2001
DOI: 10.1063/1.1334615
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Relativistic effects on the optical response of InSb by time-dependent density-functional theory

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Cited by 12 publications
(18 citation statements)
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“…Note that this redshift is compatible but smaller than the error in the calculated band gaps, in line with previous findings. 17,32 Our results indicate that for ZnTe and CdTe the relative position of the s-like conduction band with respect to the p-like top valence band is too low, whereas the dispersion of the bands is well described. The spectra of HgTe reflect the strong impact of relativity on the electronic structure: in particular, the relativistic absorption spectra show the onset at ប = 0 eV, while the nonrelativistic one shows the onset at a finite frequency and is quite different from the experiments.…”
Section: Nonmetals: Ii-vi Zinc-blende-type Znte Cdte Hgtementioning
confidence: 70%
See 1 more Smart Citation
“…Note that this redshift is compatible but smaller than the error in the calculated band gaps, in line with previous findings. 17,32 Our results indicate that for ZnTe and CdTe the relative position of the s-like conduction band with respect to the p-like top valence band is too low, whereas the dispersion of the bands is well described. The spectra of HgTe reflect the strong impact of relativity on the electronic structure: in particular, the relativistic absorption spectra show the onset at ប = 0 eV, while the nonrelativistic one shows the onset at a finite frequency and is quite different from the experiments.…”
Section: Nonmetals: Ii-vi Zinc-blende-type Znte Cdte Hgtementioning
confidence: 70%
“…A similar formalism that treats scalar relativistic effects only has previously been combined with the time-dependent currentdensity functional formulation of the linear response of solids to a macroscopic electric field. [17][18][19] Although the scalar relativistic effects account for the most important relativistic contributions in the spectra, 19,20 some characteristic features were still missing due to the neglect of spin-orbit coupling. For example, in the group VB and VIB bcc transition metals the treatment of spin-orbit coupling is expected to yield a finite gap in the interband contribution to the absorption spectra, while in the scalar relativistic calculations the absorption remains finite even down to ប = 0 eV.…”
Section: Introductionmentioning
confidence: 99%
“…15,16 They followed the description of van Lenthe and co-workers 17,18 and Philipsen et al 19 by using the zeroth-order regular approximation ͑ZORA͒. Scalar-relativistic effects are then considered by using the ground-state scalar ZORA equation,…”
Section: ͑3͒mentioning
confidence: 99%
“…The density matrix at equilibrium can be written as the Fermi function of the Hamiltonian matrix as below [11]:…”
Section: Theorymentioning
confidence: 99%
“…Which H is Hamiltonian, μ is Fermi energy and I is the identity matrix of same size as H. It can be shown; the charge density is given by diagonal elements of density matrix [11]:…”
Section: Theorymentioning
confidence: 99%