Multipolar effective-one-body waveforms for precessing binary black holes: Construction and validation
S Ossokine, A Buonanno, S Marsat, R Cotesta… - Physical Review D, 2020 - APS
As gravitational-wave detectors become more sensitive and broaden their frequency
bandwidth, we will access a greater variety of signals emitted by compact binary systems …
bandwidth, we will access a greater variety of signals emitted by compact binary systems …
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 …
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 …
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 …
Enriching the symphony of gravitational waves from binary black holes by tuning higher harmonics
For the first time, we construct an inspiral-merger-ringdown waveform model within the
effective-one-body formalism for spinning, nonprecessing binary black holes that includes …
effective-one-body formalism for spinning, nonprecessing binary black holes that includes …
Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
In Abbott et al.[Phys. Rev. X 6, 041014 (2016) PRXHAE 2160-3308 10.1103/PhysRevX.
6.041014], the properties of the first gravitational wave detected by LIGO, GW150914, were …
6.041014], the properties of the first gravitational wave detected by LIGO, GW150914, were …
Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
We leverage recent breakthrough calculations using second-order gravitational self-force
(2GSF) theory to improve both the gravitational-mode amplitudes and radiation-reaction …
(2GSF) theory to improve both the gravitational-mode amplitudes and radiation-reaction …
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 …
Bayesian inference of binary black holes with inspiral-merger-ringdown waveforms using two eccentric parameters
A Ramos-Buades, A Buonanno, J Gair - Physical Review D, 2023 - APS
Orbital eccentricity is a crucial physical effect to unveil the origin of compact-object binaries
detected by ground-and spaced-based gravitational-wave (GW) observatories. Here, we …
detected by ground-and spaced-based gravitational-wave (GW) observatories. Here, we …
Frequency-domain reduced-order model of aligned-spin effective-one-body waveforms with higher-order modes
We present a frequency-domain reduced-order model (ROM) for the aligned-spin effective-
one-body model for binary black holes (BBHs) seobnrv4hm that includes the spherical …
one-body model for binary black holes (BBHs) seobnrv4hm that includes the spherical …