamma-ray bursts (sGRBs)
detected by the Neil Gehrels Swift Observatory: GRB 160624A at= 0.483 and GRB 200522A …
detected by the Neil Gehrels Swift Observatory: GRB 160624A at= 0.483 and GRB 200522A …