Competition between orbital effects, Pauli limiting, and Fulde-Ferrell-Larkin-Ovchinnikov states in 2D transition metal dichalcogenide superconductors
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Department of Physics, University of ArizonaIssue Date
2022Keywords
Fulde-Ferrell-Larkin-Ovchinnikov stateNbS2
NbSe2
superconductivity
transition metal dichalcogenide
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Institute of PhysicsCitation
Cho, C.-W., Ng, C. Y., Wong, C. H., Abdel-Hafiez, M., Vasiliev, A. N., Chareev, D. A., Lebed, A. G., & Lortz, R. (2022). Competition between orbital effects, Pauli limiting, and Fulde-Ferrell-Larkin-Ovchinnikov states in 2D transition metal dichalcogenide superconductors. New Journal of Physics, 24(8).Journal
New Journal of PhysicsRights
Copyright © 2022 The Author(s). Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We compare the upper critical field of bulk single-crystalline samples of the two intrinsic transition metal dichalcogenide superconductors, 2H-NbSe2 and 2H-NbS2, in high magnetic fields where their layer structure is aligned strictly parallel and perpendicular to the field, using magnetic torque experiments and a high-precision piezo-rotary positioner. While both superconductors show that orbital effects still have a significant impact when the layer structure is aligned parallel to the field, the upper critical field of NbS2 rises above the Pauli limiting field and forms a Fulde-Ferrell-Larkin-Ovchinnikov (FFLO) state, while orbital effects suppress superconductivity in NbSe2 just below the Pauli limit, which excludes the formation of the FFLO state. From the out-of-plane anisotropies, the coherence length perpendicular to the layers of 31 Å in NbSe2 is much larger than the interlayer distance, leading to a significant orbital effect suppressing superconductivity before the Pauli limit is reached, in contrast to the more 2D NbS2 © 2022 The Author(s). Published by IOP Publishing Ltd on behalf of the Institute of Physics and Deutsche Physikalische GesellschaftNote
Open access journalISSN
1367-2630Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1088/1367-2630/ac8114
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Except where otherwise noted, this item's license is described as Copyright © 2022 The Author(s). Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.