Spin precession in the gravity wave analogue black hole spacetime

TL;DR

This paper proposes a laboratory analogue experiment using fluid dynamics to observe spin precession effects similar to those near rotating black holes, enabling the study of strong gravity phenomena in a controlled setting.

Contribution

It introduces a simple experimental setup with a buoyant particle thread as a gyroscope to measure spin precession and related effects in a fluid-based black hole analogue.

Findings

Demonstrates the feasibility of measuring spin precession in a fluid analogue black hole.

Shows how to simulate Lense-Thirring and geodetic effects in laboratory conditions.

Provides a method to observe strong gravity phenomena without actual black holes.

Abstract

It was predicted that the spin precession frequency of a stationary gyroscope shows various anomalies in the strong gravity regime if its orbit shrinks, and eventually its precession frequency becomes arbitrarily high very close to the horizon of a rotating black hole. Considering the gravity waves of a flowing fluid with vortex in a shallow basin, that acts as a rotating analogue black hole, one can observe the predicted strong gravity effect on the spin precession in the laboratory. Attaching a thread with the buoyant particles and anchored it to the bottom of the fluid container with a short length of miniature chain, one can construct a simple local test gyroscope to measure the spin precession frequency in the vicinity of the gravity wave analogue black hole. The thread acts as the axis of the gyroscope. By regulating the orbital frequency of the test gyroscope, one can also be able to measure the strong gravity Lense-Thirring effect and geodetic/de-Sitter effect with this experimental set-up, as the special cases. For example, to measure the Lense-Thirring effect, the length of the miniature chain can be set to zero, so that the gyroscope becomes static. One can also measure the geodetic precession with this system by orbiting the test gyroscope in the so-called Keplerian frequency around the non-rotating analogue black hole that can be constructed by making the rotation of the fluid/vortex negligible compared to its radial velocity.