Volume 18, n u m b e r 1
OPTICS ('OMMUNICATtONS L5
July I!~ 7¢,
FOUR-WAVE MIXING 1N GASES
(Invited) P. SOROKIN IBM Thomas Z Watson Research ('enter. ~orktow~ Heights, New York 10598, USA Not received
L6
FOUR-WAVE SUM-MIXING IN NO, 1400 to 1510 A
[Invited) Stephen C. WALLACE, K.K. INNES and B.P. STOICHEFF
Department of Physics, University of Toronto, Toronto, Ontario, Canada, M5S IA 7
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ub-toe Fig. 1. Three-dimensional plot of X(3)(-tJ3 , WO, COl, - w 2) versus the two intermediate frequencies w o - w 2 and ~ 1 - w2, for the region near two sharp R a m a n resonances of the sample. n o u n c e d change in the shape of one resonance as w 0 - co 2 is varied in steps across the other resonance. Experimentally, about 20 cuts in the 3-D surface in fig. t were scanned. T h e y proved to be virtually identical to the predicted theoretical curves. Similar results were f o u n d in the CuC1 case, where the interference is between uv exciton and ir polariton resonances of the material. Since the two resonances used in the double-resonance experiment do n o t need to be characteristics of the same material or solution, this experiment is useful for making accurate relative m e a s u r e m e n t s of the u n k n o w n strength of a R a m a n or two-photon resonance in terms of a k n o w n R a m a n or t w o - p h o t o n strength. For example, the exciton strength of CuC1 could be compared with the strength of the 1088 cm - I R a m a n line of calcite, or the strength of the 802 cm- 1 R a m a n line of cyclohexane could be compared to the well-known strength of the 992 cm - ! R a m a n line o f benzene. This calibration procedure m a y be very useful, since it avoids the difficulties usually e n c o u n t e r e d in such comparison measurements. In the double-resonance experiment, a strong resonance m a y be used to cancel the n o n r e s o n a n t background susceptibility. This background has been the limiting factor in the sensitivity of the single-resonance experiment to measure weak resonances.
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Recent progress in sum-frequency mixing to generate coherent light in the vacuurn'ultraviotet (vuv) has been based on the use of atomic vapours, such as Rb [ 1 ], Sr [2], and Mg [3], as the non-linear media. As an alternative to using metal vapours one m a y choose a molecular system as the non-linear material. A molecular gas can be used directly in a simple cell (without the complexities introduced by heat-pipe ovens, necessary for these atomic systems). Moreover, phase matching is simplified and good optical h o m o g e n e i t y over arbitrary lengths is assured. We report the first observations of resonantly enhanced, four wave sum-mixing into the vuv via a molecular gas, nitric oxide (NO). The incident frequencies were provided by two H~insch type dye lasers (0.1 cm - 1 linewidth) p u m p e d by a nitrogen laser (Molectron UV-1000). Nitric oxide was carefully purified by fractional distillation to remove impurities which attenuate the harmonic radiation. The dye laser radiation was focussed to a confocal beam parameter b = 1.2 cm, in the center of a glass cell 13 cm in length. The vuv radiation passed through LiF optics to a one-meter m o n o c h r o m a t o r and was detected with a solarblind photomultiplier. The two-photon transition in NO which provided the resonant e n h a n c e m e n t of the third order, non-linear susceptibility ×(3) was A ( 2 ~ +) - X(2H) in which A ( 2 Z +) is the lowest Rydberg state. Thus, a single dye laser t u n e d over a 170 c m - l ~ f r e q u e n c y range a b o u t 4530 A (the 0,0 band [4] ) or 4300 A (the 1, 0 band), produced strong third harmonic radiation in the region 1510 A and 1433 A. respectively. The peak intensity of the third harmonic was observed at the 2E+ - 2H1/2 sub-band head. Wider tunahility was then obtained by fixing one frequency to the strongest two-photon transition and tuning a second dye laser over other transitions in the Rydberg manifold [5]. Although the third order non-linear susceptibility o f NO is ~ 1 0 - 2 of that observed for the equivalent metal vapour syst e m (Ca, Sr), reasonable conversion efficiencies were realized by choosing higher n u m b e r densities. Thus, with an NO pressure of 200 torr and the appropriate phase matching, a power conversion efficiency o f 3 x 10 - 7 (107 photons per pulse) was obtained at vuv wavelengths of 1508 A and 1422 A. Dye laser powers up to 20 kW were used and no evidence for saturation of the conversion efficiency at higher laser powers was observed.