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Dear Pascal
<div class="">It is expected that in the “disentangled” part of the spectrum for there to be some differences between the wannier-interpolated and original DFT bands. In your case, it is strange that there is a difference even in part of the bandstructure where
you have applied a frozen energy window, which indicates that perhaps the disentanglement or wannierisation is not entirely satisfactory. It would be worth checking the output file in detail to see whether the calculation has actually converged and produced
localised Wannier functions.</div>
<div class="">Best wishes,</div>
<div class="">Arash</div>
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<div class="">—</div>
<div class="">Professor Arash Mostofi — <a href="http://www.mostofigroup.org" class="">
www.mostofigroup.org</a></div>
<div class="">Director, Thomas Young Centre @Imperial</div>
<div class="">Imperial College London</div>
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<div class="">On 24 Apr 2020, at 13:48, Pascal Salzbrenner <<a href="mailto:pts28@cam.ac.uk" class="">pts28@cam.ac.uk</a>> wrote:</div>
<br class="Apple-interchange-newline">
<div class="">
<div class="">Dear all,<br class="">
<br class="">
I am trying to generate a wannier90 tight-binding model for CdTe (using wannier90-1.2 for the initial post postprocessing step and wannier90-3.1 for the wannierisation). In general, it reproduces the behaviour of the bands well compared to my DFT (VASP) result,
but the conduction band is, in many places, somewhat lower using the wannier90 model than it is when generating the band structure directly from DFT. In particular, at the Gamma point, the band gap is underestimated by around 0.1 eV.<br class="">
I have tried using a variety of different projectors (even projector sets of different sizes, with between 16 and 24 projectors per unit cell). The combinations I have used are composed of atomic s- (with r=1 as well as r=2) and p-orbitals, as well as different
hybridisations. I have also tried adding orbitals using the "random" keyword. The attached figure was generated by projecting on the atomic sp2 and pz orbitals on both Cd and Te. At the Gamma point, the conduction band is highly s-like in character, but adding
s-orbitals to these projectors does not improve the fit around the Gamma point, and it worsens it in other regions of the BZ.<br class="">
I have tried excluding the higher unoccupied bands during the projection using the "exclude_bands" tag, and I have tuned the frozen window. In all these calculations, the disagreement at the gamma point persists. Does anyone have any idea what I am doing wrong,
or what I could try to get the two methods to agree at this point? The "<a href="http://wannier90.win" class="">wannier90.win</a>“ file, as well as the output band structure for the projection of the sp2 and pz orbitals (which are representative of the calculations
I tried) can be found here: <a href="https://drive.google.com/open?id=15uGvHXHVFY_iq-LDOtTeK5JHkrun6jJ6" class="">
https://drive.google.com/open?id=15uGvHXHVFY_iq-LDOtTeK5JHkrun6jJ6</a>. I’d be grateful for any help.<br class="">
<br class="">
Thanks in advance!<br class="">
<br class="">
Pascal Salzbrenner<br class="">
MPhil Student<br class="">
Monserrat Group<br class="">
Theory of Condensed Matter, University of Cambridge<br class="">
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