We derive an expression for the phase shift of an atom interferometer in a gravitational field taking into account both the finite duration of the light pulses and the effect of a small perturbing potential added to a stronger uniform gravitational field, extending the well-known results for rectangular pulses and at most quadratic potentials. These refinements are necessary for a correct analysis of present-day high-resolution interferometers.

Phase shift in atom interferometers: Corrections for nonquadratic potentials and finite-duration laser pulses

Minardi F;
2019

Abstract

We derive an expression for the phase shift of an atom interferometer in a gravitational field taking into account both the finite duration of the light pulses and the effect of a small perturbing potential added to a stronger uniform gravitational field, extending the well-known results for rectangular pulses and at most quadratic potentials. These refinements are necessary for a correct analysis of present-day high-resolution interferometers.
2019
Istituto Nazionale di Ottica - INO
Inglese
99
3
033619
033619
10
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Sì, ma tipo non specificato
wave beam-splitters; inertial sensors; quantum-theory; constant
We would like to thank B. Dubetsky for useful discussions, and B. Barrett, N. Gaaloul, and G. Lamporesi for a careful reading of the manuscript. A. B. acknowledges funding from Horizon 2020 QuantERA ERA-NET - Project TAIOL. M.P. acknowledges financial support from LAPHIA-IdEx Bordeaux.
3
info:eu-repo/semantics/article
262
Bertoldi, A; Minardi, F; Prevedelli, M
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/408391
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