We present a theory for the photon energy and polarization dependence of
ARPES intensities from the CuO plane in the framework of strong correlation
models. We show that for electric field vector in the CuO plane the
radiation characteristics' of the $O$ $2p_\sigma$ and $Cu$ $3d_{x^2-y^2}$ orbitals are strongly peaked along the CuO$_2$ plane, i.e. most photoelectrons are emitted at grazing angles. This suggests that surface states play an important role in the observed ARPES spectra, consistent with recent data from Sr$_2$CuCl$_2$O$_2$. We show that a combination of surface state dispersion and Fano resonance between surface state and the continuum of LEED-states may produce a precipitous drop in the observed photoelectron current as a function of in-plane momentum, which may well mimic a Fermi-surface crossing. This effect may explain the simultaneous observation’ of a hole-like and an
electron-like Fermi surfaces in Bi2212 at different photon energies. We show
that by suitable choice of photon polarization one can on one hand focus' the radiation characteristics of the in-plane orbitals towards the detector and on the other hand make the interference between partial waves from different orbitals more constructive’.

生成讲解博客的中文版本

生成AI智能校验的中文版本