Abstract
The theoretical interpretation of recent experiments on the time evolution of the temperature in freely expanding, ultracold plasma clouds released from a magneto-optical trap is discussed. The most interesting result of those experiments was the asymptotic behavior T e ∝ t −(1,2±0.1), instead of the behavior proportional to t −2, which was expected for a rarefied monatomic gas in the inertial expansion stage. It is shown that such a substantially slower temperature fall can be well explained by the specific properties of the equation of state of ultracold plasma with a large Coulomb coupling parameter; whereas the heat release in inelastic processes (in particular, three-body recombination) turns out to be relatively unimportant in the first approximation. This conclusion is confirmed by approximate analytic estimates from the model of virializing the energies of charged particles and also by the results of ab initio computer simulations; moreover, the computations demonstrate that the law of decrease in the electron temperature is established very rapidly, when the virialization criterion begins to be satisfied only to within a factor of order unity.
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Original Russian Text © Yu.V. Dumin, 2011, published in Fizika Plazmy, 2011, Vol. 37, No. 10, pp. 919–927.
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Dumin, Y.V. Characteristic features of temperature evolution in ultracold plasmas. Plasma Phys. Rep. 37, 858–865 (2011). https://doi.org/10.1134/S1063780X11090054
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DOI: https://doi.org/10.1134/S1063780X11090054