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. 2013:4:2874.
doi: 10.1038/ncomms3874.

Doping dependence of spin excitations and its correlations with high-temperature superconductivity in iron pnictides

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Free PMC article

Doping dependence of spin excitations and its correlations with high-temperature superconductivity in iron pnictides

Meng Wang et al. Nat Commun. 2013.
Free PMC article

Abstract

High-temperature superconductivity in iron pnictides occurs when electrons and holes are doped into their antiferromagnetic parent compounds. Since spin excitations may be responsible for electron pairing and superconductivity, it is important to determine their electron/hole-doping evolution and connection with superconductivity. Here we use inelastic neutron scattering to show that while electron doping to the antiferromagnetic BaFe₂As₂ parent compound modifies the low-energy spin excitations and their correlation with superconductivity (<50 meV) without affecting the high-energy spin excitations (>100 meV), hole-doping suppresses the high-energy spin excitations and shifts the magnetic spectral weight to low-energies. In addition, our absolute spin susceptibility measurements for the optimally hole-doped iron pnictide reveal that the change in magnetic exchange energy below and above T(c) can account for the superconducting condensation energy. These results suggest that high-T(c) superconductivity in iron pnictides is associated with both the presence of high-energy spin excitations and a coupling between low-energy spin excitations and itinerant electrons.

