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Bulletin of the American Physical Society

Modeling rubidium optical pumping in the intermediate buffer-gas-pressure regime

D. Tupa

Published Jun 9, 2015• 0 citations
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We have made a systematic study of rubidium optical pumping in a simple cylindrical cell geometry with a high-power 10W10\phantom{\rule{0.3em}{0ex}}\mathrm{W}10W diode laser array, low magnetic fields, and buffer-gas pressures of less than 50torr50\phantom{\rule{0.3em}{0ex}}\text{torr}50torr. We have determined rubidium polarizations experimentally for H2{\mathrm{H}}_{2}H2​, N2{\mathrm{N}}_{2}N2​, He, and Ar buffer gases, with Rb number densities from ${10}^{12}\phantom{\rule{0.3em}{0ex}}\text{to}\phantom{\rule{0.3em}{0ex}}{10}^{13}\phantom{\rule{0.3em}{0ex}}{\mathrm{cm}}^{\ensuremath{-}3}$. Comparison to a relatively simple optical pumping model allows us to extract useful information about radiation trapping and quenching effects.
Abstract Optical spectroscopy of atoms and molecules is a field where one usually operates very far from thermal equilibrium conditions. A prominent example is spectroscopy of thin vapors, where the pump irradiation leads to a non-equilibrium distribution within the electronic structure that is well shielded from the environment. Here we describe experimental work investigating absorption and emission lines of rubidium vapor subject to a noble buffer gas environment with pressure 100–200 bar, a regime interpolating between usual gas phase and liquid/solid state conditions. Frequent elastic collisions in the dense buffer gas sample cause a large coupling to the environment. We give a detailed account of recent observations of the Kennard–Stepanov scaling, a Boltzmann-like thermodynamic frequency scaling between absorption and emission profiles, for both atomic and molecular rubidium species in the gaseous environment. Our observations are interpreted as due to the thermalization of alkali-noble gas submanifolds in both ground and electronically excited states respectively. Both pressure broadening and shift of the high pressure buffer gas D -lines system are determined. We also discuss some prospects, including possible advances in collisional laser cooling and optical thermometry.