2014
DOI: 10.1364/ol.39.000528
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Collimated blue and infrared beams generated by two-photon excitation in Rb vapor

Abstract: Utilizing two-photon excitation in hot Rb vapor we demonstrate the generation of collimated optical fields at 420 and 1324 nm. Input laser beams at 780 and 776 nm enter a heated Rb vapor cell collinear and circularly polarized, driving Rb atoms to the 5D 5∕2 state. Under phase-matching conditions coherence among the 5S 1∕2 → 5P 3∕2 → 5D 5∕2 → 6P 3∕2 transitions produces a blue (420 nm) beam by four-wave mixing. We also observe a forward and backward propagating IR (1324 nm) beam, due to cascading decays throug… Show more

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Cited by 53 publications
(31 citation statements)
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“…It thus represents the CBL generated in the second region with IR seeding. This approximately six-fold CBL intensity increase produced by injecting extra radiation at 5.23 µm emphasizes the importance of the process of amplified spontaneous emission that is responsible for frequency down-conversion, as the enhanced mid-IR light is directly involved in preparing nonlinear polarization for the 5S1/2 -6P3/2 transition (P ~ χ (3) E1 E2 EIR, where χ (3) is nonlinear susceptibility and Ei is the amplitude of the optical field at 780, 776 and 5 320 nm, respectively) and subsequent CBL generation. However, the mechanism of forward-directed mid-IR enhancement shown in Figure 2 remains to be clarified.…”
Section: A Seeding Experimentsmentioning
confidence: 96%
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“…It thus represents the CBL generated in the second region with IR seeding. This approximately six-fold CBL intensity increase produced by injecting extra radiation at 5.23 µm emphasizes the importance of the process of amplified spontaneous emission that is responsible for frequency down-conversion, as the enhanced mid-IR light is directly involved in preparing nonlinear polarization for the 5S1/2 -6P3/2 transition (P ~ χ (3) E1 E2 EIR, where χ (3) is nonlinear susceptibility and Ei is the amplitude of the optical field at 780, 776 and 5 320 nm, respectively) and subsequent CBL generation. However, the mechanism of forward-directed mid-IR enhancement shown in Figure 2 remains to be clarified.…”
Section: A Seeding Experimentsmentioning
confidence: 96%
“…To date, studies of the FWM process in diamond-type energy-level systems in alkali atoms, mostly in Rb, have focused almost exclusively on detecting the CBL and inferring details of the generation process from the blue light properties [1][2][3][4][5][6][7][8][9][10][11][12][13]. The primary reason for this is that the mid-IR radiation at 5.23 µm generated by the process of amplified spontaneous emission (ASE) is completely absorbed by the glass windows of vapour cells usually used in such experiments.…”
Section: B Velocity Selective and Velocity Insensitive Twophoton Excmentioning
confidence: 99%
“…A generated 5.2 µm infrared radiation corresponding to the transition 5D 5/2 → 6P 3/2 , enabling the FWM process, has been observed in some of the experiments [14]. The difference between our scheme and the works in [9][10][11][12][13][14][15][16] is that, instead of the 5D 5/2 state, a lowlying Rydberg state is being excited by pump lasers. As a result, two very different frequencies outside the typical optical regime are generated, namely a THz field on transition 3 and a UV field on transition 4.…”
mentioning
confidence: 97%
“…At relatively low Rb density (N ≤ 6 × 10 12 cm −3 ), only forwarddirected collimated light at 1.37 μm is generated [13]. However, at higher N collimated emission at 1.32 μm dominates, having been observed in both the co-and counter-propagating directions and attributed to nonparametric ASE on the 6S 1∕2 → 5P 1∕2 transition [14].Appearance of the CBL and near-IR emission at 1.37 μm in only the co-propagating direction suggests a common parametric origin. The lifetimes of the 5D 5∕2 , 6P 3∕2 , and 6S 1∕2 levels (240, 120, and 46 ns, respectively) mean that ASE at 5.23 and 2.73 μm can occur along the pencil-shaped region defined by the applied laser beams.…”
mentioning
confidence: 99%
“…At relatively low Rb density (N ≤ 6 × 10 12 cm −3 ), only forwarddirected collimated light at 1.37 μm is generated [13]. However, at higher N collimated emission at 1.32 μm dominates, having been observed in both the co-and counter-propagating directions and attributed to nonparametric ASE on the 6S 1∕2 → 5P 1∕2 transition [14].…”
mentioning
confidence: 99%