51st Annual Meeting of the APS Division of Atomic, Molecular and Optical Physics
Volume 65, Number 4
Monday–Friday, June 1–5, 2020;
Portland, Oregon
Session Q01: Poster Session III
4:00 PM,
Thursday, June 4, 2020
Room: Exhibit Hall E
Abstract: Q01.00152 : Energy structure and transition data of doubly ionized mercury: Hg III.
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Abstract
Authors:
AADIL RASHID
(Aligarh Muslim University)
TAUHEED AHMAD
(Aligarh Muslim University)
The spectrum of doubly ionized mercury (Hg III) has been studied in the
wavelength region of 400 - 2000{\AA}. The Hg III is Au II like ion with its
ground configuration 5d$^{\mathrm{10\thinspace
}}(^{\mathrm{1}}$S$_{\mathrm{0}})$. The outer electron excitations are of
the type 5d$^{\mathrm{9}}$n$\ell $(n$\ge $5). Some low lying internal
excitations 5d$^{\mathrm{8}}$6s$^{\mathrm{2}}$ and 5d$^{\mathrm{8}}$6s6p
have also been reported along with 5d$^{\mathrm{9}}$ (6s, 7s {\&} 6p)
configurations. We are investigating particularly 5d$^{\mathrm{9}}$6d and
5d$^{\mathrm{9}}$8s configurations for missing levels with the aid of
experimental recordings made on a 3-m normal incidence vacuum spectrograph
using a triggered spark source. The spectra of 5d ion(s) are composite not
only quantitatively but also qualitatively, due to the overlap of
configurations. Their study requires high-resolution spectral instruments in
the ultra-violet wavelength region as well as reliable methods for the
interpretation of the spectra. The \textit{ab-initio} calculations were carried out by means
of R. D. Cowan's Hartree-Fock code with superposition of configurations and
relativistic corrections to predict the energy eigenvalues as well as the
associated wavelength and transition probabilities along with the
cancellation factor. The entire analysis was freshly carried out and was
found that earlier reported values were satisfactory except the levels of
5d$^{\mathrm{9}}$8s configuration. Only $^{\mathrm{3}}$D$_{\mathrm{3}}$
level of this configuration is being confirmed in the present work and the
others were newly established. Final results were interpreted by least
squares fitted parametric calculations. We have used Ritz extrapolation
formula using a least squares fitting code RITZPL to calculate the
ionization limit. With the three member 5d$^{\mathrm{9}}$ns series, the
ionization potential was found to be 278200 \textpm 400
cm$^{\mathrm{-1\thinspace }}$(34.49 \textpm 0.05eV).