Fully threaded transport engine: New method for multi-scale radiative transfer

A. O. Razoumov; C. Y. Cardall

doi:10.1111/j.1365-2966.2005.09409.x

Fully threaded transport engine: New method for multi-scale radiative transfer

A. O. Razoumov
, C. Y. Cardall

Theoretical and Computational Physics

Research output: Contribution to journal › Article › peer-review

36 Scopus citations

Abstract

A new, very fast method for 3D radiative transfer on fully threaded grids with arbitrarily high angular resolution is presented. The method uses completely cell-based discretization, and is ideally suited for problems with diffuse background radiation, often encountered in cosmological and star formation models. We find that for accurate statistical study of intergalactic Ly α absorption lines, one needs of the order of a few hundred angular discretization elements even for models without radiative feedback from star-forming galaxies.

Original language	English
Pages (from-to)	1413-1417
Number of pages	5
Journal	Monthly Notices of the Royal Astronomical Society
Volume	362
Issue number	4
DOIs	https://doi.org/10.1111/j.1365-2966.2005.09409.x
State	Published - Oct 1 2005

Keywords

Intergalactic medium
Methods: numerical
Radiative transfer

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10.1111/j.1365-2966.2005.09409.x

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abstract = "A new, very fast method for 3D radiative transfer on fully threaded grids with arbitrarily high angular resolution is presented. The method uses completely cell-based discretization, and is ideally suited for problems with diffuse background radiation, often encountered in cosmological and star formation models. We find that for accurate statistical study of intergalactic Ly α absorption lines, one needs of the order of a few hundred angular discretization elements even for models without radiative feedback from star-forming galaxies.",

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T2 - New method for multi-scale radiative transfer

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AU - Cardall, C. Y.

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Y1 - 2005/10/1

N2 - A new, very fast method for 3D radiative transfer on fully threaded grids with arbitrarily high angular resolution is presented. The method uses completely cell-based discretization, and is ideally suited for problems with diffuse background radiation, often encountered in cosmological and star formation models. We find that for accurate statistical study of intergalactic Ly α absorption lines, one needs of the order of a few hundred angular discretization elements even for models without radiative feedback from star-forming galaxies.

AB - A new, very fast method for 3D radiative transfer on fully threaded grids with arbitrarily high angular resolution is presented. The method uses completely cell-based discretization, and is ideally suited for problems with diffuse background radiation, often encountered in cosmological and star formation models. We find that for accurate statistical study of intergalactic Ly α absorption lines, one needs of the order of a few hundred angular discretization elements even for models without radiative feedback from star-forming galaxies.

KW - Intergalactic medium

KW - Methods: numerical

KW - Radiative transfer

UR - https://www.scopus.com/pages/publications/25844461897

U2 - 10.1111/j.1365-2966.2005.09409.x

DO - 10.1111/j.1365-2966.2005.09409.x

M3 - Article

AN - SCOPUS:25844461897

SN - 0035-8711

VL - 362

SP - 1413

EP - 1417

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 4

ER -

Fully threaded transport engine: New method for multi-scale radiative transfer

Abstract

Keywords

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