Abstract
We study the stability of the energy balance of the electron gas in very-high pressure plasmas against longitudinal perturbations, using a local dispersion analysis. After deriving a dispersion equation, we apply the model to a very-high pressure (100bar) xenon plasma and find instability for electron temperatures T <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">e</sub> in a window between 2400K and (5.5-7)×10 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sup> K, depending on the current density (10 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">6</sup> -10 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">8</sup> A/m <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sup> ). The instability can be traced back to the Joule heating of the electron gas being a growing function of T <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">e</sub> , which is due to a rising dependence of the electron-atom collision frequency on T <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">e</sub> . We then analyze the T <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">e</sub> range occurring in very-high pressure Xe lamps and conclude that only the nearanode region exhibits T <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">e</sub> sufficiently low for this instability to occur. Indeed, previous experiments (e.g., Ref. 1) have revealed that such lamps can develop voltage oscillations accompanied by electromagnetic interference (EMI), and this instability has been pinned down to the plasma-anode interaction. The calculated increment of the instability conforms to the experimental rise time of a single pulse. The above agreement represents an important, although inevitably indirect, confirmation of the theoretical conclusion <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sup> that T <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">e</sub> in the near-anode layer of very-high pressure arcs is quite low.
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