Role of Oxygen in Laser Induced Contamination at Diamond-Vacuum Interfaces

Fuente: arXiv
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Autori principali: Parthasarathy, Shreyas, Joos, Maxime, Hughes, Lillian B., Meynell, Simon A., Morrison, Taylor A., Risner-Jamtgaard, J. D., Weld, David M., Mukherjee, Kunal, Jayich, Ania C. Bleszynski
Natura: Preprint
Pubblicazione: 2024
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author Parthasarathy, Shreyas
Joos, Maxime
Hughes, Lillian B.
Meynell, Simon A.
Morrison, Taylor A.
Risner-Jamtgaard, J. D.
Weld, David M.
Mukherjee, Kunal
Jayich, Ania C. Bleszynski
author_facet Parthasarathy, Shreyas
Joos, Maxime
Hughes, Lillian B.
Meynell, Simon A.
Morrison, Taylor A.
Risner-Jamtgaard, J. D.
Weld, David M.
Mukherjee, Kunal
Jayich, Ania C. Bleszynski
contents Many modern-day quantum science experiments rely on high-fidelity measurement of fluorescent signals emitted by the quantum system under study. A pernicious issue encountered when such experiments are conducted near a material interface in vacuum is "laser-induced contamination" (LIC): the gradual accretion of fluorescent contaminants on the surface where a laser is focused. Fluorescence from these contaminants can entirely drown out any signal from e.g. optically-probed color centers in the solid-state. Crucially, while LIC appears often in this context, it has not been systematically studied. In this work, we probe the onset and growth rate of LIC for a diamond nitrogen-vacancy center experiment in vacuum, and we correlate the contamination-induced fluorescence intensities to micron-scale physical build-up of contaminant on the diamond surface. Drawing upon similar phenomena previously studied in the space optics community, we use photo-catalyzed oxidation of contaminants as a mitigation strategy. We vary the residual oxygen pressure over 9 orders of magnitude and find that LIC growth is inhibited at near-atmospheric oxygen partial pressures, but the growth rate at lower oxygen pressure is non-monotonic. Finally, we discuss a model for the observed dependence of LIC growth rate on oxygen content and propose methods to extend in situ mitigation of LIC to a wider range of operating pressures.
format Preprint
id arxiv_https___arxiv_org_abs_2401_06942
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Role of Oxygen in Laser Induced Contamination at Diamond-Vacuum Interfaces
Parthasarathy, Shreyas
Joos, Maxime
Hughes, Lillian B.
Meynell, Simon A.
Morrison, Taylor A.
Risner-Jamtgaard, J. D.
Weld, David M.
Mukherjee, Kunal
Jayich, Ania C. Bleszynski
Quantum Physics
Mesoscale and Nanoscale Physics
Many modern-day quantum science experiments rely on high-fidelity measurement of fluorescent signals emitted by the quantum system under study. A pernicious issue encountered when such experiments are conducted near a material interface in vacuum is "laser-induced contamination" (LIC): the gradual accretion of fluorescent contaminants on the surface where a laser is focused. Fluorescence from these contaminants can entirely drown out any signal from e.g. optically-probed color centers in the solid-state. Crucially, while LIC appears often in this context, it has not been systematically studied. In this work, we probe the onset and growth rate of LIC for a diamond nitrogen-vacancy center experiment in vacuum, and we correlate the contamination-induced fluorescence intensities to micron-scale physical build-up of contaminant on the diamond surface. Drawing upon similar phenomena previously studied in the space optics community, we use photo-catalyzed oxidation of contaminants as a mitigation strategy. We vary the residual oxygen pressure over 9 orders of magnitude and find that LIC growth is inhibited at near-atmospheric oxygen partial pressures, but the growth rate at lower oxygen pressure is non-monotonic. Finally, we discuss a model for the observed dependence of LIC growth rate on oxygen content and propose methods to extend in situ mitigation of LIC to a wider range of operating pressures.
title Role of Oxygen in Laser Induced Contamination at Diamond-Vacuum Interfaces
topic Quantum Physics
Mesoscale and Nanoscale Physics
url https://arxiv.org/abs/2401.06942