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arXiv:gr-qc/0304027 · International Journal of Modern Physics D

QUANTUM INTERFERENCE TO MEASURE SPACETIME CURVATURE: A PROPOSED EXPERIMENT AT THE INTERSECTION OF QUANTUM MECHANICS AND GENERAL RELATIVITY

R. Y. Chiao, Achilles D. Speliotopoulos

Published Oct 1, 2003• 11 citations
arXivHTMLPDF

Abstract

An experiment in Low Earth Orbit (LEO) is proposed to measure components of the Riemann curvature tensor using atom interferometry. We show that the difference in the quantum phase Δϕ of an atom that can travel along two intersecting geodesics is given by mR0i0j/ℏ times the spacetime volume contained within the geodesics. Our expression for Δϕ also holds for gravitational waves in the long wavelength limit.

DOI
10.1142/s0218271803003943

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An experiment in Low Earth Orbit (LEO) is proposed to measure components of the Riemann curvature tensor using atom interferometry. We show that the difference in the quantum phase Δϕ of an atom that can travel along two intersecting geodesics is given by mR0i0j/ℏ times the spacetime volume contained within the geodesics. Our expression for Δϕ also holds for gravitational waves in the long wavelength limit.
This thesis examines how atomic quantum systems can be utilized to probe spacetime effects in regimes where quantum mechanics and general relativity intersect, and how gravitational phenomena imprint on experimentally accessible observables. The work is based on two complementary studies. In Article I, we propose an experimental scheme that combines trapped-atom interferometry with Ramsey interrogation to realize a clock held in a spatial superposition at two heights in Earth’s gravitational field. Using a path-integral treatment of interferometric phases and incorporating the internal-energy contribution to mass, we derive leading relativistic corrections and identify two signatures of proper-time superposition: (i) oscillations of interferometric visibility and (ii) an effective shift of the clock transition frequency. We argue that this frequency-shift signature may be within reach of current or near-term technology, even when visibility changes are too small to resolve. In Article II, we develop a general framework for spontaneous emission in curved spacetime and apply it to a gravitational-wave background. We demonstrate that gravitational waves can induce spectral sidebands and directional modulations in the emitted radiation, and formulate parameter estimation via Fisher-information-based sensitivity bounds, yielding order-of-magnitude requirements for detectability under idealized measurement conditions.
This paper explores a possible bridge between quantum matter-wave phase and spacetime curvature. The conservative starting point is the established relation between relativistic action, proper time, and quantum phase: for massive matter, the accumulated phase is determined by the proper-time integral along a worldline. In curved spacetime, this makes matter-wave phase sensitive to the metric geometry. Building on this relation, the paper asks whether matter-wave phase may acquire additional curvature-dependent contributions beyond the standard proper-time action phase. Such a contribution would not replace quantum mechanics or general relativity. Instead, it would represent a controlled covariant correction that becomes physically meaningful only if it produces calculable and falsifiable deviations in matter-wave interferometry, precision clock comparisons, gravitational redshift tests, or related high-precision experiments. The central proposal is that quantum phase, proper time, and spacetime curvature may be linked through a deeper action-geometric structure. In this view, phase is not treated merely as a formal parameter on a fixed background, but as a possible probe of how matter samples spacetime geometry. The paper does not claim a completed theory of everything. It identifies a concrete research direction: new physics may appear as measurable curvature-dependent corrections to phase accumulation. This work is Part III of the series The Geometry of Phase. Parts I and II reconstructed quantum interference and de Broglie matter waves from a phase-first perspective within standard physics. The present paper extends that line of thought toward curvature-coupled matter-wave phase and possible experimentally testable deviations. This manuscript is intended as a conceptual and exploratory foundations paper. It separates established reconstruction from speculative extension and provides a mathematical starting point for future tests of curvature-coupled quantum phase.
The influence of space-time curvature on quantum matter which can be theoretically described by covariant wave equations has not been experimentally established yet. In this paper we analyze in detail the suitability of the Ramsey atom beam interferometer for the measurement of the phase shift caused by the Riemannian curvature of the Earth or alternatively of two parallel oriented lead blocks. It appears that for the lead blocks the detection should be possible with realistic modifications of existing devices within the near future. For the Earth's gravitational field the experimental difficulties are too big. The paper is divided into two parts. The first one is concerned with the derivation of general relativistic correction terms to the Pauli equation starting from the fully covariant Dirac equation and their physical interpretation. The inertial effects of acceleration and rotation are included. The calculation makes use of Fermi coordinates. In the second part we calculate the shift of the Ramsey fringes for the two different sources of curvature and examine various possibilities to enlarge the sensitivity of the apparatus to space-time curvature. Since the two parts may be more or less interesting for physicists with different research fields they are written in such a way that each one may be read without much reference to the other one.
Atom interferometry is a natural laboratory for precision tests of general relativity, but there is no simple relationship between atom interferometer phase and geometric properties of spacetime. Here we show that a different atom interferometer observable, the phase shear, can be expressed directly as the integrated sectional curvature over a spacetime surface enclosed by the interferometer arms and final beamsplitter. This is a consequence of a generalized Gauss-Bonnet theorem, which also explicitly computes small correction terms arising from gravitational redshift of atom optics pulses. This synthesis of quantum mechanics, relativity, and differential geometry affords a manifestly coordinate-free and representation-free means of measuring spacetime properties. Additionally, it provides a convenient computational tool for predicting atom interferometer properties in arbitrary background spacetimes.
An experiment to test for relativistic frame dragging effects with quantum interferometry is proposed. The idea that the classical trajectories of the interferometer surround a spherical mass source whose angular momentum is perpendicular to the plane containing these trajectories. A simple analysis allows one to find the phase shift for particles traveling in the innermost stable circular orbit; the result can be easily generalized for more realistic orbits. The phase difference goes like the source's angular momentum per mass times the quantum particles' mass. This is a small effect but it can be amplified by making the classical paths go around the source several times. Moreover, this experiment has the advantage that the source's angular momentum can be easily controlled.