Physics
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phla..153..133m&link_type=abstract
Physics Letters A, Volume 153, Issue 2-3, p. 133-135.
Physics
1
Scientific paper
Motivated by the fact that CH4 is a major constituent of the outer planets, a simple electronic model is used to predict the variation of the X-H equilibrium bond length for condensed XH4 under pressure fore heavy central atoms X. In particular, an analytical expression is obtained relating the X-H length in the condensed phase to the free space bond length.
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