[doi:10.1038/nphys1763]
a, YBCO6.34 nodal dispersion and MDCs at EF (±15 meV integration, shaded region), for light polarization parallel to Γ–S. b, YBCO7 MDCs for polarization along Γ–Y (note the strong polarization dependence). c, Evolution of kF,NB (down triangles) and kF,NAB (up triangles); below p≃0.15 the B–AB splitting vanishes and only one single kF,N is detected (diamonds). d, ZN as determined from the B–AB splitting with and the rescaled low-energy spectral-weight ratio . Also shown are spline guides-to-the-eye and the 2p/(p+1) relation (dashed red line). For the splitting-derived data, error bars are determined from the B–AB MDC fits when splitting is detected, and from the experimental resolutions otherwise; for the spectral weight ratio (SWR), they are calculated from the spread in SWR values for integration windows smaller than
No comments:
Post a Comment