2021
DOI: 10.1002/qute.202100029
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Tank‐Circuit Assisted Coupling Method for Sympathetic Laser Cooling

Abstract: The coupling of the motion of two ion species in separate Penning traps via a common tank circuit is discussed. The enhancement of the coupling assisted by the tank circuit is demonstrated by an avoided crossing behavior measurement of the motional modes of two coupled ions. An intermittent laser cooling method for sympathetic cooling is proposed and a theoretical description is provided. The technique enables tuning of the coupling strength between two ion species in separate traps and thus allows for efficie… Show more

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Cited by 8 publications
(7 citation statements)
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“…must be satisfied. Inserting this condition into equation ( 25) reproduces the previously reported formula [2,3] for the Rabi oscillation frequency. Equation ( 27) reflects the simultaneous conservation of energy and conservation of charge on the common-endcap capacitance within one Rabi cycle.…”
Section: Common-endcap Couplingsupporting
confidence: 72%
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“…must be satisfied. Inserting this condition into equation ( 25) reproduces the previously reported formula [2,3] for the Rabi oscillation frequency. Equation ( 27) reflects the simultaneous conservation of energy and conservation of charge on the common-endcap capacitance within one Rabi cycle.…”
Section: Common-endcap Couplingsupporting
confidence: 72%
“…The cooling rate for the proton is given by the local slope of the energy exchange curve, i.e. it vanishes to first order for continuously cooled 9 Be + ions [3].…”
Section: Common-endcap Couplingmentioning
confidence: 99%
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“…There are several motivations to study the hyperfine structure specifically in H + 2 . Recent efforts and proposals towards high-resolution laser spectroscopy of this ion [12][13][14] offer new opportunities to test the theory; accurate theoretical predictions of the hyperfine splitting are also likely to be required to extract spin-averaged transition frequencies, similarly to HD + [1, 2]. Moreover, H + 2 is of high astrophysical importance due to its role in the formation of H + 3 .…”
Section: Introductionmentioning
confidence: 99%