Gravitational wave astrophysics relies heavily on the use of matched filtering both to detect signals in noisy data from detectors and to perform parameter estimation and tests of general relativity on those signals. Matched filtering relies upon prior knowledge of the signals expected to be produced by a range of astrophysical systems, such as binary black holes. These waveform signals can be computed using numerical relativity techniques, where the Einstein field equations are solved numerically, and the signal is extracted from the simulation. Numerical relativity simulations are, however, computationally expensive, leading to the need for a surrogate model which can predict waveform signals in regions of the physical parameter space whi...
We present a reduced-order surrogate model of gravitational waveforms fromnon-spinning binary black ...
Funding for Open Access provided by the UMD Libraries Open Access Publishing Fund.We propose a solut...
Gravitational-wave astronomy of compact binaries relies on theoretical models of the gravitational-w...
Gravitational wave astrophysics relies heavily on the use of matched filtering both to detect signal...
We present the first surrogate model for gravitational waveforms from the coalescence of precessing ...
Models of gravitational waveforms play a critical role in detecting and characterizing the gravitati...
A generic, noneccentric binary black hole (BBH) system emits gravitational waves (GWs) that are comp...
Simulating a binary black hole coalescence by solving Einstein’s equations is computationally expens...
We present and assess a Bayesian method to interpret gravitational wave signals from binary black ho...
We present and assess a Bayesian method to interpret gravitational wave signals from binary black ho...
Only numerical relativity simulations can capture the full complexities of binary black hole mergers...
This repository contains all publicly available numerical relativity surrogate data for waveforms pr...
We present a reduced-order surrogate model of gravitational waveforms fromnon-spinning binary black ...
Funding for Open Access provided by the UMD Libraries Open Access Publishing Fund.We propose a solut...
Gravitational-wave astronomy of compact binaries relies on theoretical models of the gravitational-w...
Gravitational wave astrophysics relies heavily on the use of matched filtering both to detect signal...
We present the first surrogate model for gravitational waveforms from the coalescence of precessing ...
Models of gravitational waveforms play a critical role in detecting and characterizing the gravitati...
A generic, noneccentric binary black hole (BBH) system emits gravitational waves (GWs) that are comp...
Simulating a binary black hole coalescence by solving Einstein’s equations is computationally expens...
We present and assess a Bayesian method to interpret gravitational wave signals from binary black ho...
We present and assess a Bayesian method to interpret gravitational wave signals from binary black ho...
Only numerical relativity simulations can capture the full complexities of binary black hole mergers...
This repository contains all publicly available numerical relativity surrogate data for waveforms pr...
We present a reduced-order surrogate model of gravitational waveforms fromnon-spinning binary black ...
Funding for Open Access provided by the UMD Libraries Open Access Publishing Fund.We propose a solut...
Gravitational-wave astronomy of compact binaries relies on theoretical models of the gravitational-w...