<div dir="ltr"><div dir="ltr"><div><div> System under study is SrTiO3 doped with Hf-181 tdpac probe for TDPAC spectroscopy by thermal equillibriation method (1250 C for >12 hours). the doping is substitutional as Hf(IV) and Ti(IV) has nearby ionic radius and same oxidation state. Bulk STO shows no efg, no assymetry parameter as STO is cubic lattice and Hf/Ti present at octahedral symmetry but in another synthetic procedure where synthesis parameters can be controlled shows STO with probe showing very pure HFI. From literature, STO is known to have oxygen vacancies depending on synthesis route. <br></div> Calculation: STO structure is optimized and minimized. Created supercell 3x2x2 as it allows me to use 5 processor with 8 gb ram (with 3x3x3, calc. restricted to only 2 processors due to RAM limitation. So long scf run time. i will try now) . Problem of breaking symmetry did not strike me at the time of calculation. Replaced one Ti by Hf. Then supercell calculation was done for oxygen vacancies in first cordination and fourth nearest neighbour cordination. The efg matched for the later case (oxygen vacancy at fourth nearest neighbour) but not assymetry parameter. Minimization of forces on supercell was not done ( i thought basic lattice unit was already optimized). <br></div><div> What i understood from previous replies of this thread is 1.Must do 3x3x3 supercell calculation, 2. Electron electron correlation can also be included for improvement of calculation, 3. Need to check calculation with reduced RMT of Sr and Ti. <br> <br></div><div>To what % agreemnet wrt experimental efg data, efg values from theoretical calculation can be accepted. <br>Thanks Dr. Cottenier for the suggestion, i had already subscribed to HF course A (ID: iak). I will subscribe to Course B after finishing course A. <br><br></div><div>Thanks,<br></div><div>A. Kumar<br></div><br></div></div><br><div class="gmail_quote"><div dir="ltr">On Wed, Dec 19, 2018 at 12:08 AM Ashwani Kumar <<a href="mailto:ashwani.ism@gmail.com">ashwani.ism@gmail.com</a>> wrote:<br></div><blockquote class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><div dir="ltr"><div>hi,</div><div> thanks for reply. the assymetry parameter, (Vxx-Vyy)/Vzz, is zero (wien2k calculation) whereas i got 0.52 from TDPAC (Time dependent perturbed angular correlation) spectroscopy for a SrTiO3 (STO) defect structure. EFG component is -1.63 x10^21 V/m2 (wien2k, lapw2 -efg) and i obtained 1.69 x 10^21 V/m2 (calculated from TDPAC results). STO has cubic lattice so no efg and no assymetry parameter (for both wien2k and TDPAC) but defect STO structure showed very pure hyperfine interactions with assymetry parameter : 0.52. So i am not having confidence over my wien2k calculation because :</div><div>1. i am getting assymetry parameter =0</div><div>2. Negative EFG which i understood from previous answers that negative sign indicates the rate of decrease of z-component of EF wrt to distance. <br></div><div><br></div><div>Am i missing something?, <br></div><div>Calculation parameters are :Supercell (3x2x2) STO with doped Hf atom, PBE, KGEN:200, rkmax: 7.0, <br></div><div><br></div><div>thanks,</div><div>A. Kumar<br></div></div><br><div class="gmail_quote"><div dir="ltr">On Fri, Dec 14, 2018 at 11:02 PM Ashwani Kumar <<a href="mailto:ashwani.ism@gmail.com" target="_blank">ashwani.ism@gmail.com</a>> wrote:<br></div><blockquote class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><div dir="ltr"><div>Hi, <br></div><div> i have calculated EFG the defect structure of crystalline system from experimental data from PAC spectroscopy. Then using WIEN2K (crystal structure--> supercell--> defect introduced), EFG is calculated. <br></div><div>Exper. Calculated : 1.69 x 10^21 V/m2 whereas wien2k calculation: -1.66 x 10^21 V/m2 (crude value still have to do lapw2 -efg) on probe atom. Wien2k calculation shows negative value. is there any significance of the negative sign.</div><div><br></div><div>thanks,</div><div>A. Kumar<br></div></div>
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