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Updated helium nlte page in docs with in-text citation #2574

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2 changes: 1 addition & 1 deletion docs/physics/setup/plasma/helium_nlte.rst
Original file line number Diff line number Diff line change
Expand Up @@ -3,7 +3,7 @@ Helium NLTE

The `helium_treatment` setting in the TARDIS config. file will accept one of three options:
* `none`: The default setting. Populate helium in the same way as the other elements.
* `recomb-nlte`: Treats helium in NLTE using the analytical approximation outlined in an upcoming paper.
* `recomb-nlte`: Treats helium in NLTE using the analytical approximation outlined in :cite:`Boyle2017`.
* `numerical-nlte`: To be implemented. Will allow the use of a separate module (not distributed with TARDIS) to perform helium NLTE calculations numerically.

Recombination He NLTE
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17 changes: 17 additions & 0 deletions docs/tardis.bib
Original file line number Diff line number Diff line change
Expand Up @@ -331,3 +331,20 @@ @ARTICLE{Ore1949
adsurl = {https://ui.adsabs.harvard.edu/abs/1949PhRv...75.1696O},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{Boyle2017,
author = {{Boyle}, Aoife and {Sim}, Stuart A. and {Hachinger}, Stephan and {Kerzendorf}, Wolfgang},
title = "{Helium in double-detonation models of type Ia supernovae}",
journal = {\aap},
keywords = {supernovae: general, white dwarfs, radiative transfer, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics},
year = 2017,
month = mar,
volume = {599},
eid = {A46},
doi = {10.1051/0004-6361/201629712},
archivePrefix = {arXiv},
eprint = {1611.05938},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2017A&A...599A..46B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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