Multigap superconductivity in ThAsFeN investigated using μSR measurements

Devashibhai Adroja, Amitava Bhattacharyya, Pabitra Kumar Biswas, Michael Smidman, Adrian D. Hillier, Huican Mao, Huiqian Luo, Guang-Han Cao, Zhicheng Wang, and Cao Wang
Phys. Rev. B 96, 144502 – Published 3 October 2017

Abstract

We have investigated the superconducting ground state of the newly discovered superconductor ThFeAsN with a tetragonal layered crystal structure using resistivity, magnetization, heat capacity, and transverse-field muon-spin rotation (TFμSR) measurements. Our magnetization and heat-capacity measurements reveal an onset of bulk superconductivity with Tc30K. A nonlinear magnetic-field dependence of the specific heat coefficient γ(H) has been found in the low-temperature limit, which indicates that there is a nodal energy gap. Our analysis of the TFμSR results shows that the temperature dependence of the superfluid density is better described by a two-gap model either isotropic s+s wave or s+d wave than a single-gap isotropic s-wave model for the superconducting gap, consistent with other Fe-based superconductors. The combination of γ(H) and TFμSR results suggest that the (s+d)-wave model is the most consistent candidate for the gap structure of ThFeAsN. The observation of two gaps in ThFeAsN suggests a multiband nature of the superconductivity possibly arising from the d bands of Fe ions. Furthermore, from our TFμSR study we have estimated the magnetic penetration depth in the polycrystalline sample of λL(0)=375nm, superconducting carrier density ns=4.97×1027m3, and carrier's effective-mass m*=2.48me. We compare the results of our present paper with those reported for the Fe-pnictide families of superconductors.

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  • Received 9 June 2017
  • Revised 11 September 2017

DOI:https://doi.org/10.1103/PhysRevB.96.144502

©2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Devashibhai Adroja1,2,*, Amitava Bhattacharyya1,3,†, Pabitra Kumar Biswas1, Michael Smidman4, Adrian D. Hillier1, Huican Mao5, Huiqian Luo5, Guang-Han Cao6, Zhicheng Wang6, and Cao Wang7

  • 1ISIS Facility, Rutherford Appleton Laboratory, Chilton, Didcot Oxon OX11 0QX, United Kingdom
  • 2Highly Correlated Matter Research Group, Physics Department, University of Johannesburg, P.O. Box 524, Auckland Park 2006, South Africa
  • 3Department of Physics, Ramakrishna Mission Vivekananda University, Howrah 711202, India
  • 4Center for Correlated Matter and Department of Physics, Zhejiang University, Hangzhou 310058, China
  • 5Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 6Department of Physics, State Key Laboratory of Silicon Materials, Zhejiang University, Hangzhou 310027, China
  • 7Department of Physics, Shandong University of Technology, Zibo 255049, China

  • *devashibhai.adroja@stfc.ac.uk
  • amitava.bhattacharyya@rkmvu.ac.in

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Vol. 96, Iss. 14 — 1 October 2017

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