In-Plane Magnetic Penetration Depth in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>Sr</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>RuO</mml:mi></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:mrow></mml:math>: Muon-Spin Rotation and Relaxation Study
R. Khasanov, Aline Ramires, Vadim Grinenko, Ilya Shipulin, Naoki Kikugawa, D. A. Sokolov, Jonas A. Krieger, T. J. Hicken, Y. Maeno, H. Luetkens, Zurab Guguchia
Abstract
We report on measurements of the in-plane magnetic penetration depth (${\ensuremath{\lambda}}_{\mathrm{ab}}$) in single crystals of ${\mathrm{Sr}}_{2}{\mathrm{RuO}}_{4}$ down to $\ensuremath{\simeq}0.015\text{ }\text{ }\mathrm{K}$ by means of muon-spin rotation-relaxation. The linear temperature dependence of ${\ensuremath{\lambda}}_{\mathrm{ab}}^{\ensuremath{-}2}$ for $T\ensuremath{\lesssim}0.7\text{ }\text{ }\mathrm{K}$ suggests the presence of nodes in the superconducting gap. This statement is further substantiated by observation of the Volovik effect, i.e., the reduction of ${\ensuremath{\lambda}}_{ab}^{\ensuremath{-}2}$ as a function of the applied magnetic field. The experimental zero-field and zero-temperature value of ${\ensuremath{\lambda}}_{\mathrm{ab}}=124(3)\text{ }\text{ }\mathrm{nm}$ agrees with ${\ensuremath{\lambda}}_{\mathrm{ab}}\ensuremath{\simeq}130\text{ }\text{ }\mathrm{nm}$, calculated based on results of electronic structure measurements reported in A. Tamai et al. [High-resolution photoemission on ${\mathrm{Sr}}_{2}{\mathrm{RuO}}_{4}$ reveals correlation-enhanced effective spin-orbit coupling and dominantly local self-energies, Phys. Rev. X 9, 021048 (2019)]. Our analysis reveals that a simple nodal superconducting energy gap, described by the lowest possible harmonic of a gap function, does not capture the dependence of ${\ensuremath{\lambda}}_{\mathrm{ab}}^{\ensuremath{-}2}$ on $T$, so the higher angular harmonics of the energy gap function need to be introduced.