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An \(L^1\) refined projection approximate solution of the radiation transfer equation in stellar atmospheres - MaRDI portal

An \(L^1\) refined projection approximate solution of the radiation transfer equation in stellar atmospheres (Q1602762)

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scientific article; zbMATH DE number 1758417
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English
An \(L^1\) refined projection approximate solution of the radiation transfer equation in stellar atmospheres
scientific article; zbMATH DE number 1758417

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    An \(L^1\) refined projection approximate solution of the radiation transfer equation in stellar atmospheres (English)
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    24 June 2002
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    The authors consider the numerical solution of a weakly singular second kind Fredholm integral equation which appears in astrophysics by a piecewise constant Galerkin method. They prove convergence in \(L^1\) and develop an iterative refinement method to deal with a large number of unknowns. A parallel implementation of the algorithm and the results of numerical test are discussed.
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    weakly singular kernel
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    second kind Fredholm integral equation
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    iterative refinement
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    parallelization
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    radiation transfer equation
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    stellar atmospheres
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    numerical examples
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    astrophysics
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    Galerkin method
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    convergence
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