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SRC Users' Meeting - Synchrotron Radiation Center - University of ...

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Fig. 2: Comparison <strong>of</strong> the experimental initial state bulk band structure <strong>of</strong> Bi along<br />

the T direction with various model calculations.<br />

Furthermore, scattering events can play a significant role in the interpretation <strong>of</strong><br />

photoemission spectra. They lead to various phenomena that can be observed in the<br />

photoemission spectra. It has been shown for bismuth that scattering events induce loss features<br />

in the 5d-core level spectra [2], which can be associated with interband transitions inside the<br />

crystal. In the normal emission spectra we present here secondary cone emission features, which<br />

result from transitions involving reciprocal lattice vectors not parallel to the normal emission<br />

direction, can be observed. For these features to be observed in the normal emission spectra the<br />

photoelectrons need to be scattered back into the normal emission direction. We show that for a<br />

complete data analysis secondary cone emission phenomena have to be included. The presence<br />

<strong>of</strong> secondary cone emission features in the spectra clearly shows the significance <strong>of</strong> scattering<br />

phenomena in photoemission spectra <strong>of</strong> bismuth.<br />

Figure 2 shows the extracted initial state bands (black lines) in comparison with a third<br />

neighbor tight-binding calculation [3], as well as two first principle calculations [4, 5] (dotted<br />

lines). The agreement in the dispersion is mostly qualitatively. The tight binding calculation has<br />

difficulties reproducing the dispersion <strong>of</strong> the middle band, whereas the calculation by Gonze [4]<br />

shows the best agreement with the experimental initial state bands.<br />

[1] G. Jezequel, J. Thomas, and I. Pollini, Phys. Rev. B 56, 6620 (1997)<br />

[2] C. R. Ast and H. Höchst, Phys. Rev. Lett. in press (2003).<br />

[3] Y. Liu and R. E. Allen, Phys. Rev. B 52, 1566 (1995)<br />

[4] X. Gonze, J.-P. Michenaud, and J.-P. Vigneron, Phys. Rev. B 41, 11827 (1990)<br />

[5] A. B. Shick, J. B. Ketterson, D. L. Novikov, and A. J. Freeman, Phys. Rev. B 60, 15484<br />

(1999)

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