Closed jmstone closed 4 months ago
In GitLab by @pdmullen on Nov 24, 2022, 09:15
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In GitLab by @pdmullen on Nov 24, 2022, 09:18
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In GitLab by @pdmullen on Nov 24, 2022, 09:26
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In GitLab by @pdmullen on Nov 24, 2022, 09:28
marked this merge request as ready
In GitLab by @pdmullen on Nov 24, 2022, 09:28
requested review from @jmstone216
In GitLab by @pdmullen on Nov 25, 2022, 10:06
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In GitLab by @pdmullen on Nov 28, 2022, 09:48
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In GitLab by @jmstone216 on Nov 28, 2022, 14:52
What can I say? A major step forward representing a huge increase in capability, now all in master. I am sure lots of little things can be tweaked in the future, but all looks great to me now.
In GitLab by @jmstone216 on Nov 28, 2022, 14:52
approved this merge request
In GitLab by @jmstone216 on Nov 28, 2022, 14:52
mentioned in commit e2d4cec62fbf3ef4abb7a19a5662df5dce9787fb
In GitLab by @pdmullen on Nov 24, 2022, 09:13
Merges radiation -> master
Overview
This MR introduces a physics module for GR radiation transport plus coupling to (magneto)hydrodynamics. An exhaustive Wiki has been generated here, therefore, I will be brief in the MR text.
New Features
Needs Work
be7f84565b
of the Athena++gr_rad
branch. I still suspect there may be some differences between this implementation and what is in @c-white's currentgr_rad
73dcf16
. What is the better formulation? Are they equivalent?r_\mathrm{KS} = 1
$ and zero intensities for angles with $\lvert n_0 \rvert \leq 0.1
$. This is a hack; we need to do better.