Initialising Radiation Transport Systems #605
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yanfeij
hwhitehead
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It is recommended to read the documentation and try out some of the test
problems first:
https://github.com/PrincetonUniversity/athena/wiki/Non-relativistic-Radiation-Transport
…On Tue, Jul 23, 2024 at 9:53 AM Henry Whitehead ***@***.***> wrote:
Would anyone be able to provide information as to how best to initialize
systems with radiation transfer?
If I wished to study the evolution of a disc of hot gas, do the initial
conditions need to include the details of the radiation field, or will the
code initialize the field from the gas temperature?
Can any advice be given on reasonable numbers of angles to use with RT? If
I was primarily focused on the vertical energy flux, would setting nzeta
= 1 and npsi = 0 result in solving only for the vertical radiation flux?
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Best,
Yan-Fei Jiang
Associate Research Scientist,
Flatiron Institute,
160 Fifth Avenue
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I added an example near the end of the page:
https://github.com/PrincetonUniversity/athena/wiki/Non-relativistic-Radiation-Transport
Hope it is helpful.
…On Wed, Jul 24, 2024 at 7:48 AM Henry Whitehead ***@***.***> wrote:
Perhaps you could help me with some of the definitions in the
documentation. I believe there are four opacities that are used in the code
associated with scattering, Rosseland mean, Planck mean and "radiation
energy weighted mean". I could not find this last opacity in the code
papers referenced in the documentation, do you know how it is defined?
Can any information be given as to the "default" opacity settings, are
they set by free-free absorption? I see an option for enrolling a custom
opacity function, but I do not believe there are any examples of its use in
the wiki or example pgen files. Are there any examples of its usage
available? The only examples I can see feature setting all non-scattering
opacities to constants.
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Yan-Fei Jiang
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Flatiron Institute,
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Answer selected by
hwhitehead
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Extra information about the NR-RT module can be found in this thread. |
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Would anyone be able to provide information as to how best to initialize systems with radiation transfer?
If I wished to study the evolution of a disc of hot gas, do the initial conditions need to include the details of the radiation field, or will the code initialize the field from the gas temperature?
Can any advice be given on reasonable numbers of angles to use with RT? If I was primarily focused on the vertical energy flux, would setting
nzeta = 1
andnpsi = 0
result in solving only for the vertical radiation flux?Beta Was this translation helpful? Give feedback.
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