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Physical Review A

Mesoscopic physics in vapor-phase atomic systems: Collision-shift gradients and the 0-0 hyperfine transition

Andrew Hudson, James C. Camparo

Published Oct 19, 2018• 8 citations
Publisher

Abstract

Vapor-phase atomic clocks and atomic magnetometers are achieving levels of stability and measurement precision today that would have been considered unrealistic in the not too distant past. To make further progress, researchers will need a more detailed understanding of vapor-phase atomic physics, in particular, the manner in which mesoscopic variations of atomic perturbations map onto the observed resonant phenomena: length scales larger than that of homogeneous quantum dynamics, where atoms within some localized region of the vapor all experience the same optical and microwave fields and collisional perturbations; but smaller than that of the vapor as a whole, where the atomic system is described in terms of (for example) vapor pressure, heat content, and optical depth. In this paper, we discuss the issue of mesoscopic physics as it manifests itself in vapor-phase collision-shift gradients affecting the 0-0 hyperfine transition of $^{87}\mathrm{Rb}$. We show that these gradients not only produce increased line broadening but lead to lineshape asymmetry and an increased sensitivity of the observed resonance to power-broadening. We develop a statistical theory describing the experimental results, and through that theory we show that mesoscopic atomic physics encompasses a broader class of phenomena than that described by the circumscribed term ``inhomogeneous broadening.''

