Dielectronic Recombination Rates In Astrophysical Plasmas
  In this work we introduce a new expression of the plasma Dielecronic Recombination (DR) rate as a function of the temperature, derived assuming a small deformation of the Maxwell-Boltzmann distribution and containing corrective factors, in addition to the usual exponential behaviour, caused by non-linear effects in slightly non ideal plasmas. We then compare the calculated DR rates with the experimental DR fits in the low temperature region. 
Fatima Bachari, Fabrizio Ferro, Giancarlo Maero and Piero Quarati