2015
DOI: 10.1016/j.optmat.2015.06.009
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Structural, surface morphology and optical properties of NiSnO3 thin films prepared using spray technique

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Cited by 18 publications
(4 citation statements)
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“…9(a) shows the bandgaps of ANiO 3 (O- Pnma ) (A = Eu, Gd, Tb, Dy, Yb, La, Tm, Nd, Sm), EuBO 3 (O- Pbnm ) (B = Zr, Hf), EuTiO 3 (C- Pm 3̄ m ), DNbO 3 (O- Pnma ) (D = Ag, Ba, Ca, Sr, Eu, K, Na), SrTM 1 O 3 (C- Pm 3̄ m ) (TM 1 = Hf, Zr, Ti), KTaO 3 (C- Pm 3̄ m ), LaTM 2 O 3 (O- Pnma ) (TM 2 = Al, Sc, Fe, Cr, Ti, Ga, Co), SrTcO 3 (O- Pnma ), NaOsO 3 (O- Pbca ), MSnO 3 (R- R 3 c ) (M = Hg, Mg, Zn, Fe, Mn), NiSnO 3 (C- Pm 3̄ m ), SrNiO 3 (C- Pm 3̄ m ), BaSnO 3 (C- Pm 3̄ m ), CaSnO 3 (O- Pnma ), CoSnO 3 (O- Pnma ), TiSnO 3 (T- I 4/ mcm ), MnTiO 3 (R- R 3 c ), PbTiO 3 (T- I 4/ mcm ), CaZrO 3 (O- Pnma ), and BaFeO 3 (C- Pm 3̄ m ). As can be seen, there is good agreement in the bandgaps between our calculations and the experimental data and other reported HSE06 and G 0 W 0 data, 31–52 which demonstrates the accuracy of our method.…”
Section: Methodssupporting
confidence: 85%
“…9(a) shows the bandgaps of ANiO 3 (O- Pnma ) (A = Eu, Gd, Tb, Dy, Yb, La, Tm, Nd, Sm), EuBO 3 (O- Pbnm ) (B = Zr, Hf), EuTiO 3 (C- Pm 3̄ m ), DNbO 3 (O- Pnma ) (D = Ag, Ba, Ca, Sr, Eu, K, Na), SrTM 1 O 3 (C- Pm 3̄ m ) (TM 1 = Hf, Zr, Ti), KTaO 3 (C- Pm 3̄ m ), LaTM 2 O 3 (O- Pnma ) (TM 2 = Al, Sc, Fe, Cr, Ti, Ga, Co), SrTcO 3 (O- Pnma ), NaOsO 3 (O- Pbca ), MSnO 3 (R- R 3 c ) (M = Hg, Mg, Zn, Fe, Mn), NiSnO 3 (C- Pm 3̄ m ), SrNiO 3 (C- Pm 3̄ m ), BaSnO 3 (C- Pm 3̄ m ), CaSnO 3 (O- Pnma ), CoSnO 3 (O- Pnma ), TiSnO 3 (T- I 4/ mcm ), MnTiO 3 (R- R 3 c ), PbTiO 3 (T- I 4/ mcm ), CaZrO 3 (O- Pnma ), and BaFeO 3 (C- Pm 3̄ m ). As can be seen, there is good agreement in the bandgaps between our calculations and the experimental data and other reported HSE06 and G 0 W 0 data, 31–52 which demonstrates the accuracy of our method.…”
Section: Methodssupporting
confidence: 85%
“…[ 39 ] The band at 589 cm −1 may be due to the presence of chloride (Cl – ) ions left behind during the synthesis process (due to SnCl 4 precursor). [ 40 ] IR bands corresponding to CO vibrations appear at 1125, 1414, and 1132 cm −1 , respectively, and two small peaks observed at 2317 and 2380 cm −1 represent CO 2 absorbed from the atmosphere. [ 41 ] CH stretching and bending vibrations have been noted from 2983 and 3067 cm –1 bands.…”
Section: Resultsmentioning
confidence: 99%
“…and other perovskite materials [20][21][22][23][24] were consequently proposed using DFT simulations as well as experimental efforts. Astonishing magnetoelectric coupling in transition metal titanates ATiO3 (A = Mn, Fe, Ni) make them the most capable members of MF family.…”
Section: Introductionmentioning
confidence: 99%