Lunar gravitational-wave detection
A new era of lunar exploration has begun bringing immense opportunities for science as
well. It has been proposed to deploy a new generation of observatories on the lunar surface …
well. It has been proposed to deploy a new generation of observatories on the lunar surface …
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 …
Theoretical groundwork supporting the precessing-spin two-body dynamics of the effective-one-body waveform models SEOBNRv5
Waveform models are essential for gravitational-wave (GW) detection and parameter
estimation of coalescing compact-object binaries. More accurate models are required for the …
estimation of coalescing compact-object binaries. More accurate models are required for the …
gwfish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks
An important step in the planning of future gravitational-wave (GW) detectors and of the
networks they will form is the estimation of their detection and parameter-estimation …
networks they will form is the estimation of their detection and parameter-estimation …
Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasicircular and nonspinning black hole binaries. II. The large …
A Albertini, A Nagar, A Pound, N Warburton, B Wardell… - Physical Review D, 2022 - APS
We compare recently computed waveforms from second-order gravitational self-force (GSF)
theory to those generated by a new, GSF-informed, effective one body (EOB) waveform …
theory to those generated by a new, GSF-informed, effective one body (EOB) waveform …
Sensitivity of space-based gravitational-wave interferometers to ultralight bosonic fields and dark matter
JC Yu, YH Yao, Y Tang, YL Wu - Physical Review D, 2023 - APS
Ultralight bosonic fields (ULBFs) are predicted by various theories beyond the standard
model of particle physics and are viable candidates of cold dark matter. There has been …
model of particle physics and are viable candidates of cold dark matter. There has been …
Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
S Wu, AH Nitz - Physical Review D, 2023 - APS
The next-generation (3G/XG) ground-based gravitational-wave (GW) detectors such as
Einstein Telescope (ET) and Cosmic Explorer (CE) will begin observing in the next decade …
Einstein Telescope (ET) and Cosmic Explorer (CE) will begin observing in the next decade …
Future prospects on testing extensions to through the weak lensing of gravitational waves
CT Mpetha, G Congedo, A Taylor - Physical Review D, 2023 - APS
With planned space-based and 3rd generation ground-based gravitational wave detectors
(LISA, Einstein Telescope, Cosmic Explorer), and proposed DeciHz detectors (DECIGO, Big …
(LISA, Einstein Telescope, Cosmic Explorer), and proposed DeciHz detectors (DECIGO, Big …
Hierarchical Bayesian method for constraining the neutron star equation of state with an ensemble of binary neutron star postmerger remnants
AW Criswell, J Miller, N Woldemariam, T Soultanis… - Physical Review D, 2023 - APS
Binary neutron star (BNS) postmerger gravitational-wave emission can occur in the
aftermath of a BNS merger—provided the system avoids prompt collapse to a black hole …
aftermath of a BNS merger—provided the system avoids prompt collapse to a black hole …
Worldtube excision method for intermediate-mass-ratio inspirals: Scalar-field model in dimensions
NA Wittek, M Dhesi, L Barack, HP Pfeiffer, A Pound… - Physical Review D, 2023 - APS
Binary black hole simulations become increasingly more computationally expensive with
smaller mass ratios, partly because of the longer evolution time, and partly because the …
smaller mass ratios, partly because of the longer evolution time, and partly because the …