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Ultrathin two-dimensional superconductivity with strong spin-orbit coupling.


ABSTRACT: We report on a study of epitaxially grown ultrathin Pb films that are only a few atoms thick and have parallel critical magnetic fields much higher than the expected limit set by the interaction of electron spins with a magnetic field, that is, the Clogston-Chandrasekhar limit. The epitaxial thin films are classified as dirty-limit superconductors because their mean-free paths, which are limited by surface scattering, are smaller than their superconducting coherence lengths. The uniformity of superconductivity in these thin films is established by comparing scanning tunneling spectroscopy, scanning superconducting quantum interference device (SQUID) magnetometry, double-coil mutual inductance, and magneto-transport, data that provide average superfluid rigidity on length scales covering the range from microscopic to macroscopic. We argue that the survival of superconductivity at Zeeman energies much larger than the superconducting gap can be understood only as the consequence of strong spin-orbit coupling that, together with substrate-induced inversion-symmetry breaking, produces spin splitting in the normal-state energy bands that is much larger than the superconductor's energy gap.

SUBMITTER: Nam H 

PROVIDER: S-EPMC5035894 | biostudies-other | 2016 Sep

REPOSITORIES: biostudies-other

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Ultrathin two-dimensional superconductivity with strong spin-orbit coupling.

Nam Hyoungdo H   Chen Hua H   Liu Tijiang T   Kim Jisun J   Zhang Chendong C   Yong Jie J   Lemberger Thomas R TR   Kratz Philip A PA   Kirtley John R JR   Moler Kathryn K   Adams Philip W PW   MacDonald Allan H AH   MacDonald Allan H AH   Shih Chih-Kang CK  

Proceedings of the National Academy of Sciences of the United States of America 20160906 38


We report on a study of epitaxially grown ultrathin Pb films that are only a few atoms thick and have parallel critical magnetic fields much higher than the expected limit set by the interaction of electron spins with a magnetic field, that is, the Clogston-Chandrasekhar limit. The epitaxial thin films are classified as dirty-limit superconductors because their mean-free paths, which are limited by surface scattering, are smaller than their superconducting coherence lengths. The uniformity of su  ...[more]

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