Quantum State Characterization of Gravitational Waves via Graviton Counting Statistics

TL;DR

This paper proposes a method to characterize the quantum state of gravitational waves through graviton counting, enabling quantum state discrimination and tomography, which advances understanding of gravitational radiation at the quantum level.

Contribution

It introduces a technique to extract quantum state information of gravitational waves using graviton detection probabilities and correlation functions, enabling full quantum state tomography.

Findings

Graviton detection probabilities distinguish between squeezed, coherent, and thermal states.

Second-order correlation functions can be measured independently of gravitational interaction strength.

The method allows for full quantum state tomography of Gaussian gravitational wave states.

Abstract

Although gravitational waves are now routinely observed, the detection of individual gravitons has long been regarded as impossible. Recent work, however, has demonstrated that single-graviton detection can be achieved and may be feasible in the near future. Here we show that beyond mere particle detection, these detectors provide access to the quantum state and particle statistics of gravitational waves. We show that graviton detection probabilities enable the discrimination between squeezed, coherent, and thermal radiation. We further demonstrate that the full quantum statistics contained in the second-order correlation function of the passing wave can be directly measured at the detector, independent of the weak gravitational interaction strength. Building on recent quantum-optical techniques, this capability opens the way to full quantum state tomography of Gaussian states. Our results demonstrate that single-graviton detection is not only of foundational significance but also of practical value, allowing for the characterization of quantum statistics and the states of the gravitational radiation field, which remain currently unknown.