Extending the emission range of gas lasers is an attractive proposition, for example, in laser spectroscopy, atmosphere sensing, laser media diagnostics, initiating chemical reactions, and separating elemental isotopes. In this context, carbon monoxide (CO) lasers offer several advantages over other sources of IR radiation, including control of output energy and pulse duration over a wide dynamic range. Moreover, they ensure high average power in repetitively pulsed modes. An electric discharge CO laser can operate on every spectral line from among a few hundred in both fundamental ( 4.7–8.2 m)1 and firstovertone ( 2.5–4.2 m) spectral bands.2–4 In addition, parametric frequency conversion (i.e., frequency doubling, or sum or difference frequency generation) of CO laser radiation using a single nonlinear crystal can cover both midand far-IR spectral ranges. However, to achieve high-frequency conversion efficiency, CO laser radiation must have high peak power. The first mode-locked (i.e., pulsing) laser was reported decades ago. But it had a peak power of only a few kilowatts because it operated at room temperature. No efforts have been made since then to obtain substantially higher power. We have developed a cryogenically cooled, electron-beamsustained-discharge (EBSD) mode-locked CO laser that produces a train of 5–15ns full width at half-maximum spikes with a pulse repetition rate of 10MHz in the mid-IR range of 5 m.5 We obtained maximum output power of up to 120kW for a multiline mode and 70kW for a single-line mode of operation. As suggested elsewhere,6 such radiation could be used to pump an optical parametric amplifier for stochastic cooling in a relativistic heavy-ion collider (see Figure 1). Figure 1. Imaginary layout of the optical stochastic cooling system for the relativistic heavy-ion collider (Brookhaven National Laboratory, US). The storage ring measures 4km. CO: Carbon monoxide. : Wavelength. OPA: Oscillator-power amplifier. : Wavelength.
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