Abstract

We report results of self-consistent, relativistic linear-muffin-tin-orbital calculations of the band structure of CsI under compression in the observed crystal structures. We show that the relativistic effects as well as the effects of the high-pressure structural phase transition---which have so far not been theoretically examined---reduce the metallization pressure significantly. We find that metallization occurs by the closure of the direct band gap at the \ensuremath{\Gamma} point. As the crystal is compressed the band gap closes faster in the tetragonal and orthorhombic phases than in the simple-cubic phase. Our calculated metallization volume, ${V}_{M}$/${V}_{0}$=0.50, is in good agreement with recent experimental estimates.

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