Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
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 …
Binary neutron star mergers: mass ejection, electromagnetic counterparts, and nucleosynthesis
D Radice, A Perego, K Hotokezaka… - The Astrophysical …, 2018 - iopscience.iop.org
We present a systematic numerical relativity study of the mass ejection and the associated
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …
The SXS Collaboration catalog of binary black hole simulations
Accurate models of gravitational waves from merging black holes are necessary for
detectors to observe as many events as possible while extracting the maximum science …
detectors to observe as many events as possible while extracting the maximum science …
Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
Merging binaries of neutron-stars are not only strong sources of gravitational waves, but also
have the potential of revealing states of matter at densities and temperatures not accessible …
have the potential of revealing states of matter at densities and temperatures not accessible …
Improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
We improve the accuracy of the effective-one-body (EOB) waveforms that were employed
during the first observing run of Advanced LIGO for binaries of spinning, nonprecessing …
during the first observing run of Advanced LIGO for binaries of spinning, nonprecessing …
Eccentricity estimate for black hole mergers with numerical relativity simulations
V Gayathri, J Healy, J Lange, B O'Brien… - Nature …, 2022 - nature.com
The origin of black hole mergers discovered by the LIGO and Virgo gravitational-wave
observatories is currently unknown. GW190521, is the heaviest black hole merger detected …
observatories is currently unknown. GW190521, is the heaviest black hole merger detected …
Collapsars as a major source of r-process elements
DM Siegel, J Barnes, BD Metzger - Nature, 2019 - nature.com
The production of elements by rapid neutron capture (r-process) in neutron-star mergers is
expected theoretically and is supported by multimessenger observations,–of gravitational …
expected theoretically and is supported by multimessenger observations,–of gravitational …
A new moment-based general-relativistic neutrino-radiation transport code: Methods and first applications to neutron star mergers
D Radice, S Bernuzzi, A Perego… - Monthly Notices of the …, 2022 - academic.oup.com
We present a new moment-based energy-integrated neutrino transport code for neutron star
merger simulations in general relativity. In the merger context, ours is the first code to include …
merger simulations in general relativity. In the merger context, ours is the first code to include …
Multimode frequency-domain model for the gravitational wave signal from nonprecessing black-hole binaries
We present the imrphenomxhm frequency domain phenomenological waveform model for
the inspiral, merger, and ringdown of quasicircular nonprecessing black hole binaries. The …
the inspiral, merger, and ringdown of quasicircular nonprecessing black hole binaries. The …