Temperature-averaged and total free-free Gaunt factors for and Maxwellian distributions of electrons
arXiv:1505.05608 · doi:10.1051/0004-6361/201526104
Abstract
Aims. Optically thin plasmas may deviate from thermal equilibrium and thus, electrons (and ions) are no longer described by the Maxwellian distribution. Instead they can be described by -distributions. The free-free spectrum and radiative losses depend on the temperature-averaged (over the electrons distribution) and total Gaunt factors, respectively. Thus, there is a need to calculate and make available these factors to be used by any software that deals with plasma emission. Methods. We recalculated the free-free Gaunt factor for a wide range of energies and frequencies using hypergeometric functions of complex arguments and the Clenshaw recurrence formula technique combined with approximations whenever the difference between the initial and final electron energies is smaller than in units of . We used double and quadruple precisions. The temperature- averaged and total Gaunt factors calculations make use of the Gauss-Laguerre integration with 128 nodes. Results. The temperature-averaged and total Gaunt factors depend on the parameter, which shows increasing deviations (with respect to the results obtained with the use of the Maxwellian distribution) with decreasing . Tables of these Gaunt factors are provided.
Paper accepted for publication in Astronomy & Astrophysics. Contains 5 pages, 4 figures, and 9 tables
References in corpus (5)
- Detecting shock waves in cosmological smoothed particle hydrodynamics simulations
- Resolving the electron temperature discrepancies in HII Regions and Planetary Nebulae: kappa-distributed electrons
- Measuring nebular temperatures: the effect of new collision strengths with equilibrium and kappa-distributed electron energies
- Accurate determination of the free-free Gaunt factor; I - non-relativistic Gaunt factors
- Discrepancies between the [OIII] and [SIII] Temperatures in HII Regions
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