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Crystal stability of heavy-rare-gas solids on the melting line

Journal Article · · Physical Review, B: Condensed Matter; (United States)
;  [1];  [2]
  1. Department of Chemistry, Korea Advanced Institute of Science Technology, Taejon (Korea, Republic of)
  2. University of California, Lawrence Livermore National Laboratory, Livermore, California 94551 (United States)

Contrary to static-energy predictions favoring a hexagonal-close-packed phase, heavy rare gases solidify into a face-centered-cubic phase over a large temperature range. Our recent perturbation theory and hard-sphere radial distribution functions are applied to give a conclusive calculation that agrees with experiment near the melting lines of heavy-rare-gas solids. The observed stability is due to thermal contributions to the Helmholtz free energy which far exceed the opposing static term. The Lennard-Jones potentials used here reproduce melting data of these solids to 1 GPa.

DOE Contract Number:
W-7405-ENG-48
OSTI ID:
6277430
Journal Information:
Physical Review, B: Condensed Matter; (United States), Journal Name: Physical Review, B: Condensed Matter; (United States) Vol. 48:5; ISSN PRBMDO; ISSN 0163-1829
Country of Publication:
United States
Language:
English