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Figures

Figure 1
Figure 1. Summary of transport and neutron scattering results.
(a) The electronic phase diagram of electron and hole-doped BaFe2As2 (ref. 9). The right inset shows crystal and AF spin structures of BaFe2As2 with marked the nearest (J1a, J1b) and next nearest neighbor (J2) magnetic exchange couplings. The left insets show the evolution of low-energy spin excitations in Ba1−xKxFe2As2. (b,c) Temperature dependence of magnetic susceptibility for our KFe2As2 and Ba0.67K0.33Fe2As2. (d) Temperature dependence of the resistivity for BaFe1.7Ni0.3As2. (eg) The filled circles are spin excitation dispersions of KFe2As2 at 5 K, Ba0.67K0.33Fe2As2 at 9 K, and BaFe1.7Ni0.3As2 at 5 K, respectively. The shaded areas indicate vanishing spin excitations and the solid lines show spin wave dispersions of BaFe2As2 (ref. 13). (h) Energy dependence of χ(ω) for BaFe1.9Ni0.1As2 (dashed line), BaFe1.7Ni0.3As2 (green solid circles), Ba0.67K0.33Fe2As2 below (solid red circles and solid red line) and above (open purple circles and solid lines) Tc. The inset shows Energy dependence of χ(ω) for KFe2As2. The vertical error bars indicate the statistical errors of one standard deviation. The horizontal error bars in (h) indicate the energy integration range.
Figure 2
Figure 2. Schematics of Fermi surface evolution as a function of Ni-doping for BaFe2−xNixAs2 and for Ba0.67K0.33Fe2As2.
(ac) Evolution of Fermi surfaces with Ni-dopings of xe=0,0.1,0.3. The dxz, dyz, and dxy orbitals for different Fermi surfaces are coloured as red, green and blue, respectively. (d) Fermi surfaces for Ba0.67K0.33Fe2As2.
Figure 3
Figure 3. Constant-energy slices through magnetic excitations of iron pnictides at different energies.
The colour bars represent the vanadium normalized absolute spin excitation intensity in the units of mbarn sr−1 meV−1 f.u.−1. 2D images of spin excitations at 5 K for KFe2As2 (a) E=8±3 meV obtained with Ei=20 meV. The right side incommensurate peak is obscured by background scattering. (b) 13±3 meV with Ei=35 meV, (c) 53±10 meV with Ei=80 meV. For Ba0.67K0.33Fe2As2 at T=45 K, images of spin excitations at (d) E=5±1 meV obtained with Ei=20 meV, (e) 15±1 meV with Ei=35 meV, and (f) 50±2 meV obtained with Ei=80 meV. The dashed box in (d) indicates the AF zone boundaries for a single FeAs layer and the black dashed lines mark the orientations of spin excitations at different energies. Images of spin excitations for BaFe1.7Ni0.3As2 at T=5 K and (g) E=9±3 meV obtained with Ei=80 meV, (h) 30±10 meV with Ei=450 meV, and (i) 59±10 meV with Ei=250 meV. The white crosses indicate the position of QAF.
Figure 4
Figure 4. The dispersion of spin excitations for BaFe2−xNixAs2 along the [1,K] direction.
(a,b) The dispersion cuts of BaFe2As2 with Ei=250 meV and Ei=450 meV along [1,K] direction. The data are from MAPS. (c,d) Identical dispersion cuts of BaFe1.7Ni0.3As2 (xe=0.3) at MAPS.
Figure 5
Figure 5. Constant-energy images of spin excitations of iron pnictides and its comparison with RPA/DMFT calculations.
Spin excitations of BaFe1.7Ni0.3As2 in the 2D [H,K] plane at energy transfers of (a) E=70±10 meV obtained with Ei=250 meV; (b) 112±10 meV Ei=250 meV; (c) 157±10 meV and (d) 214±10 meV with Ei=450 meV. All obtained at 5 K. A flat backgrounds have been subtracted from the images. Spin excitations of Ba0.67K0.33Fe2As2 at energy transfers of (e) E=70±10 meV obtained with Ei=170 meV; (f) 115±10 meV; (g) 155±10 meV; (h) 195±10 meV obtained with Ei=450 meV, all at 9 K. Wave vector dependent backgrounds have been subtracted from the images. RPA calculations of spin excitations for Ba0.67K0.33Fe2As2 at (i) E=70 meV and (j) E=155 meV. DMFT calculations for Ba0.67K0.33Fe2As2 at (k) E=70 meV and (l) E=155 meV.
Figure 6
Figure 6. The effect of magnetic exchange couplings J (J1a, J1b and J2) on the band top of spin excitations.
The black line is energy cut at (0.8<H<1.2, 0.8<K<1.2) r.l.u for BaFe2As2 in the Heisenberg spin wave model. The red line is for Ba0.67K0.33Fe2As2 with 10 % soften band top. The blue line is a similar estimation for KFe2As2 assuming zone boundary is around E=25 meV.
Figure 7
Figure 7. RPA and LDA+DMFT calculated local susceptibility for different iron pnictides.
RPA and LDA+DMFT calculations of χ(ω) in absolute units for KFe2As2 and Ba0.67K0.33Fe2As2 comparing with earlier results for BaFe2As2 and BaFe1.9Ni0.1As2.
Figure 8
Figure 8. Properties of the resonance across Tc=38.5 K for Ba0.67K0.33Fe2As2.
Constant-energy (E=15±1 meV) images of spin excitations at (a) T=25, (b) 38, (c) 40, and (d) 45 K obtained with Ei=35 meV. In order to make fair comparison of the scattering line shape at different temperatures, the peak intensity at each temperature is normalized to 1. The pink and green arrows in (a) mark wave vector cut directions across the resonance. The integration ranges are −0.2≤K≤0.2 along the [H,0] direction and 0.8≤H≤1.2 along the [1,K] direction. The full-width-at-half-maximum (FWHM) of spin excitations are marked as dashed lines. (e) The FWHM of the resonance along the [H,0] and [1,K] directions as a function of temperature across Tc. (f) Energy dependence of the resonance obtained by subtracting the low-temperature data from the 45 K data, and correcting for the Bose population factor. (g) The black diamonds show temperature dependence of the sum of hole and electron pocket electronic gaps obtained from Angle Resolved Photoemission experiments for Ba0.67K0.33Fe2As2 (ref. 40). The red solid circles show temperature dependence of the resonance. (h) Temperature dependence of the superconducting condensation energy from heat capacity measurements and the intensity of the resonance integrated from 14–16 meV. The error bars indicate the statistical errors of one s.d.

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