# Ultrasensitive Inverse Weak-Value Tilt Meter

**Authors:** Juli\'an Mart\'inez-Rinc\'on, Christopher A. Mullarkey, Gerardo I., Viza, Wei-Tao Liu, John C. Howell

arXiv: 1701.05208 · 2017-08-02

## TL;DR

This paper introduces an interferometric tilt measurement technique leveraging inverse weak-value amplification, achieving ultra-sensitive detection of tiny tilts with low noise floors, suitable for low-frequency applications.

## Contribution

The work presents a novel interferometric method using misalignment-induced signal amplification for ultra-sensitive tilt measurements, especially effective at low frequencies.

## Key findings

- Shot noise limited sensitivity of 56 frad/√Hz
- Measured noise floor of 200 frad/√Hz above 2 Hz
- Achieved a noise floor of about 70 prad/√Hz between 2 and 100 mHz

## Abstract

We present an interferometric technique for measuring ultra-small tilts. The information of a tilt in one of the mirrors of a modified Sagnac interferometer is carried by the phase difference between the counter propagating laser beams. Using a small misalignment of the interferometer, orthogonal to the plane of the tilt, a bimodal (or two-fringe) pattern is induced in the beam's transverse power distribution. By tracking the mean of such a distribution, using a split detector, a sensitive measurement of the phase is performed. With 1.2 mW of continuous-wave laser power, the technique has a shot noise limited sensitivity of 56 frad/$\sqrt{\mbox{Hz}}$, and a measured noise floor of 200 frad/$\sqrt{\mbox{Hz}}$ for tilt frequencies above 2 Hz. A tilt of 200 frad corresponds to a differential displacement of 4.0 fm in our setup. The novelty of the protocol relies on signal amplification due to the misalignment, and on good performance at low frequencies. A noise floor of about 70 prad/$\sqrt{\mbox{Hz}}$ is observed between 2 and 100 mHz.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1701.05208/full.md

## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1701.05208/full.md

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Source: https://tomesphere.com/paper/1701.05208