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Titlebook: Numerical Methods for Initial Value Problems in Physics; Francisco S. Guzmán Textbook 2023 The Editor(s) (if applicable) and The Author(s)

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樓主: Embolism
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發(fā)表于 2025-3-23 12:09:13 | 只看該作者
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發(fā)表于 2025-3-23 15:46:55 | 只看該作者
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發(fā)表于 2025-3-23 19:11:53 | 只看該作者
Francisco Guzmánsulted in extensive knowledge of the structure and dynamics of biological macromolecules. This information has been gained by studies of phenomena that affect the excited state, such as the local environment, quenching processes, and energy transfer. Topics in Fluorescence Spectroscopy, Volume 4: Pr
14#
發(fā)表于 2025-3-24 02:12:58 | 只看該作者
Francisco Guzmánsulted in extensive knowledge of the structure and dynamics of biological macromolecules. This information has been gained by studies of phenomena that affect the excited state, such as the local environment, quenching processes, and energy transfer. Topics in Fluorescence Spectroscopy, Volume 4: Pr
15#
發(fā)表于 2025-3-24 05:12:30 | 只看該作者
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發(fā)表于 2025-3-24 09:45:02 | 只看該作者
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發(fā)表于 2025-3-24 17:11:12 | 只看該作者
Finite Volume Methods,ion of the formation of the stationary solar wind assuming spherical symmetry. We also show the power and need of the method in relativistic physics by solving the relativistic Euler equations in . dimensions and with the problem of the accretion of a perfect fluid onto a Schwarzschild black hole.
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發(fā)表于 2025-3-24 20:32:28 | 只看該作者
Textbook 2023tial Value Problems (IVPs). Beginning with IVPs involving Ordinary Differential Equations (ODEs) and progressing to problems with Partial Differential Equations (PDEs) in 1+1 and 3+1 dimensions, it provides readers with a clear and systematic progression from simple to complex concepts...The numeric
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發(fā)表于 2025-3-25 02:48:58 | 只看該作者
Method of Lines for Initial Value Problems Involving PDEs,l Minkowski space-time, which also helps illustrating some concepts of relativistic physics. We also solve Schr?dinger equation with this method and compare the solutions with those constructed previously. We finalize the chapter with an advanced problem of relativity, the accretion of a spherical wave by a black hole.
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