# Speedmeter scheme for gravitational-wave detectors based on EPR quantum   entanglement

**Authors:** E. Knyazev, S. Danilishin, S. Hild, F. Ya. Khalili

arXiv: 1701.01694 · 2017-10-25

## TL;DR

This paper introduces an EPR-based quantum speed meter scheme for gravitational-wave detectors that enhances low-frequency sensitivity with minimal hardware modifications.

## Contribution

It presents a novel implementation of a quantum speed meter using EPR entanglement, improving sensitivity below 30 Hz in gravitational-wave detection.

## Key findings

- Significantly improved sensitivity below 30 Hz.
- Compatible with existing interferometer topologies.
- Allows switching between position and speed measurement modes.

## Abstract

We propose a new implementation of a quantum speed meter QND measurement scheme. It employs two independent optical readouts of the interferometer test masses, featuring strongly different values of the bandwidths $\gamma_{1,2}$ and of the optical circulating power $I_{1,2}$, with the special relationship of $I_1/I_2=\gamma_1/\gamma_2$. The outputs of these two position meters have to be combined by an additional beamsplitter. In this scheme, signals at the common and the differential outputs of the interferometer setup are proportional to the position and the velocity of the test masses, respectively. The influence of the position meter-like back action force associated with the position signal can be cancelled using the EPR approach by measuring the amplitude quadrature of the beamsplitter common output correlated with this force. In the standard signal-recycled Michelson interferometer topology of the modern gravitational-wave detectors, two independent optical position meters can be implemented by two orthogonal polarisations of the probe light. Our analysis shows that the EPR speedmeter provides significantly improved sensitivity for all frequencies below $\sim 30\,{\rm Hz}$ compared to an equivalent signal recycled Michelson interferometer. We believe the EPR speedmeter scheme to be very attractive for future upgrades of gravitational wave detectors, because it requires only minor changes to be implemented in the interferometer hardware and allows to switch between the position meter and the speed meter modes within short time-scales and without any changes to the hardware.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1701.01694/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1701.01694/full.md

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Source: https://tomesphere.com/paper/1701.01694