Ab initio calculations of the effect of hydrostatic pressure on the Fermi surface of transition metals, vanadium (V), niobium (Nb), and tantalum (Ta) using the linear mufin‐tin orbital method in the atomic‐sphere approximation are presented. The self‐consistent calculations are performed with the use of various exchange‐correlation potentials. The results are compared with available experimental data and theoretical Calculations.
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Solanki et al. (1994) studied this question.
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