Sparse tensor spherical harmonics approximation in radiative transfer (Q414015)

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scientific article; zbMATH DE number 6031687
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Sparse tensor spherical harmonics approximation in radiative transfer
scientific article; zbMATH DE number 6031687

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    Sparse tensor spherical harmonics approximation in radiative transfer (English)
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    8 May 2012
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    radiative transfer equation
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    Galerkin finite element method
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    spectral discretization with harmonics
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    numerical examples
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    Dirichlet boundary value problem
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    The process of stationary radiative transfer is presented as a Dirichlet boundary value problem NEWLINE\[NEWLINE Lu=f,\qquad u|_{\partial\Omega_{-}}=0,NEWLINE\]NEWLINE where \(u(x,s)\) is the radiative intensity, \({\partial\Omega_{-}}\) denote inflow part of the boundary of the domain \( \Omega=D\times S^{d_{s}}\) and the operator \(L\) can be split in the form \( L=T+Q_{\sigma}\) with the operator \(T\) that define the transport part and \(Q_{\sigma}\) is the scattering operator. Using the variational formulation of this problem the authors apply two methods to obtain the approximate solution: a Galerkin finite element method in the physical space and a spectral discretization with the harmonics for the angular variable. The graphical behavior of the error is shown for six examples.
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