Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm

We report on the observation and coherent excitation of atoms on the narrow inner-shell orbital transition, connecting the erbium ground state [Xe]4f^{12}(^{3}H_{6})6s^{2} to the excited state [Xe]4f^{11}((^{4}I_{15/2})^{0})5d(^{5}D_{3/2})6s^{2}(15/2,3/2)_{7}^{0}. This transition corresponds to a wa...

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Main Authors: A. Patscheider, B. Yang, G. Natale, D. Petter, L. Chomaz, M. J. Mark, G. Hovhannesyan, M. Lepers, F. Ferlaino
Format: Article
Language:English
Published: American Physical Society 2021-09-01
Series:Physical Review Research
Online Access:http://doi.org/10.1103/PhysRevResearch.3.033256
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author A. Patscheider
B. Yang
G. Natale
D. Petter
L. Chomaz
M. J. Mark
G. Hovhannesyan
M. Lepers
F. Ferlaino
author_facet A. Patscheider
B. Yang
G. Natale
D. Petter
L. Chomaz
M. J. Mark
G. Hovhannesyan
M. Lepers
F. Ferlaino
author_sort A. Patscheider
collection DOAJ
description We report on the observation and coherent excitation of atoms on the narrow inner-shell orbital transition, connecting the erbium ground state [Xe]4f^{12}(^{3}H_{6})6s^{2} to the excited state [Xe]4f^{11}((^{4}I_{15/2})^{0})5d(^{5}D_{3/2})6s^{2}(15/2,3/2)_{7}^{0}. This transition corresponds to a wavelength of 1299 nm and is optically closed. We perform high-resolution spectroscopy to extract the g_{J} factor of the 1299-nm state and to determine the frequency shift for four bosonic isotopes. We further demonstrate coherent control of the atomic state and extract a lifetime of 178(19) ms, which corresponds to a linewidth of 0.9(1) Hz. The experimental findings are in good agreement with our semi-empirical model. In addition, we present theoretical calculations of the atomic polarizability, revealing several different magic-wavelength conditions. Finally, we make use of the vectorial polarizability and confirm a possible magic wavelength at 532 nm.
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spelling doaj.art-6b59da1fa39d4ffd8c0e0f588fffc00c2024-04-12T17:14:05ZengAmerican Physical SocietyPhysical Review Research2643-15642021-09-013303325610.1103/PhysRevResearch.3.033256Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nmA. PatscheiderB. YangG. NataleD. PetterL. ChomazM. J. MarkG. HovhannesyanM. LepersF. FerlainoWe report on the observation and coherent excitation of atoms on the narrow inner-shell orbital transition, connecting the erbium ground state [Xe]4f^{12}(^{3}H_{6})6s^{2} to the excited state [Xe]4f^{11}((^{4}I_{15/2})^{0})5d(^{5}D_{3/2})6s^{2}(15/2,3/2)_{7}^{0}. This transition corresponds to a wavelength of 1299 nm and is optically closed. We perform high-resolution spectroscopy to extract the g_{J} factor of the 1299-nm state and to determine the frequency shift for four bosonic isotopes. We further demonstrate coherent control of the atomic state and extract a lifetime of 178(19) ms, which corresponds to a linewidth of 0.9(1) Hz. The experimental findings are in good agreement with our semi-empirical model. In addition, we present theoretical calculations of the atomic polarizability, revealing several different magic-wavelength conditions. Finally, we make use of the vectorial polarizability and confirm a possible magic wavelength at 532 nm.http://doi.org/10.1103/PhysRevResearch.3.033256
spellingShingle A. Patscheider
B. Yang
G. Natale
D. Petter
L. Chomaz
M. J. Mark
G. Hovhannesyan
M. Lepers
F. Ferlaino
Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm
Physical Review Research
title Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm
title_full Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm
title_fullStr Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm
title_full_unstemmed Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm
title_short Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm
title_sort observation of a narrow inner shell orbital transition in atomic erbium at 1299 nm
url http://doi.org/10.1103/PhysRevResearch.3.033256
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