BANDS OF H-3(+) UP TO 4-NU-2 - ROVIBRATIONAL TRANSITIONS FROM 1ST PRINCIPLES CALCULATIONS

被引：55

作者：

DINELLI, BM ^{[1
]}

MILLER, S ^{[1
]}

TENNYSON, J ^{[1
]}

机构：

[1] IST SPETTROSCOPIA MOLEC, I-40126 BOLOGNA, ITALY

来源：

JOURNAL OF MOLECULAR SPECTROSCOPY | 1992年 / 153卷 / 1-2期

关键词：

D O I：

10.1016/0022-2852(92)90506-J

中图分类号：

O64 [物理化学（理论化学）、化学物理学]; O56 [分子物理学、原子物理学];

学科分类号：

070203 ; 070304 ; 081704 ; 1406 ;

摘要：

Band origins and Einstein A coefficients are presented for transitions linking all the vibrational levels of H3+ up to 4ν2(l = 4). The importance of these data for astrophysical modeling is discussed. For H3+, rovibrational wavefunctions and energy levels are obtained for J up to 16. These are used to synthesize sample rovibrational spectra with particular emphasis on the ν1 + 2ν2(l = 2) ← 0 and 4ν2(l = 2) ← 0 bands, which would appear to be good candidates for laboratory observation. © 1992.

引用

页码：718 / 725

页数：8