Published April 11, 2025 | Version Published
Journal Article Open

Digital Discovery of Interferometric Gravitational Wave Detectors

  • 1. ROR icon Max Planck Institute for the Science of Light
  • 2. ROR icon California Institute of Technology

Abstract

Gravitational waves, detected a century after they were first theorized, are space-time distortions caused by some of the most cataclysmic events in the Universe, including black hole mergers and supernovae. The successful detection of these waves has been made possible by ingenious detectors designed by human experts. Beyond these successful designs, the vast space of experimental configurations remains largely unexplored, offering an exciting territory potentially rich in innovative and unconventional detection strategies. Here, we demonstrate an intelligent computational strategy to explore this enormous space, discovering unorthodox topologies for gravitational wave detectors that significantly outperform the currently best-known designs under realistic experimental constraints. This increases the potentially observable volume of the Universe by up to 50-fold. Moreover, by analyzing the best solutions from our superhuman algorithm, we uncover entirely new physics ideas at their core. At a bigger picture, our methodology can readily be extended to AI-driven design of experiments across wide domains of fundamental physics, opening fascinating new windows into the Universe.

Copyright and License

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Open access publication funded by the Max Planck Society.

Acknowledgement

The authors thank Daniel D. Brown and Anna C. Green for very informative discussions about the finesse simulator and Haixing Miao for reviewing our manuscript and useful comments that improved our presentation. The authors are thankful to the support of the Quantum Noise Working Group and the Advanced Interferometer Configurations Working Group. Y. D. and R. X. A. are supported by the National Science Foundation (NSF) (PHY-0823459 and PHY-1764464). R. X. A. acknowledges support provided by the Institute for Quantum Information and Matter, an NSF Physics Frontiers Center (NSF Grant No. PHY-1733907).

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Additional details

Related works

Is new version of
Discussion Paper: arXiv:2312.04258 (arXiv)

Funding

National Science Foundation
PHY-0823459
National Science Foundation
PHY-1764464
National Science Foundation
PHY-1733907

Dates

Accepted
2025-02-21

Caltech Custom Metadata

Caltech groups
Institute for Quantum Information and Matter, LIGO, Division of Physics, Mathematics and Astronomy (PMA)
Publication Status
Published