On the computation of moments in the Super-Transition-Arrays model for radiative opacity calculations
Jean-Christophe Pain, Brian Wilson

TL;DR
This paper improves the computation of moments in the Super-Transition-Arrays model for radiative opacity, offering faster, more accurate formulas and addressing numerical challenges in the process.
Contribution
It introduces new formulas and recursion relations for partition functions and moments, enhancing computational efficiency and stability in the Super-Transition-Arrays method.
Findings
Derived a recursion relation and explicit formula for supershell partition functions.
Proposed a positive-definite, non-alternating formula for moments of any order.
Presented methods to accelerate calculations and avoid numerical difficulties.
Abstract
In the Super-Transition-Array statistical method for the computation of radiative opacity of hot dense matter, the moments of the absorption or emission features involve partition functions with reduced degeneracies, occurring through the calculation of averages of products of subshell populations. In the present work, we discuss several aspects of the computation of such peculiar partition functions, insisting on the precautions that must be taken in order to avoid numerical difficulties. In a previous work, we derived a formula for supershell partition functions, which takes the form of a functional of the distribution of energies within the supershell and allows for fast and accurate computations, truncating the number of terms in the expansion. The latter involves coefficients for which we obtained a recursion relation and an explicit formula. We show that such an expansion can be…
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Taxonomy
TopicsSuperconducting and THz Device Technology · Radio Astronomy Observations and Technology · Antenna Design and Optimization
