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This research proposes a novel quantum optical magnetometry technique using direct ultraviolet detection of noble gas nuclear spins, eliminating the need for alkali vapors to achieve hours-long spin relaxation at room temperature. The analysis identifies critical operational regimes where high laser power and low intensity noise are essential to surpass current cryogenic magnetometer performance, predicting record-breaking sensitivities achievable with standard UV laser specifications.
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Towards noble gas quantum optical magnetometry using direct ultraviolet detection

arXiv2 min read

arXiv:2609.38633v1 Announce Type: new Abstract: We analyze a novel approach for quantum magnetic sensing via optical detection of nuclear spin precession in a noble gas. The detection is carried out with an ultraviolet frequency comb laser, so no alkali vapor is required to be mixed with the noble gas during the sensing stage, allowing for hours-long spin relaxation time at room temperature. Our analysis reveals that combining high laser power and low laser intensity noise is crucial to achieving and exceeding state-of-the-art magnetometric performance, including that of cryogenic magnetometers. We find operational regimes where either fundamental or technical noise dominate, which directs experimental effort towards increasing laser power or lowering laser intensity noise, respectively. We also show that optimizing beam size is key to achieving optimal sensitivity. Our calculations predict that a record-breaking sensitivity of $24~\mathrm{aT}/\sqrt{\mathrm{Hz}}$ is achievable in 10 minutes with a 10 W ultraviolet laser with a relative intensity noise of -100 dBc/Hz.

Abstract:We analyze a novel approach for quantum magnetic sensing via optical detection of nuclear spin precession in a noble gas. The detection is carried out with an ultraviolet frequency comb laser, so no alkali vapor is required to be mixed with the noble gas during the sensing stage, allowing for hours-long spin relaxation time at room temperature. Our analysis reveals that combining high laser power and low laser intensity noise is crucial to achieving and exceeding state-of-the-art magnetometric performance, including that of cryogenic magnetometers. We find operational regimes where either fundamental or technical noise dominate, which directs experimental effort towards increasing laser power or lowering laser intensity noise, respectively. We also show that optimizing beam size is key to achieving optimal sensitivity. Our calculations predict that a record-breaking sensitivity of $24~\mathrm{aT}/\sqrt{\mathrm{Hz}}$ is achievable in 10 minutes with a 10 W ultraviolet laser with a relative intensity noise of -100 dBc/Hz.

Quantum Physics (quant-ph); Applied Physics (physics.app-ph); Atomic Physics (physics.atom-ph); Instrumentation and Detectors (physics.ins-det)

arXiv:2609.38633 [quant-ph]

(or arXiv:2609.38633v1 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2609.38633 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

https://doi.org/10.1103/nqvv-hbym Focus to learn more DOI(s) linking to related resources

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Full text under the publisher's open licence · 264 words

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