GUIDING CENTER ATOMS - 3-BODY RECOMBINATION IN A STRONGLY MAGNETIZED PLASMA

The three-body recombination rate is calculated for an ion introduced into a magnetically confined, weakly correlated, and cryogenic pure electron plasma. The plasma is strongly magnetized in the sense that the cyclotron radius for an electron r(ce) = square-root-k(B)T(e)/m(e)/OMEGA-ce is small compared to the classical distance of closest approach b = e2/k(B)T(e), where T(e) is the electron temperature and OMEGA-ce = eB/m(e)c is the electron cyclotron frequency. Since the recombination rate is controlled by a kinetic bottleneck a few k(B)T(e) below ionization, the rate may be determined by considering only the initial cascade through states of electron-ion pairs with separation of order b. These pairs may be described as guiding center atoms since the dynamics is classical and treatable with the guiding center drift approximation. In this paper, an ensemble of plasmas characterized by guiding center electrons and stationary ions is described with the BBGKY hierarchy. Under the assumption of weak electron correlation, the hierarchy is reduced to a master equation. Insight to the physics of the recombination process is obtained from the variational theory of reaction rates and from an approximate Fokker-Planck analysis. The master equation is solved numerically using a Monte Carlo simulation, and the recombination rate is determined to be 0.070(10)n(e)2v(e)b5 per ion, where n(e) is the electron density and v(e) = square-root k(B)T(e)/m(e) is the thermal velocity. Also determined by the numerical simulation is the transient evolution of the distribution function from a depleted potential well about the ion to its steady state.