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2016ApJ...824..147A - Astrophys. J., 824, 147-147 (2016/June-3)

Effective hyperfine-structure functions of ammonia.

AUGUSTOVICOVA L., SOLDAN P. and SPIRKO V.

Abstract (from CDS):

The hyperfine structure of the rotation-inversion (v2=0+, 0–, 1+, 1–) states of the 14NH3 and 15NH3 ammonia isotopomers is rationalized in terms of effective (ro-inversional) hyperfine-structure (hfs) functions. These are determined by fitting to available experimental data using the Hougen's effective hyperfine-structure Hamiltonian within the framework of the non-rigid inverter theory. Involving only a moderate number of mass independent fitting parameters, the fitted hfs functions provide a fairly close reproduction of a large majority of available experimental data, thus evidencing adequacy of these functions for reliable prediction. In future experiments, this may help us derive spectroscopic constants of observed inversion and rotation-inversion transitions deperturbed from hyperfine effects. The deperturbed band centers of ammonia come to the forefront of fundamental physics especially as the probes of a variable proton-to-electron mass ratio.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): cosmological parameters - infrared: ISM - line: profiles - molecular data - submillimeter: ISM

Simbad objects: 2

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