New horizons for fundamental physics with LISA
KG Arun, E Belgacem, R Benkel, L Bernard… - Living Reviews in …, 2022 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders
about the fundamental theory of nature at play in the extreme gravity regime, where the …
about the fundamental theory of nature at play in the extreme gravity regime, where the …
The dynamics of binary neutron star mergers and GW170817
D Radice, S Bernuzzi, A Perego - Annual Review of Nuclear …, 2020 - annualreviews.org
With the first observation of a binary neutron star merger through gravitational waves and
light, GW170817, compact binary mergers have now taken the center stage in nuclear …
light, GW170817, compact binary mergers have now taken the center stage in nuclear …
Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
Spin precession is one of the key physical effects that coul unveil the origin of the compact
binaries detected by ground-and space-based gravitational-wave (GW) detectors, and shed …
binaries detected by ground-and space-based gravitational-wave (GW) detectors, and shed …
Laying the foundation of the effective-one-body waveform models SEOBNRv5: Improved accuracy and efficiency for spinning nonprecessing binary black holes
We present SEOBNRv5HM, a more accurate and faster inspiral-merger-ringdown
gravitational waveform model for quasicircular, spinning, nonprecessing binary black holes …
gravitational waveform model for quasicircular, spinning, nonprecessing binary black holes …
[引用][C] Model Comparison from LIGO–Virgo Data on GW170817's Binary Components and Consequences for the Merger Remnant
BP Abbott, R Abbott, TD Abbott, S Abraham… - Default …, 2020 - andrews.elsevierpure.com
Model Comparison from LIGO–Virgo Data on GW170817’s Binary Components and
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …
Improving the NRTidal model for binary neutron star systems
T Dietrich, A Samajdar, S Khan, NK Johnson-McDaniel… - Physical Review D, 2019 - APS
Accurate and fast gravitational waveform (GW) models are essential to extract information
about the properties of compact binary systems that generate GWs. Building on previous …
about the properties of compact binary systems that generate GWs. Building on previous …
Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections
T Dietrich, T Hinderer, A Samajdar - General Relativity and Gravitation, 2021 - Springer
Gravitational waves emitted from the coalescence of neutron star binaries open a new
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …
Second-order self-force calculation of gravitational binding energy in compact binaries
Self-force theory is the leading method of modeling extreme-mass-ratio inspirals (EMRIs),
key sources for the gravitational-wave detector LISA. It is well known that for an accurate …
key sources for the gravitational-wave detector LISA. It is well known that for an accurate …
Modeling frequency-dependent tidal deformability for environmental black hole mergers
Motivated by events in which black holes can lose their environment due to tidal interactions
in a binary system, we develop a waveform model in which the tidal deformability …
in a binary system, we develop a waveform model in which the tidal deformability …
Effective-one-body waveforms for precessing coalescing compact binaries with post-Newtonian twist
Spin precession is a generic feature of compact binary coalescences that leaves clear
imprints in the gravitational waveforms. Building on previous work, we present an efficient …
imprints in the gravitational waveforms. Building on previous work, we present an efficient …