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Distinguishing s± and s++ electron pairing symmetries by neutron spin resonance in superconducting NaFe0.935Co0.045As

Chenglin Zhang, H.-F. Li, Yu Song, Yixi Su, Guotai Tan, Tucker Netherton, Caleb Redding, Scott V. Carr, Oleg Sobolev, Astrid Schneidewind, Enrico Faulhaber, L. W. Harriger, Shiliang Li, Xingye Lu, Dao-Xin Yao, Tanmoy Das, A. V. Balatsky, Th. Brückel, J. W. Lynn, and Pengcheng Dai
Phys. Rev. B 88, 064504 – Published 9 August 2013

Abstract

A determination of the superconducting (SC) electron pairing symmetry forms the basis for establishing a microscopic mechanism for superconductivity. For iron pnictide superconductors, the s±-pairing symmetry theory predicts the presence of a sharp neutron spin resonance at an energy below the sum of hole and electron SC gap energies (E2Δ) below Tc. On the other hand, the s++-pairing symmetry expects a broad spin excitation enhancement at an energy above 2Δ below Tc. Although the resonance has been observed in iron pnictide superconductors at an energy below 2Δ consistent with the s±-pairing symmetry, the mode has also been interpreted as arising from the s++-pairing symmetry with E2Δ due to its broad energy width and the large uncertainty in determining the SC gaps. Here we use inelastic neutron scattering to reveal a sharp resonance at E=7 meV in SC NaFe0.935Co0.045As (Tc=18 K). On warming towards Tc, the mode energy hardly softens while its energy width increases rapidly. By comparing with calculated spin-excitation spectra within the s± and s++-pairing symmetries, we conclude that the ground-state resonance in NaFe0.935Co0.045As is only consistent with the s± pairing, and is inconsistent with the s++-pairing symmetry.

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  • Received 17 May 2013

DOI:https://doi.org/10.1103/PhysRevB.88.064504

©2013 American Physical Society

Authors & Affiliations

Chenglin Zhang1,2, H.-F. Li3,4, Yu Song1,2, Yixi Su5, Guotai Tan6,2, Tucker Netherton2, Caleb Redding2, Scott V. Carr1,2, Oleg Sobolev7, Astrid Schneidewind5,8, Enrico Faulhaber9,8, L. W. Harriger10, Shiliang Li11, Xingye Lu11, Dao-Xin Yao12, Tanmoy Das13, A. V. Balatsky13, Th. Brückel14, J. W. Lynn10, and Pengcheng Dai1,2,11,*

  • 1Department of Physics and Astronomy, Rice University, Houston, Texas 77005, USA
  • 2Department of Physics and Astronomy, The University of Tennessee, Knoxville, Tennessee 37996-1200, USA
  • 3Jülich Centre for Neutron Science JCNS, Forschungszentrum Jülich GmbH, Outstation at Institut Laue-Langevin, Boı̂te Postale 156, F-38042 Grenoble Cedex 9, France
  • 4Institut für Kristallographie der RWTH Aachen, 52056 Aachen, Germany
  • 5Jülich Centre for Neutron Science JCNS, Forschungszentrum Jülich GmbH, Outstation at MLZ, D-85747 Garching, Germany
  • 6Department of Physics, Beijing Normal University, Beijing 100875, China
  • 7Institut für Physikalische Chemie, Georg-August-Universität Göttingen, Tammannstrasse 6, 37077 Göttingen, Germany
  • 8Forschungsneutronenquelle Heinz Maier-Leibnitz (FRM-II), TU München, D-85747 Garching, Germany
  • 9Gemeinsame Forschergruppe HZB–TU Dresden, Helmholtz-Zentrum Berlin für Materialien und Energie, D-14109 Berlin, Germany
  • 10NIST Center for Neutron Research, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA
  • 11Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 12State Key Laboratory of Optoelectronic Materials and Technology, Sun Yat-Sen University, Guangzhou 510275, China
  • 13Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico, 87545, USA
  • 14Jülich Centre for Neutron Science JCNS and Peter Grünberg Institut PGI, JARA-FIT, Forschungszentrum Jülich GmbH, 52425 Jülich, Germany

  • *pdai@rice.edu

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Vol. 88, Iss. 6 — 1 August 2013

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