Gravitational-wave lensing beyond rays: a disordered-system approach
Ripalta Amoruso, Ginevra Braga, Alice Garoffolo, Francescopaolo Lopez, Nicola Bartolo, Sabino Matarrese

TL;DR
This paper introduces a novel theoretical framework for modeling gravitational wave propagation through stochastic lens distributions, extending beyond geometric optics by employing disordered-system techniques.
Contribution
It develops a path-integral formalism using the Schwinger Keldysh approach to describe wave interference, diffraction, and fluctuations in a unified manner.
Findings
Derived explicit form of the averaged density matrix for wave propagation.
Identified physical scales for coherence loss in gravitational wave signals.
Applicable to wave propagation in disordered media beyond gravitational lensing.
Abstract
We develop a framework to describe gravitational wave propagation through a stochastic distribution of weak gravitational lenses beyond the geometric optics limit. We model the lens distribution as a static random background field and formulate the problem in the language of quenched disorder, treating the disorder averaged density matrix as the fundamental object from which observables are computed. Using the Schwinger Keldysh formalism, we construct a path-integral representation of the averaged density matrix and derive its explicit form perturbatively for a suitable class of couplings. The result naturally separates into a quadratic exponential term, which governs the suppression of phase sensitive contributions in the averaged description, and a purely oscillatory contribution, which modifies coherent propagation through a disorder-induced correction to the propagation kernel. This…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
