Mathematics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...255..490k&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 255, no. 1-2, p. 490-494.
Mathematics
27
Algorithms, Iterative Solution, Nonlinear Equations, Radiative Transfer, Stellar Atmospheres, Approximation, Equilibrium Equations, Matrices (Mathematics), Reaction Kinetics
Scientific paper
Non-LTE radiation transfer calculations can be made much more efficient and powerful, when the Iteration with Approximate Lambda Operators (ALI) is combined with a modern method for solving the nonlinear rate equations which occur within that framework. We explain in detail how Broyden's method from the class of so-called 'least change secant methods' can be applied for that purpose, replacing the conventional Newton iteration. Very positive experiences were collected when we implemented Broyden's method into our non-LTE code for modeling spherically expanding stellar atmospheres (Wolf-Rayet stars). Compared to the conventional Newton algorithm, the new technique offers a twofold advantage. First, the computational effort to solve the equations of statistical equilibrium is greatly reduced (e.g., by a factor of eight in our case), and, second, the number of atomic levels which can be accounted for is increased far beyond the usual limit of 100 where the Newton algorithm becomes numerically unstable.
Hamann Wolf-Rainer
Koesterke Lars
Kosmol P.
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