Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
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
Self-force and radiation reaction in general relativity
L Barack, A Pound - Reports on Progress in Physics, 2018 - iopscience.iop.org
The detection of gravitational waves from binary black-hole mergers by the LIGO–Virgo
Collaboration marks the dawn of an era when general-relativistic dynamics in its most …
Collaboration marks the dawn of an era when general-relativistic dynamics in its most …
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 …
Comparison of post-Minkowskian and self-force expansions: Scattering in a scalar charge toy model
We compare numerical self-force results and analytical fourth-order post-Minkowskian (PM)
calculations for hyperbolic-type scattering of a pointlike particle carrying a scalar charge Q …
calculations for hyperbolic-type scattering of a pointlike particle carrying a scalar charge Q …
Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
Scientific analysis for the gravitational wave detector LISA will require theoretical waveforms
from extreme-mass-ratio inspirals (EMRIs) that extensively cover all possible orbital and spin …
from extreme-mass-ratio inspirals (EMRIs) that extensively cover all possible orbital and spin …
Comparing second-order gravitational self-force, numerical relativity, and effective one body waveforms from inspiralling, quasicircular, and nonspinning black hole …
We present the first systematic comparison between gravitational waveforms emitted by
inspiralling, quasicircular and nonspinning black hole binaries computed with three different …
inspiralling, quasicircular and nonspinning black hole binaries computed with three different …
Waveform modelling for the laser interferometer space antenna
LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave
astronomy. As the first anticipated space-based gravitational-wave detector, it will expand …
astronomy. As the first anticipated space-based gravitational-wave detector, it will expand …
Eccentric self-forced inspirals into a rotating black hole
We develop the first model for extreme mass-ratio inspirals (EMRIs) into a rotating massive
black hole driven by the gravitational self-force (GSF). Our model is based on an action …
black hole driven by the gravitational self-force (GSF). Our model is based on an action …
Precisely computing bound orbits of spinning bodies around black holes. I. General framework and results for nearly equatorial orbits
LV Drummond, SA Hughes - Physical Review D, 2022 - APS
Very large mass ratio binary black hole systems are of interest both as a clean limit of the
two-body problem in general relativity, as well as for their importance as sources of low …
two-body problem in general relativity, as well as for their importance as sources of low …
Metric perturbations of Kerr spacetime in Lorenz gauge: Circular equatorial orbits
We construct the metric perturbation in Lorenz gauge for a compact body on a circular
equatorial orbit of a rotating black hole (Kerr) spacetime, using a newly-developed method …
equatorial orbit of a rotating black hole (Kerr) spacetime, using a newly-developed method …