TY - JOUR
T1 - Band calculation for Ce-compounds on the basis of dynamical mean field theory
AU - Sakai, Osamu
AU - Shimizu, Yukihiro
AU - Kaneta, Yasunori
PY - 2005/9
Y1 - 2005/9
N2 - The band calculation scheme for f electron compounds is developed on the basis of the dynamical mean field theory (DMFT) and the LMTO method. The auxiliary impurity problem is solved by a method named as NCAf2v', which includes the correct exchange process of the f1 → f 2 virtual excitation as the vertex correction to the non-crossing approximation (NCA) for the f1 → f0 fluctuation. This method leads to the correct magnitude of the Kondo temperature, TK, and makes it possible to carry out quantitative DMFT calculation including the crystalline field (CF) and the spin-orbit (SO) splitting of the self-energy. The magnetic excitation spectra are also calculated to estimate TK. It is applied to Ce metal and CeSb at T = 300K as the first step. In Ce metal, the hybridization intensity (HI) just below the Fermi energy is reduced in the DMFT band. The photo-emission spectra (PES) have a conspicuous SO side peak, similar to that of experiments. TK is estimated to be about 70K in γ-Ce, while to be about 1700K in α-Ce. In CeSb, the double-peak-like structure of PES is reproduced. The HI is enhanced just at the Fermi energy in the DMFT band of CeSb. Therefore, TK ∼ 60 K, which is comparable to but slightly larger than the experimental value, is obtained.
AB - The band calculation scheme for f electron compounds is developed on the basis of the dynamical mean field theory (DMFT) and the LMTO method. The auxiliary impurity problem is solved by a method named as NCAf2v', which includes the correct exchange process of the f1 → f 2 virtual excitation as the vertex correction to the non-crossing approximation (NCA) for the f1 → f0 fluctuation. This method leads to the correct magnitude of the Kondo temperature, TK, and makes it possible to carry out quantitative DMFT calculation including the crystalline field (CF) and the spin-orbit (SO) splitting of the self-energy. The magnetic excitation spectra are also calculated to estimate TK. It is applied to Ce metal and CeSb at T = 300K as the first step. In Ce metal, the hybridization intensity (HI) just below the Fermi energy is reduced in the DMFT band. The photo-emission spectra (PES) have a conspicuous SO side peak, similar to that of experiments. TK is estimated to be about 70K in γ-Ce, while to be about 1700K in α-Ce. In CeSb, the double-peak-like structure of PES is reproduced. The HI is enhanced just at the Fermi energy in the DMFT band of CeSb. Therefore, TK ∼ 60 K, which is comparable to but slightly larger than the experimental value, is obtained.
KW - Band theory
KW - Ce metal
KW - Ce-pnictides
KW - Dynamical mean field theory
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U2 - 10.1143/JPSJ.74.2517
DO - 10.1143/JPSJ.74.2517
M3 - Article
AN - SCOPUS:25144473969
SN - 0031-9015
VL - 74
SP - 2517
EP - 2529
JO - Journal of the Physical Society of Japan
JF - Journal of the Physical Society of Japan
IS - 9
ER -