Generating gravitational waveform libraries of exotic compact binaries with deep learning
(2024) In Physical Review D 109(12).- Abstract
Current gravitational wave (GW) detections rely on the existence of libraries of theoretical waveforms. Consequently, finding new physics with GWs requires libraries of nonstandard models, which are computationally demanding. We discuss how deep learning frameworks can be used to generate new waveforms "learned"from a simulation dataset obtained, say, from numerical relativity simulations. Concretely, we use the WaveGAN architecture of a generative adversarial network (GAN). As a proof of concept we provide this neural network (NN) with a sample of (>500) waveforms from the collisions of exotic compact objects (Proca stars), obtained from numerical relativity simulations. Dividing the sample into a training and a validation set, we... (More)
Current gravitational wave (GW) detections rely on the existence of libraries of theoretical waveforms. Consequently, finding new physics with GWs requires libraries of nonstandard models, which are computationally demanding. We discuss how deep learning frameworks can be used to generate new waveforms "learned"from a simulation dataset obtained, say, from numerical relativity simulations. Concretely, we use the WaveGAN architecture of a generative adversarial network (GAN). As a proof of concept we provide this neural network (NN) with a sample of (>500) waveforms from the collisions of exotic compact objects (Proca stars), obtained from numerical relativity simulations. Dividing the sample into a training and a validation set, we show that after a sufficiently large number of training epochs the NN can produce from 12% to 25% of the synthetic waveforms with an overlapping match of at least 95% with the ones from the validation set. We also demonstrate that a NN can be used to predict the overlapping match score, with 90% accuracy, of new synthetic samples. These are encouraging results for using GANs for data augmentation and interpolation in the context of GWs, to cover the full parameter space of, say, exotic compact binaries, without the need for intensive numerical relativity simulations.
(Less)
- author
- Freitas, Felipe F. ; Herdeiro, Carlos A.R. ; Morais, António P. LU ; Onofre, António ; Pasechnik, Roman LU ; Radu, Eugen ; Sanchis-Gual, Nicolas and Santos, Rui
- organization
- publishing date
- 2024-06
- type
- Contribution to journal
- publication status
- published
- subject
- in
- Physical Review D
- volume
- 109
- issue
- 12
- article number
- 124059
- publisher
- American Physical Society
- external identifiers
-
- scopus:85196951560
- ISSN
- 2470-0010
- DOI
- 10.1103/PhysRevD.109.124059
- language
- English
- LU publication?
- yes
- id
- b6cbc437-c5f9-4f3a-8fa1-db49374e2456
- date added to LUP
- 2024-10-03 15:45:39
- date last changed
- 2024-10-03 15:46:30
@article{b6cbc437-c5f9-4f3a-8fa1-db49374e2456, abstract = {{<p>Current gravitational wave (GW) detections rely on the existence of libraries of theoretical waveforms. Consequently, finding new physics with GWs requires libraries of nonstandard models, which are computationally demanding. We discuss how deep learning frameworks can be used to generate new waveforms "learned"from a simulation dataset obtained, say, from numerical relativity simulations. Concretely, we use the WaveGAN architecture of a generative adversarial network (GAN). As a proof of concept we provide this neural network (NN) with a sample of (>500) waveforms from the collisions of exotic compact objects (Proca stars), obtained from numerical relativity simulations. Dividing the sample into a training and a validation set, we show that after a sufficiently large number of training epochs the NN can produce from 12% to 25% of the synthetic waveforms with an overlapping match of at least 95% with the ones from the validation set. We also demonstrate that a NN can be used to predict the overlapping match score, with 90% accuracy, of new synthetic samples. These are encouraging results for using GANs for data augmentation and interpolation in the context of GWs, to cover the full parameter space of, say, exotic compact binaries, without the need for intensive numerical relativity simulations.</p>}}, author = {{Freitas, Felipe F. and Herdeiro, Carlos A.R. and Morais, António P. and Onofre, António and Pasechnik, Roman and Radu, Eugen and Sanchis-Gual, Nicolas and Santos, Rui}}, issn = {{2470-0010}}, language = {{eng}}, number = {{12}}, publisher = {{American Physical Society}}, series = {{Physical Review D}}, title = {{Generating gravitational waveform libraries of exotic compact binaries with deep learning}}, url = {{http://dx.doi.org/10.1103/PhysRevD.109.124059}}, doi = {{10.1103/PhysRevD.109.124059}}, volume = {{109}}, year = {{2024}}, }