Published June 25, 2024 | Version v1
Journal article

Generating gravitational waveform libraries of exotic compact binaries with deep learning

  • 1. Departamento de Física, Universidade de Aveiro, Campus de Santiago, 3810-183 Aveiro, Portugal
  • 2. Centre for Research and Development in Mathematics and Applications (CIDMA), Campus de Santiago, 3810-183 Aveiro, Portugal
  • 3. Departamento de Matemática, Universidade de Aveiro, Campus de Santiago, 3810-183 Aveiro, Portugal
  • 4. Centro de Física das Universidades do Minho e do Porto (CF-UM-UP), Universidade do Minho, 4710-057 Braga, Portugal
  • 5. Department of Astronomy and Theoretical Physics, Lund University, 221 00 Lund, Sweden
  • 6. Departamento de Astronomía y Astrofísica, Universitat de València, Dr. Moliner 50, 46100, Burjassot (València), Spain
  • 7. ISEL—Instituto Superior de Engenharia de Lisboa, Instituto Politécnico de Lisboa 1959-007 Lisboa, Portugal
  • 8. Centro de Física Teórica e Computacional, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, Edifício C8 1749-016 Lisboa, Portugal

Description

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.

Additional details

Identifiers

DOI
10.1103/PhysRevD.109.124059;
arXiv
arXiv:2203.01267;
Crossref Funder ID
10.13039/501100018711; 10.13039/501100001871; 10.13039/501100008530; 10.13039/100012470; 10.13039/100010661; 10.13039/501100023561; 10.13039/501100004837; 10.13039/501100011033; 10.13039/501100000780; 10.13039/501100004359; 10.13039/501100000781;

Publishing Information

Journal Title
Physical Review D
Journal Volume
109
Journal Issue
12
Journal Page Range
16 pgs.
ISSN
1089-4918

Optional Information