DOI
10.1103/physreva.98.042510

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•Jul 28, 2014•0 citations
Vapor-phase atomic clocks and atomic magnetometers are achieving levels of stability and measurement precision today that would have been considered unrealistic in the not too distant past. To make further progress, researchers will need a more detailed understanding of vapor-phase atomic physics, in particular, the manner in which mesoscopic variations of atomic perturbations map onto the observed resonant phenomena: length scales larger than that of homogeneous quantum dynamics, where atoms within some localized region of the vapor all experience the same optical and microwave fields and collisional perturbations; but smaller than that of the vapor as a whole, where the atomic system is described in terms of (for example) vapor pressure, heat content, and optical depth. In this paper, we discuss the issue of mesoscopic physics as it manifests itself in vapor-phase collision-shift gradients affecting the 0-0 hyperfine transition of 87Rb^{87}\mathrm{Rb}87Rb. We show that these gradients not only produce increased line broadening but lead to lineshape asymmetry and an increased sensitivity of the observed resonance to power-broadening. We develop a statistical theory describing the experimental results, and through that theory we show that mesoscopic atomic physics encompasses a broader class of phenomena than that described by the circumscribed term ``inhomogeneous broadening.''
In the early 1980s, it was common to hear that Rb atomic clocks were limited to Sy(τ) = 10-11/τ1/2at best, and that their ultimate frequency stability could never be better than low-parts of 10-13. Twenty-first century Rb clocks put the lie to those pronouncements. Today, it is not uncommon for vapor-cell clocks to exhibit short-term stabilities at low-parts of 10-13/τ1/2, and ultimate stability levels in parts of 10-15. Here, we discuss what it will take to improve those clocks further (e.g., getting the long-term stability to break into the 10-16range). Specifically, it is our contention that next steps will require a better understanding of mesoscopic physics in vapor-phase systems: atomic phenomena occurring on a scale between the microscopic level of quantum dynamics and the macroscopic level of vapor temperature and pressure. Though at present we have some understanding of mesoscopic physics and its effects, much more needs to be understood. Further, while past and present advances have been driven by “one-off” phenomenological discoveries, it is our opinion that rapid advancement will be best facilitated by a more overarching vision of mesoscopic vapor-phase physics, which at present is lacking.
The ac Stark shift (also known as the ``light shift'') is one of the most important physical processes that arises in precision spectroscopy, affecting the basic understanding of field-matter interactions, measurements of fundamental constants, and even the atomic clocks onboard GPS satellites. Although the theory of the ac Stark shift was fully developed by the 1960s and 1970s, precision tests of theory have, for the most part, been few. Taking advantage of recent developments in atomic clock technology, specifically the pulsed approach to atomic signal generation, which allows frequency measurements with a resolution of $\ensuremath{\sim}{10}^{\ensuremath{-}15}$, we demonstrate a methodology for measuring the ac Stark shift. Here, we report results from a precision examination of the ac Stark shift in a vapor phase system, examining the resonant frequency of the 87Rb^{87}\text{Rb}87Rb 0-0 hyperfine transition for a perturbing laser tuned over a broad optical frequency range (18 GHz) around the D1{D}_{1}D1​ absorption resonance. Over the full frequency range the agreement between semiclassical theory and experiment is very good (better than $5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}2}$), and in our experiments we test both the frequency dependence of the scalar and tensor components of the light shift.
The dynamic Stark shift of an inhomogeneously broadened spectral transition has been studied. Our measurements show a shift in the observed 87 Rb ground-state hyperfine transition, which has a nonlinear dependence on light intensity when the conditions for inhomogeneous broadening are met. The nonlinearity is the result of light-intensity gradients in the signal volume, which produce an inhomogeneously broadened asymmetric microwave transition. We show that our measurements are in full agreement with the second-order perturbation-theory treatment of light-induced energy-level shifts when the effects of inhomogeneities are properly taken into consideration. The effects of inhomogeneous broadening must be carefully considered when one extracts oscillator strengths from light-shift data, or performs high-precision laser spectroscopy. Originator-supplied keywords include: AC stark effect, Atomic clocks, Atomic line shapes, Light shifts.
The dynamic Stark shift of an inhomogeneously broadened spectral transition has been studied. Our measurements show a shift in the observed 87Rb^{87}\mathrm{Rb}87Rb ground-state hyperfine transition which has a nonlinear dependence on light intensity when the conditions for inhomogeneous broadening are met. The nonlinearity is the result of light-intensity gradients in the signal volume, which produce an inhomogeneously broadened asymmetric microwave transition. We show that our measurements are in full agreement with the second-order perturbation-theory treatment of light-induced energy-level shifts, when the effects of inhomogeneities are properly taken into consideration. The effects of inhomogeneous broadening must be carefully considered when extracting oscillator strengths from light-shift data, or when performing high-precision laser spectroscopy.
Just as it is possible to stabilize the frequency of an electromagnetic field to an atomic resonance between energy eigenstates, it is possible to stabilize the intensity or brightness of a field to an atomic Rabi resonance. For ease of reference, such a stabilized field is termed an ``atomic candle.'' Here, we describe a microwave atomic candle based on the (F=2,(F=2,(F=2, mF=0){m}_{F}=0)mF​=0)--(F=1,(F=1,(F=1, mF=0){m}_{F}=0)mF​=0) ground-state hyperfine transition of 87Rb{}^{87}\mathrm{Rb}87Rb (6834.7 MHz) as observed in an optically pumped vapor. We discuss the atomic candle's operation and the intensity stability of the field it produces (relative to the Rabi-resonance peak). We then discuss our use of the candle to investigate Rabi-resonance shifts. Specifically, we find that the Rabi resonance depends on the ac Stark shift of the hyperfine transition, the microwave field-atom detuning, and the alkali-metal vapor temperature.
In this work we investigate the transmission in an optical cell containing an atomic vapor, when a laser is tuned to the wings of the Doppler line, presenting inhomogeneous broadening. The experiment is designed to detect the transmission of a laser beam through a an atomic cesium vapor within a quartz cell. Due to the high atomic density in the 1 mm cell, the laser beam is totally absorbed at resonance. On the other hand, when the detuning by few GHz from the center of the line an oscillatory signal is observed as a function of the laser frequency. The amplitude of the transmission signal varies linearly with the laser intensity. These oscillations exhibit diferent behavior as we change some parameters of the system, and the rate of the oscillations vary with laser detuning and on the atomic density. The phase of the transmited field is also sensitive to the angle of incidence of the laser beam in the cell, which allows to vary the lineshape of the signal without changing the parameters of the laser (intensity, frequency, ...) or atomic vapor. Out of resonance with the atomic vapor, the parallel windows of commercial optical cell cavity works as a low finesse Fabry-Pérot with a free spectral range of 150 GHz. However, in resonance, the optical path of the cavity changes varies with frequency due to the dispersive response of the atomic vapor. This study experimentally characterized the transmission signal through a cavity containing resonant vapor as a function of intensity and frequency of the laser, as well as its dependence on the angle of incidence of the beam. A numerical model that allows to determine the collisional broadening of the atomic vapor adjusting the spectral curves of the transmission signal was developed. As an application, exploring the oscillations in the wings of the resonance, we can lock the laser frequency at a few GHz off the center of the atomic resonance. The lock was performed in the frequency range between 0,8 GHz and 2,4 GHz from the center of the D2 line of cesium. To characterize the locking stability we measure the optical beat signal between two similar experiments, using the same locking technique.