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Thesis High-Resolution Photoemission Study of Kondo Insulators ...

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38 Chapter 3. <strong>Photoemission</strong> <strong>Study</strong> <strong>of</strong> YbB12 with Variable Photon Energies<br />

Intensity (arb. units)<br />

LDA<br />

B p DOS<br />

YbB 12<br />

hν = 21.2 eV<br />

Au<br />

0.10 0.00 -0.10<br />

Binding Energy (eV)<br />

Figure 3.5: He I spectrum <strong>of</strong> YbB12 in the vicinity <strong>of</strong> EF . The solid curves is the<br />

spectrum <strong>of</strong> Au evaporated onto the sample. The B p partial DOS given by the LDA<br />

band-structure calculation broadened by the instrumental resolution is also shown.<br />

study <strong>of</strong> the Anderson lattice as a model for a <strong>Kondo</strong> insulator [3.22].<br />

Therefore, we expect that the Yb 4f spectral lineshape is likewise subject to the<br />

strong renormalization <strong>of</strong> energy bands. Instead <strong>of</strong> first-principles approaches such<br />

as second-order perturbation calculations [3.23], we have employed a phenomenological<br />

approach and fitted the observed spectral lineshape using a model self-energy correction.<br />

As shown in Fig. 3.6 by the dashed curve, the Yb f partial DOS has structures from<br />

∼150 to ∼400 meV while the observed peak position is ∼40 meV below EF . This peak<br />

exhibits a steep rise from EF as in the case <strong>of</strong> the B 2p-derived He I spectrum, and<br />

a slow tailing <strong>of</strong>f on the higher binding energy side, resulting in a highly asymmetric<br />

lineshape. This indicates that the band narrowing is energy dependent and is stronger<br />

near EF . The model self-energy which we have employed to calculate the 4f spectral<br />

function ρf(ω) is <strong>of</strong> the same type as that previously used for FeSi [3.13]:<br />

where<br />

Σh(ω) =<br />

Σ(ω) =Σh(ω)+Σl(ω)+Σl ′(ω), (3.1)<br />

gh(ω − δ)<br />

,<br />

(ω − δ + iγh) 2

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