[Mesa-users] Plotting evaporation mass loss
Ebraheem Farag
ekfarag at asu.edu
Thu Jul 6 13:31:50 UTC 2023
Hello Divyansh,
I don't believe a mass loss rate due to evaporation exists in MESA by
default. To incorporate the effects of evaporation on the companion star,
you'll likely need to implement equation (12) from the paper you shared
yourself as a run_star_extras routine using an 'other hook', see Extending
MESA
<https://docs.mesastar.org/en/release-r23.05.1/using_mesa/extending_mesa.html#extending-mesa>
and adding extra history/profile output
<https://docs.mesastar.org/en/release-r23.05.1/using_mesa/extending_mesa.html#adding-history-profile-output>.
If you want to model the effects of evaporation mass loss on the evolution
of the companion you can use 'other_wind' or 'other_adjust_mdot' to modify
the mass loss rate of the companion. Otherwise, you can just use the
'data_for_extra_history_columns' function to compute what it would be given
the state of your model, and output it to your history.data file, with no
impact on the evolution of your model, although this is not a
self-consistent approach.
Let me know if this was helpful.
-EbF
On Thu, Jul 6, 2023 at 5:06 AM Divyansh Tripathi 20108 via Mesa-users <
mesa-users at lists.mesastar.org> wrote:
> Hello all, I am working on this paper Kun Jia and Xiang-Dong Li 2015 ApJ
> 814 74
> <https://urldefense.com/v3/__https://iopscience.iop.org/article/10.1088/0004-637X/814/1/74__;!!IKRxdwAv5BmarQ!dRDOrC31zVmVsRVcyVceoMAQX-ji6WgIREat8X_IJnGokaaVSyRY3VLYauHY4iQv8V10hNnGVmjPvBc1b7EaXzfd$>
>
> I have to plot mass-loss rate due to evaporation with star mass.
> I can't figure out which variable in history.data gives this quantity.
>
> Any help would be appreciated.
>
> Regards
> Divyansh Tripathi
> _______________________________________________
> mesa-users at lists.mesastar.org
>
> https://urldefense.com/v3/__https://lists.mesastar.org/mailman/listinfo/mesa-users__;!!IKRxdwAv5BmarQ!dRDOrC31zVmVsRVcyVceoMAQX-ji6WgIREat8X_IJnGokaaVSyRY3VLYauHY4iQv8V10hNnGVmjPvBc1bzhSwvku$
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>
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