11.07.2015 Views

Calculating the effective U in APW methods. NiO - WIEN 2k

Calculating the effective U in APW methods. NiO - WIEN 2k

Calculating the effective U in APW methods. NiO - WIEN 2k

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

<strong>Calculat<strong>in</strong>g</strong> <strong>the</strong> <strong>effective</strong> U <strong>in</strong> <strong>APW</strong> <strong>methods</strong>. <strong>NiO</strong>Georg K. H. Madsen and Pavel Novák(Dated: June 19, 2007)The follow<strong>in</strong>g is an example of how to calculate <strong>the</strong> <strong>effective</strong> U follow<strong>in</strong>g <strong>the</strong> prescription of ref.[1]. The follow<strong>in</strong>gsteps are described• generat<strong>in</strong>g a supercell• modify<strong>in</strong>g <strong>the</strong> <strong>in</strong>put files• Perform <strong>the</strong> two SCF calculations• calculat<strong>in</strong>g <strong>the</strong> U from <strong>the</strong> values <strong>in</strong> <strong>the</strong> scf file.I. GENERATING A SUPERCELLThis can be done <strong>in</strong> several ways. For <strong>the</strong> present case we chose a 2 × 2 × 2 F-centered cell. The steps are:1. set-up <strong>the</strong> standard F-centered, a=7.927 a.u. <strong>NiO</strong>.struct file.2. For this example choose R MT to 2.3 a.u. and 1.65 a.u. for Ni and O respectively. The result shouldn’t be toosensitive to <strong>the</strong>se choices.3. Run supercell and choose a 2 × 2 × 2 F-centered cell.4. Change <strong>the</strong> name of <strong>the</strong> first Ni to Ni1 (to break symmetry). This is your impurity.5. Run x sgroup and copy <strong>NiO</strong>.struct sgroup to <strong>NiO</strong>.struct. Your struct file should now have <strong>the</strong> header:<strong>NiO</strong>F LATTICE,NONEQUIV.ATOMS: 5 225 Fm-3mMODE OF CALC=RELA unit=15.854002 15.854002 15.854002 90.000000 90.000000 90.000000ATOM 1: X=0.00000000 Y=0.00000000 Z=0.00000000MULT= 1 ISPLIT= 2Ni1 NPT= 781 R0=0.00050000 RMT= 2.3000 Z: 28.0II.RUN NORMAL SCFRun <strong>the</strong> <strong>in</strong>it as usual. Use just one k-po<strong>in</strong>t. For <strong>the</strong> present choose an Rkmax of 5. The orig<strong>in</strong>al Anisimov andGunnarsson[2] force everyth<strong>in</strong>g but <strong>the</strong> impurity d states to be non-sp<strong>in</strong>polarized. This is not really necessary andwould make our calculations more complicated. We <strong>the</strong>refore run <strong>the</strong> calculation sp<strong>in</strong>polarized, but start with only<strong>the</strong> impurity <strong>in</strong> a sp<strong>in</strong>polarized states. This also improves convergence. Modify <strong>in</strong>st so that it looks like:NiAr 3 53, 2,2.0 P3, 2,2.0 P3,-3,3.0 P3,-3,1.0 P4,-1,1.0 N4,-1,1.0 NNiAr 3 53, 2,2.0 N3, 2,2.0 N


23,-3,2.0 N3,-3,2.0 N4,-1,1.0 N4,-1,1.0 NNiAr 3 53, 2,2.0 N3, 2,2.0 N3,-3,2.0 N3,-3,2.0 N4,-1,1.0 N4,-1,1.0 NOHe 3 52,-1,1.0 N2,-1,1.0 N2, 1,1.0 N2, 1,1.0 N2,-2,1.0 N2,-2,1.0 NOHe 3 52,-1,1.0 N2,-1,1.0 N2, 1,1.0 N2, 1,1.0 N2,-2,1.0 N2,-2,1.0 N********now runx lstartx dstartx dstart -upx dstart -dnrunspsave <strong>NiO</strong>_origThis is actually only to get a good start<strong>in</strong>g density. The results are not needed directly.III.MODIFYING THE INPUT FILESYou now need to change <strong>in</strong>1, <strong>in</strong>2 and <strong>in</strong>c to put a constra<strong>in</strong>ed number of d-electrons <strong>in</strong> <strong>the</strong> core.A. Add<strong>in</strong>g d to <strong>the</strong> core.Usually Ni 2+ has 8 d electrons. You now want to perform two calculations. One with 4.5 ↑, 4 ↓ and one with 4.5↑, 3 ↓ constra<strong>in</strong>ed d-electrons.[1] You thus make 4 .<strong>in</strong>c files and here <strong>the</strong> headers are givenThe 4.5 ↑, 4 ↓ calculation. First atom<strong>NiO</strong>.<strong>in</strong>cup_+.50: <strong>NiO</strong>.<strong>in</strong>cdn_+.507 1.00 7 1.001,-1,2 1,-1,22,-1,2 2,-1,22, 1,2 2, 1,2

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!