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High-Precision Spectroscopy of Molecular Iodine: From Optical Frequency Standards to Global Descriptions of Hyper ne Interactions and Associated Electronic Structure
A widely tunable and high-resolution spectrometer based on a frequency-doubled
Ti:sapphire laser is used to explore sub-Doppler transitions of molecular iodine in the
wavelength range 523 - 498 nm. We investigate the natural width of the hyper
fine
components at various transitions and its wavelength dependence is mapped out in
this region. The narrowest natural width observed is ~52 kHz near 508 nm. The
observed excellent signal-to-noise ratio should lead to high-quality optical frequency
standards that are better than those of the popular 532-nm system. In addition, we
employ a self-referenced femtosecond optical comb to measure the absolute frequency
of the length standard at 514.67 nm, which is based on the a3 hyperfi
ne component
of transition P(13) 43-0. This technique improves the precision of the frequency mea-
surement by two orders of magnitude as compared with previous wavelength-based
results.
The hyper
fine spectra of B ← X transitions in the wavelength range 500-517
nm are investigated systematically. Four effective hyper
fine parameters, eqQB, CB,
dB, and δB, are determined for an extensive number of rovibrational levels spanning
the intermediate region 42 < υ' < 70 in the B0+u (3Πu) state. Near vibrational lev-
els υ' = 57 - 60, the 1g(1Πg) electronic state strongly perturbs the B0+u (3Πu) state
through rotational coincidence, leading to effects such as abnormal variations in the
hyper
fine parameters and strong u-g mixing recorded at the transition P(84) 60-0.
Various perturbation effects in the B0+u (3Πu) state identi
ed so far are summarized.
We have also performed a high-resolution analysis of the six electronic states
that share the same dissociation limit with the excited electronic state B0+u (3Πu) in
molecular iodine. These six states are coupled to the B0+u (3Πu) state via hyper
fine
interactions. The four hyper
fine parameters are calculated using available potential
energy curves and wave functions constructed from the separated-atom basis set. We
obtain a maximum separation of the respective contributions from all six electronic
states and compare each individual contribution with high-precision spectroscopic
data, allowing an independent veri
cation of the relevant electronic structure.
| Attachment | Size |
|---|---|
| chen_lisheng_thesis.pdf | 8.4 MB |
