A Coupled-channels Potential Fit Describing The Low-lying X<sup>2</sup>∆, <sup>2</sup>Π And <sup>2</sup>Σ<sup>+</sup> States Of Nih To Experimental Accuracy
Havalyova, Ilvie
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https://hdl.handle.net/2142/111174
Description
Title
A Coupled-channels Potential Fit Describing The Low-lying X2∆, 2Π And 2Σ+ States Of Nih To Experimental Accuracy
Author(s)
Havalyova, Ilvie
Contributor(s)
Crozet, Patrick
Ross, Amanda J.
Pashov, Asen
BOZHINOVA, Ivayla
Issue Date
2021-06-25
Keyword(s)
Small molecules
Abstract
A direct potential fit to Hund's case (a) potential curves for the low-lying `supermultiplet' states (${X{}^2\Delta}$, ${{}^2\Pi}$, ${}^2\Sigma^{+}$) of NiH
and to R-dependent spin-orbit and rotational coupling functions has reproduced the experimental term values of $^{58}$NiH, $^{60}$NiH, $^{62}$NiH up to 6500 cm$^{-1}$,
with a root mean square deviation very close to the estimated uncertainty of 0.01 cm$^{-1}$.
Second-order Born-Oppenheimer breakdown corrections to the rotational Hamiltonian had to be included to achieve this result.
The spin-orbit interaction A$_{so}$(R) associated with Ni$^{+}$ is large compared to the energy separations between the three electronic states, so that most of the observed rovibrational states
are strong mixtures of the $\Omega$-components of the multiplet. This made the fitting procedure particularly difficult, because there were no
perturbation-free data to determine the starting values for the model functions. Potential curves were optimized from RKR turning-points generated from
earlier work using an effective Hamiltonian approach\footnote{M. Abbasi $et~al$, J. Mol. Spectrosc. \underline{349} 49-59 (2018)}, and the spin-orbit and rotational coupling functions from theoretical predictions\footnote{C. Marian, J. Chem. Phys., \underline{93(2)} 1176-1186 (1990)}.
We believe that this model may be reliably extrapolated to higher rotational states, with potential applications in the simulation
of high temperature spectra, for example in the context of stellar atmospheres.
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