Rotational spectrum and structure of Si3 -: art. no. 213003

被引:45
|
作者
McCarthy, MC
Thaddeus, P
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] Harvard Univ, Div Engn & Appl Sci, Cambridge, MA 02138 USA
关键词
D O I
10.1103/PhysRevLett.90.213003
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The rotational spectrum of a pure silicon cluster, the Si-3 trimer, has been observed for the first time. From the rotational constants of the normal and the Si-29 and Si-30 isotopic species, a precise geometrical structure has been derived: the trimer is an isosceles triangle with a bond to the apex Si of length 2.177(1) Angstrom and an apex angle of 78.10(3)degrees. The substantial inertial defect and fairly large centrifugal distortion suggest that the molecule possesses a shallow bending potential. Si-3 is a good candidate for astronomical detection because radio lines of comparably massive silicon molecules (e.g., SiC2, SiC4, and SiS) are readily observed in at least one astronomical source. The rotational spectra of Si-6, Si-9, and even larger polar silicon clusters may be detectable with the present technique, as well as similar germanium clusters.
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页数:4
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