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…d to introduce two new 4D arrays for LW flux as LW photons travel in straight lines). Also included USE_ADIABATIC_FLUCTUATIONS to allow the possibility to begin the simulation with homogeneous T_k
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for more information, see https://pre-commit.ci
Codecov Report❌ Patch coverage is
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+ Coverage 88.16% 88.42% +0.25%
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Files 32 32
Lines 4741 4778 +37
Branches 800 811 +11
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+ Hits 4180 4225 +45
+ Misses 401 394 -7
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Branch is finally ready to be reviewed. Unlike what my previous comment says, it is now possible to have In the code itself, I refer to equations from here: https://arxiv.org/pdf/2601.14360. |
steven-murray
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Thanks @jordanflitter as far as I can tell, this is well written and makes sense. I had only a few comments. In addition, it would be great to have a quick tutorial on this model (I know there's the paper, but having something very brief with plots would be good).
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Thanks @steven-murray for you review and suggestions! I haven't made yet the tutorial you asked since I'm not entirely sure what you have in mind (the results that I can show there are basically already presented in the paper). We could discuss this more next time we meet. IMPORTANT NOTE: I don't know if you noticed, but I also added in this PR some "unnecessary" outputs (like the Lya flux) since I needed them for my paper. While these outputs were very useful for my project, their presence adds of course more required memory, which is exactly the issue we try to fix in the other PRs. There are several choices we can make here:
Clearly, I favor option (4) :) |
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Thanks @jordanflitter yeah I think it would be a good idea to sort out how we're going to treat "optional" quantities before merging this, so that users don't all of a sudden get a huge increase in required memory. Let's chat tomorrow. |
… peak and storage memory. They will return
…e Lya multiple scattering effect. Also changed the maxlimit for large files because the figures take ~1.5MB
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Update of what was done since last review:
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docs: improve input parameter docs
This is a draft for the Lya multiple scattering branch.$\alpha$ and $\beta$ , are determined by the current redshift $z$ , the filter radius $R$ and the ionization fraction $x_\mathrm{HI}$ . Unfortunately GSL doesn't support computing 2F3 so I had to come up with my own implementation, which works pretty well based on the tests that I made.$\alpha\gg\beta$ , as in this limit 2F3 approaches the Bessel function. This configuration should be used only as a sanity check that the new window function (multiple scattering = MS) yields the same output as the old one (straight line = SL) in the appropriate limit.
There are now two new flags, called
LYA_MULTIPLE_SCATTERINGandTEST_SL_WITH_MS_FILTER, the latter becomes relevant only when the former is True, while the former is relevant only ifUSE_HALO_FIELD=True.When
LYA_MULTIPLE_SCATTERING=True, ifTEST_SL_WITH_MS_FILTER=False, the code uses a modified window function that replaces the window function of Eq. (22) in Davies, Mesinger, Murray 2025 (it replaces only the window function that is applied on the SFRD, not the one that is applied on X-ray luminosity). It is a subtraction of two hypergeometric functions 2F3 (instead of a subtraction of two Bessel functions) where the parameters of 2F3,When
LYA_MULTIPLE_SCATTERING=True, andTEST_SL_WITH_MS_FILTER=True, the code uses the same modified window function but withCurrently, this branch is designed to work only when
USE_MINI_HALOS=False. With mini-halos, the SFRD is also used for the Lyman-Werner feedback, but the applied filter should correspond to the old one (as LW photons travel in straight lines), which is not supported by the current implementation whenLYA_MULTIPLE_SCATTERING=True. In the future, two new more fields inXraySourceBox(likefiltered_sfr_lwandfiltered_sfr_lw_mini) should be introduced in this setting (thereby increasing the amount of used memory), or alternatively we can throw an error whenUSE_MINI_HALOSandLYA_MULTIPLE_SCATTERINGare both True.