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Titlebook: Computational Methods in Transport; Granlibakken 2004 Frank Graziani Conference proceedings 2006 Springer-Verlag Berlin Heidelberg 2006 App

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樓主: Washington
51#
發(fā)表于 2025-3-30 08:50:15 | 只看該作者
52#
發(fā)表于 2025-3-30 16:21:27 | 只看該作者
Finite-Difference Methods Implemented in SATURN Complex to Solve Multidimensional Time-Dependent TraNumerical simulation of multidimensional particle transport problems falls into the category of the most complex and labor-intensive application problems.
53#
發(fā)表于 2025-3-30 19:34:17 | 只看該作者
Radiation Hydrodynamics in Astrophysics, radiation hydrodynamics codes are being used in a growing number of astrophysics problems from energetic out flows of compact remnants such as core-collapse supernovae and active galactic nuclei to the formation of stars and planets to cosmological simulations of the first stars. In this paper, we
54#
發(fā)表于 2025-3-30 22:38:06 | 只看該作者
Radiative Transfer in Astrophysical Applicationsave (and will ever have) about distant objects (exceptions are detected neutrinos from the Sun and supernova SN1987a, and in a near future the gravitational waves). However, there is an even more compelling reason for the a need to deal with detailed radiation transport in astrophysics: In many astr
55#
發(fā)表于 2025-3-31 04:03:39 | 只看該作者
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