Boron heat of formation revisited:: Relativistic effects on the BF3 atomization energy

被引:31
作者
Bauschlicher, CW
Martin, JML
Taylor, PR
机构
[1] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[2] Weizmann Inst Sci, Dept Organ Chem, IL-76100 Rehovot, Israel
[3] Univ Calif San Diego, San Diego Supercomp Ctr, La Jolla, CA 92093 USA
[4] Univ Calif San Diego, Dept Chem & Biochem MC0505, La Jolla, CA 92093 USA
关键词
D O I
10.1021/jp991713a
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
The one-electron Douglas-Kroll approach, and perturbation theory including only the mass-velocity and Darwin terms, are used to compute the scalar relativistic contribution to the atomization energies of BS. Both approaches predict an approximately 0.7 kcal/mol reduction in the atomization energy. In combination with improved one-particle extrapolation techniques, this leads to a revised estimate for the heat of formation of gaseous boron, Delta H(f,0)degrees[B(g)] = 135.1 kcal/mol and Delta H(f,298)degrees[B(g)] = 136.3 kcal/mol, with error bars +/-0.75 kcal/mol or less.
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页码:7715 / 7718
页数:4
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