High resolution spectroscopic data for H-3(+), H2D+, D2H+, and D-3(+) is used to determine effective, mass-dependent potential energy surfaces for each isotopomers. These surfaces are expressed as a sum of the mass-independent Born-Oppenheimer (BO) potential and a mass dependent adiabatic correction. For H-3(+) and D-3(+) the adiabatic correction is a single surface of the same symmetry and functional form as the BO surface. For H2D+ and D2H+ a second, lower symmetry surface is required. Fits to all three surfaces were started from recent, high quality ab initio calculations. The standard deviations for fits using all the available data with J less than or equal to 9 are 0.015 cm(-1) for H-3(+), 0.010 (-1) for H2D+ and D2H+ combined, and 0.015 cm(-1) for D-3(+). These values are close to the intrinsic experimental error of much of the data and improve on the corresponding ab initio surfaces by at least an order of magnitude. The fits are very compact: nearly 1600 data are fitted by adjusting 36 constants and freezing 51 at their ab initio values. (C) 1995 American Institute of Physics.

Spectroscopically determined Born-Oppenheimer and adiabatic surfaces for H-3(+), H2D+, D2H+, and D-3(+)

1995

Abstract

High resolution spectroscopic data for H-3(+), H2D+, D2H+, and D-3(+) is used to determine effective, mass-dependent potential energy surfaces for each isotopomers. These surfaces are expressed as a sum of the mass-independent Born-Oppenheimer (BO) potential and a mass dependent adiabatic correction. For H-3(+) and D-3(+) the adiabatic correction is a single surface of the same symmetry and functional form as the BO surface. For H2D+ and D2H+ a second, lower symmetry surface is required. Fits to all three surfaces were started from recent, high quality ab initio calculations. The standard deviations for fits using all the available data with J less than or equal to 9 are 0.015 cm(-1) for H-3(+), 0.010 (-1) for H2D+ and D2H+ combined, and 0.015 cm(-1) for D-3(+). These values are close to the intrinsic experimental error of much of the data and improve on the corresponding ab initio surfaces by at least an order of magnitude. The fits are very compact: nearly 1600 data are fitted by adjusting 36 constants and freezing 51 at their ab initio values. (C) 1995 American Institute of Physics.
1995
Istituto di Scienze dell'Atmosfera e del Clima - ISAC
Inglese
103
24
10433
10438
Sì, ma tipo non specificato
3
info:eu-repo/semantics/article
262
Dinelli BM Dinelli BM, ; Polyansky OL Polyansky OL, ; J Tennyson J, Tennyson
01 Contributo su Rivista::01.01 Articolo in rivista
none
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/120138
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