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Physical Review Letters

Observation of Population Inversion by Optical Adiabatic Rapid Passage

M. M. T. Loy

Published Apr 15, 1974• 235 citations
Publisher

Abstract

I report the observation of population inversion by optical adiabatic rapid passage. These observations, on an ${\mathrm{NH}}_{3}$ infrared transition with all the relevant parameters known, agree with theoretical expectations. The pressure dependence of ${T}_{1}$, obtained by this technique, makes possible the first estimate of the collision-induced rotational lifetime of ${\mathrm{NH}}_{3}$ in an excited band, which is significantly longer than the rotational lifetime in the ground vibrational band.

DOI
10.1103/physrevlett.32.814

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I report the observation of population inversion by optical adiabatic rapid passage. These observations, on an NH3{\mathrm{NH}}_{3}NH3​ infrared transition with all the relevant parameters known, agree with theoretical expectations. The pressure dependence of T1{T}_{1}T1​, obtained by this technique, makes possible the first estimate of the collision-induced rotational lifetime of NH3{\mathrm{NH}}_{3}NH3​ in an excited band, which is significantly longer than the rotational lifetime in the ground vibrational band.
This Letter reports the first experimental observation of population inversion of a two-photon transition in NH3{\mathrm{H}}_{3}H3​ using the adiabatic rapid-passage technique. The population inversion was demonstrated by the observation of stimulated two-photon gain and emission. By use of this technique, the two-photon population relaxation time T1{T}_{1}T1​ was measured.
The transition probability PPP in the optical adiabatic rapid passage is calculated for a two-level model with dephasing. In the limit $\frac{{T}_{2}}{{\ensuremath{\tau}}_{p}}\ensuremath{\rightarrow}0$, where T2{T}_{2}T2​ is the dephasing time and ${\ensuremath{\tau}}_{p}$ is the time scale of passage through the resonance region, PPP is given by $P=\frac{[1\ensuremath{-}\mathrm{exp}(\ensuremath{-}\frac{\ensuremath{\pi}{\ensuremath{\chi}}^{2}}{|\stackrel{\ifmmode \dot{}\else \.{}\fi{}}{\ensuremath{\omega}}|})]}{2}$ in which $\ensuremath{\chi}$ is the Rabi flopping frequency at resonance and $\stackrel{\ifmmode \dot{}\else \.{}\fi{}}{\ensuremath{\omega}}$ is the time derivative of the offset angular frequency. Generally, PPP takes its maximum value at an intermediate $\stackrel{\ifmmode \dot{}\else \.{}\fi{}}{\ensuremath{\omega}}$ for fixed $\ensuremath{\chi}$ and is bounded by the above formula and by $P=1\ensuremath{-}\mathrm{exp}(\ensuremath{-}\frac{\ensuremath{\pi}{\ensuremath{\chi}}^{2}}{2|\stackrel{\ifmmode \dot{}\else \.{}\fi{}}{\ensuremath{\omega}}|})$, which gives the asymptotic value in the limit $\frac{{T}_{2}}{{\ensuremath{\tau}}_{p}}\ensuremath{\rightarrow}\ensuremath{\infty}$.