Search NASA⌕ Search

NASA NTRS · 19780038890

Formation of metallic LiH

Abstract

It is shown that a metallic form of LiH may be produced at the relatively low transition pressure of 1.1 mbar. LiH may thus be applied to studies of insulator-metal transition at high pressure. Experimental data is used to calculate LiH transition parameters: first, Herzfeld's criterion (1927) is used to determine the volume at which metallic behavior begins, and second, pressure-volume measurements for estimating the pressure at which this volume is achieved are extrapolated. For comparison, the same volume-pressure calculation is performed for H2, and it is found that the metallization of LiH should occur more easily than that of H2.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Vaisnys, J. R., Zmuidzinas, J. S.. 1978-02-01. Formation of metallic LiH. https://ntrs.nasa.gov/citations/19780038890

Cite the original work for its findings. Save a collection to share your selection of sources.