Discontinuous Galerkin finite element methods for radiative transfer in spherical symmetry

被引:13
|
作者
Kitzmann, D. [1 ,2 ]
Bolte, J. [3 ]
Patzer, A. B. C. [3 ]
机构
[1] Univ Bern, Inst Phys, Sidlerstr 5, CH-3012 Bern, Switzerland
[2] Univ Bern, Ctr Space & Habitabil, Sidlerstr 5, CH-3012 Bern, Switzerland
[3] Tech Univ Berlin, Zentrum Astron & Astrophys, Hardenbergstr 36, D-10623 Berlin, Germany
基金
瑞士国家科学基金会;
关键词
radiative transfer; methods: numerical; stars: atmospheres; MULTIDIMENSIONAL LINE TRANSFER; OPERATOR PERTURBATION; MULTILINE TRANSFER; ATMOSPHERES; DYNAMICS; SYSTEMS; SCHEME;
D O I
10.1051/0004-6361/201628578
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The discontinuous Galerkin finite element method (DG-FEM) is successfully applied to treat a broad variety of transport problems numerically. In this work, we use the full capacity of the DG-FEM to solve the radiative transfer equation in spherical symmetry. We present a discontinuous Galerkin method to directly solve the spherically symmetric radiative transfer equation as a two-dimensional problem. The transport equation in spherical atmospheres is more complicated than in the plane-parallel case owing to the appearance of an additional derivative with respect to the polar angle. The DG-FEM formalism allows for the exact integration of arbitrarily complex scattering phase functions, independent of the angular mesh resolution. We show that the discontinuous Galerkin method is able to describe accurately the radiative transfer in extended atmospheres and to capture discontinuities or complex scattering behaviour which might be present in the solution of certain radiative transfer tasks and can, therefore, cause severe numerical problems for other radiative transfer solution methods.
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页数:14
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