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Volumn 66, Issue 9, 2002, Pages 1-9

(formula presented) (formula presented) Ge, Sn) Heusler compounds: An ab initio study of their structural, electronic, and magnetic properties at zero and elevated pressure

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EID: 15844374717     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.66.094421     Document Type: Article
Times cited : (17)

References (49)
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    • G. Prinz, Science 282, 1660 (1998);
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  • 23
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    • edited by G. T. Rado and H. Shul (Academic, New York
    • A. J. Freeman and R. E. Watson, in Magnetism, edited by G. T. Rado and H. Shul (Academic, New York, 1965), Vol. IIA;
    • (1965) Magnetism , vol.2 A
    • Freeman, A.J.1    Watson, R.E.2
  • 37
    • 85038907780 scopus 로고    scopus 로고
    • Although we included spin-orbit coupling in the calculations (see below), we do not show its effect on the band structure for the sake of simplicity in the presentation
    • Although we included spin-orbit coupling in the calculations (see below), we do not show its effect on the band structure for the sake of simplicity in the presentation.
  • 38
    • 85038960482 scopus 로고    scopus 로고
    • The accuracy in the position of (formula presented) with respect to the minority VBM has been checked by increasing the number of (formula presented) points and the (formula presented) value, in order to achieve a higher level of convergence. We found that the relative alignment is stable to within 0.02 eV
    • The accuracy in the position of (formula presented) with respect to the minority VBM has been checked by increasing the number of (formula presented) points and the (formula presented) value, in order to achieve a higher level of convergence. We found that the relative alignment is stable to within 0.02 eV.
  • 39
    • 85038965598 scopus 로고    scopus 로고
    • Our results concerning (formula presented) and the Fermi level position with respect to the minority VBM are consistent (within 0.3 eV at most) with previous LSDA calculations (Ref. 14) with the linearized muffin-tin orbital in the atomic sphere approximation (LMTO-ASA) method (at their calculated equilibrium lattice constants). The disagreement is certainly due to the different computational methods used and specifically to their use of the ASA, which is not very accurate in the case of appreciable asphericities in the charge density (as in these Heusler compounds)
    • Our results concerning (formula presented) and the Fermi level position with respect to the minority VBM are consistent (within 0.3 eV at most) with previous LSDA calculations (Ref. 14) with the linearized muffin-tin orbital in the atomic sphere approximation (LMTO-ASA) method (at their calculated equilibrium lattice constants). The disagreement is certainly due to the different computational methods used and specifically to their use of the ASA, which is not very accurate in the case of appreciable asphericities in the charge density (as in these Heusler compounds).
  • 40
    • 0035844611 scopus 로고    scopus 로고
    • It was recently argued [see
    • It was recently argued [see K. Capelle and G. Vignale, Phys. Rev. Lett. 86, 5546 (2001)] that spin density functional potentials are not unique functionals of the spin densities, so that our values could miss the contribution due to the discontinuity of the exchange-correlation potential, and so show a problem similar to the underestimation of the band-gap in semiconductors occurring in the original (i.e., not spin-resolved) DFT.
    • (2001) Phys. Rev. Lett. , vol.86 , pp. 5546
    • Capelle, K.1    Vignale, G.2
  • 44
    • 0000524261 scopus 로고    scopus 로고
    • It has been pointed out [see
    • It has been pointed out [see, M. Battocletti, H. Ebert, and H. Akai, Phys. Rev. B 53, 9776 (1996)] that care has to be taken when dealing with the calculation of hyperfine fields within GGA; in fact, due to a divergence inherent in the general expression of the exchange potential in the GGA as the radius approaches zero, the s gradient density in the nuclear region could take values well beyond the range for which the GGA parametrization has been optimized. It was therefore recommended to use a “finite nucleus model” within GGA.
    • (1996) Phys. Rev. B , vol.53 , pp. 9776
    • Battocletti, M.1    Ebert, H.2    Akai, H.3
  • 45
    • 0000703726 scopus 로고    scopus 로고
    • Phys. Rev. BIn our calculations and in most recent simulations [see, for example, Ref. 8 andP. Ravindran, A. Delin, P. James, B. Johansson, J.M. Willis, R. Ahuja, and O. Eriksson, 59, 15 680 (1998)] however, a “point nucleus model” was used, since the results for the hyperfine fields are in reasonable agreement with experiment.
    • (1998) Phys. Rev. B , vol.59 , pp. 15680
    • Ravindran, P.1    Delin, A.2    James, P.3    Johansson, B.4    Willis, J.M.5    Ahuja, R.6    Eriksson, O.7


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.