Optimal pulses for enhanced interferometer sensitivity and contrast
Optimal pulses for enhanced interferometer sensitivity and contrast
The mirrors and beamsplitters of atom interferometers often suffer from inhomogeneities in coupling strength and effective detuning because different atoms see different laser intensities, Zeeman and Doppler shifts and are in different Zeeman sub-states. This limits the fringe visibility for a simple interferometer, which falls off rapidly if extra mirrors are added, for example to increase the interferometer area. In practice, one usually therefore filters the atomic velocities/sub-states, thus losing signal, and/or restricting operation to small-area interferometers with low sensitivity.
The problem is familiar in the field of NMR, where, instead of using simple pi or pi/2 pulses, the phase and potentially amplitude are modulated during the pulse so as to make the result robust to the inhomogeneities encountered. Despite the similarities with NMR systems, the numbers, correlations and performance measures for atom interferometry are different. We have used optimal control theory to obtain robust high fidelity mirror pulses for atom interferometry. Importantly, while the designs are found by computational simulation, we can validate them experimentally, with remarkably good agreement.
We have addressed the optimization of individual mirror pulses, but the eventual aim is to optimize the interferometer as a whole: errors introduced in one pulse can be compensated at a later stage, for example. Our pulses yield high contrast without the need to filter the atomic sample and maintain this even in the case of extended pulse sequences, thus making it possible to achieve significantly larger interferometer areas than with simple pi pulses.
Saywell, Jack, Cameron
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Carey, Max
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Elcock, David, Emanuel
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Belal, Mohammad
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Kuprov, Ilya
bb07f28a-5038-4524-8146-e3fc8344c065
Freegarde, Timothy
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20 September 2018
Saywell, Jack, Cameron
da7a642a-ed67-4bd0-8959-e4c2874a8e67
Carey, Max
c2b2911d-e3a9-4537-b16e-9bbfd3b68c6c
Elcock, David, Emanuel
03ce0d6c-6a49-4a4d-8caf-71b32b254ac4
Belal, Mohammad
33550de9-0df1-4c90-bae6-3eb65c62778a
Kuprov, Ilya
bb07f28a-5038-4524-8146-e3fc8344c065
Freegarde, Timothy
01a5f53b-d406-44fb-a166-d8da9128ea7d
Saywell, Jack, Cameron, Carey, Max, Elcock, David, Emanuel, Belal, Mohammad, Kuprov, Ilya and Freegarde, Timothy
(2018)
Optimal pulses for enhanced interferometer sensitivity and contrast.
Frontiers in Matter Wave Optics, , Crete, Greece.
17 - 21 Sep 2018.
Record type:
Conference or Workshop Item
(Poster)
Abstract
The mirrors and beamsplitters of atom interferometers often suffer from inhomogeneities in coupling strength and effective detuning because different atoms see different laser intensities, Zeeman and Doppler shifts and are in different Zeeman sub-states. This limits the fringe visibility for a simple interferometer, which falls off rapidly if extra mirrors are added, for example to increase the interferometer area. In practice, one usually therefore filters the atomic velocities/sub-states, thus losing signal, and/or restricting operation to small-area interferometers with low sensitivity.
The problem is familiar in the field of NMR, where, instead of using simple pi or pi/2 pulses, the phase and potentially amplitude are modulated during the pulse so as to make the result robust to the inhomogeneities encountered. Despite the similarities with NMR systems, the numbers, correlations and performance measures for atom interferometry are different. We have used optimal control theory to obtain robust high fidelity mirror pulses for atom interferometry. Importantly, while the designs are found by computational simulation, we can validate them experimentally, with remarkably good agreement.
We have addressed the optimization of individual mirror pulses, but the eventual aim is to optimize the interferometer as a whole: errors introduced in one pulse can be compensated at a later stage, for example. Our pulses yield high contrast without the need to filter the atomic sample and maintain this even in the case of extended pulse sequences, thus making it possible to achieve significantly larger interferometer areas than with simple pi pulses.
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Published date: 20 September 2018
Venue - Dates:
Frontiers in Matter Wave Optics, , Crete, Greece, 2018-09-17 - 2018-09-21
Identifiers
Local EPrints ID: 425404
URI: http://eprints.soton.ac.uk/id/eprint/425404
PURE UUID: 03ddad9f-b958-4958-aa34-a283019f7bee
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Date deposited: 18 Oct 2018 16:30
Last modified: 23 Feb 2023 02:58
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Contributors
Author:
Jack, Cameron Saywell
Author:
Max Carey
Author:
David, Emanuel Elcock
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