Oxygen isotope effect on the superfluid density within the d-wave and s-wave pairing channels of YBa2Cu4O8
Abstract
We report on measurements of the oxygen isotope (16O/18O) effect (OIE) on the transition temperature T c and the zero-temperature in-plane magnetic penetration depth λ ab(0) in the stoichiometric cuprate superconductor YBa2Cu4O8 by means of muon-spin rotation/relaxation. An analysis of the temperature evolution of λ-2 ab in terms of coexisting s+d-wave order parameters reveals that the OIE on the superfluid density s(0)λ-2 ab(0) stems predominantly from the d-wave component while the contribution of the s-wave one is almost zero. The OIE on the transition temperature T c is found to be rather small: δ T c/T c= -0.32(7)%, compared to the total OIE on the superfluid density s(0): δ s(0)/ s(0)= -2.8(1.0)%. The partial OIE's on the corresponding d-wave and s-wave components of s(0) are δ s,d(0)/ s(0)= -3.0(1.2)%, and δ s,s(0)/ s(0)= 0.2(1.2)%, respectively. Our results demonstrate that polaron formation in the CuO2 planes is the origin of the observed OIE in the d-wave channel. In the much weaker s-wave channel, fermionic quasiparticles are present, which do not contribute to the OIE on s(0). Our results support the original idea of K. Alex M\"uller on the polaronic nature of the supercarries in high-temperature cuprate superconductors.
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