Intrinsic Paramagnetic Meissner Effect due to s-wave Odd-Frequency Superconductivity

dc.contributor.authorDi Bernardo, Angelo
dc.contributor.authorSalman, Zaher
dc.contributor.authorWang, Xiaolei
dc.contributor.authorAmado, Mario
dc.contributor.authorEgilmez, Mehmet
dc.contributor.authorFlokstra, Machiel G.
dc.contributor.authorSuter, Andreas
dc.contributor.authorLee, Steve L.
dc.contributor.authorZhao, Jianhua
dc.contributor.authorRobinson, Jason W. A.
dc.date.accessioned2020-01-20T13:57:55Z
dc.date.available2020-01-20T13:57:55Z
dc.date.issued2015eng
dc.description.abstractIn 1933, Meissner and Ochsenfeld reported the expulsion of magnetic flux, the diamagnetic Meissner effect, from the interior of superconducting lead. This discovery was crucial in formulating the Bardeen-Cooper-Schrieffer (BCS) theory of superconductivity. In exotic superconducting systems BCS theory does not strictly apply. A classical example is a superconductor-magnet hybrid system where magnetic ordering breaks time-reversal symmetry of the superconducting condensate and results in the stabilisation of an odd-frequency superconducting state. It has been predicted that under appropriate conditions, odd-frequency superconductivity should manifest in the Meissner state as fluctuations in the sign of the magnetic susceptibility meaning that the superconductivity can either repel (diamagnetic) or attract (paramagnetic) external magnetic flux. Here we report local probe measurements of faint magnetic fields in a Au/Ho/Nb trilayer system using low energy muons, where antiferromagnetic Ho (4.5 nm) breaks time-reversal symmetry of the proximity induced pair correlations in Au. From depth-resolved measurements below the superconducting transition of Nb we observe a local enhancement of the magnetic field in Au that exceeds the externally applied field, thus proving the existence of an intrinsic paramagnetic Meissner effect arising from an odd-frequency superconducting state.eng
dc.description.versionpublishedeng
dc.identifier.arxiv1605.02199eng
dc.identifier.doi10.1103/PhysRevX.5.041021eng
dc.identifier.ppn1687895996
dc.identifier.urihttps://kops.uni-konstanz.de/handle/123456789/48284
dc.language.isoengeng
dc.rightsAttribution 3.0 Unported
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/
dc.subject.ddc530eng
dc.titleIntrinsic Paramagnetic Meissner Effect due to s-wave Odd-Frequency Superconductivityeng
dc.typeJOURNAL_ARTICLEeng
dspace.entity.typePublication
kops.citation.bibtex
@article{DiBernardo2015Intri-48284,
  year={2015},
  doi={10.1103/PhysRevX.5.041021},
  title={Intrinsic Paramagnetic Meissner Effect due to s-wave Odd-Frequency Superconductivity},
  number={4},
  volume={5},
  journal={Physical Review X},
  author={Di Bernardo, Angelo and Salman, Zaher and Wang, Xiaolei and Amado, Mario and Egilmez, Mehmet and Flokstra, Machiel G. and Suter, Andreas and Lee, Steve L. and Zhao, Jianhua and Robinson, Jason W. A.},
  note={Article Number: 041021}
}
kops.citation.iso690DI BERNARDO, Angelo, Zaher SALMAN, Xiaolei WANG, Mario AMADO, Mehmet EGILMEZ, Machiel G. FLOKSTRA, Andreas SUTER, Steve L. LEE, Jianhua ZHAO, Jason W. A. ROBINSON, 2015. Intrinsic Paramagnetic Meissner Effect due to s-wave Odd-Frequency Superconductivity. In: Physical Review X. 2015, 5(4), 041021. eISSN 2160-3308. Available under: doi: 10.1103/PhysRevX.5.041021deu
kops.citation.iso690DI BERNARDO, Angelo, Zaher SALMAN, Xiaolei WANG, Mario AMADO, Mehmet EGILMEZ, Machiel G. FLOKSTRA, Andreas SUTER, Steve L. LEE, Jianhua ZHAO, Jason W. A. ROBINSON, 2015. Intrinsic Paramagnetic Meissner Effect due to s-wave Odd-Frequency Superconductivity. In: Physical Review X. 2015, 5(4), 041021. eISSN 2160-3308. Available under: doi: 10.1103/PhysRevX.5.041021eng
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kops.sourcefieldPhysical Review X. 2015, <b>5</b>(4), 041021. eISSN 2160-3308. Available under: doi: 10.1103/PhysRevX.5.041021deu
kops.sourcefield.plainPhysical Review X. 2015, 5(4), 041021. eISSN 2160-3308. Available under: doi: 10.1103/PhysRevX.5.041021deu
kops.sourcefield.plainPhysical Review X. 2015, 5(4), 041021. eISSN 2160-3308. Available under: doi: 10.1103/PhysRevX.5.041021eng
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