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Stochastic sheath heating is the dominant heating mechanism at low pressures for radio frequency (RF) capacitive discharges. It produces an electron energy probability distribution function (EEPF) that approximates a two-temperature Maxwellian, as seen in both experiments and numerical simulations. We have used the fundamental kinetic equation to obtain a space- and time-averaged kinetic equation. We assume that electrons with the x component kinetic energy lower than a certain threshold /spl Phi/ are prevented from interacting with the sheath heating fields. With these approximations and either a knowledge of the central density or an ansatz on /spl Phi/, we obtain a self-consistent solution for the quasiequilibrium discharge parameters valid for low pressures in argon. The results are compared to those found in experiments, yielding reasonable agreement.
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Wang et al. (1998) studied this question.
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