[Mesa-users] Degeneracy

[Francis Timmes]

hi étienne,

super. happy stellar modeling.

fxt




> On Dec 8, 2020, at 9:31 AM, Étienne Massé <etiennemasse123 at gmail.com> wrote:
> 
> Hi Francis,
> 
> Thanks a lot for the answer! That folder indeed contains the information we wanted, you were a great help. 
> 
> Étienne
> 
> 
> 
> Le jeu. 3 déc. 2020 à 11:30, Francis Timmes <fxt44 at mac.com> a écrit :
> hi étienne,
> 
> > ... a way to obtain the degeneracy pressure from the MESA outputs ...
> 
> 
> in $MESA_DIR/star/defaults/profile_columns.list you will find
> 
>    !pgas ! gas pressure at center of zone (electrons and ions)
> 
> the gas pressure is dominated by the electrons in electron degenerate regimes.
> this is likely what you want. 
> 
> 
> 
> >  ... H burn line, etc). Is there a way to obtain these lines ...
> 
> 
> $MESA_DIR/data/star_data/plot_info
> 
> stores the data for the eps_nuc = 1 erg/g/s burning curves seen in a pgstar (rho,T) profile plot.
> 
> fxt
> 
> 
> 
> 
> 
> 
> > On Dec 2, 2020, at 10:49 AM, Étienne Massé via Mesa-users <mesa-users at lists.mesastar.org> wrote:
> > 
> > Hello everyone,
> > 
> > A classmate and I are presently working on brown dwarf models and our maximum age is such that they run until the degeneracy pressure alters the EOS enough to crash the simulation. We would like to know if there is a way to obtain the degeneracy pressure from the MESA outputs in a way that it could be used with mesa_reader, for example. 
> > 
> > On another note, we are drawing logT - Log rho graphs using the MESA outputs but they lack the theoretical limits we see in pgstar (Eddington limit, H burn line, etc). Is there a way to obtain these lines and plot them outside of pgstar?
> > _______________________________________________
> > mesa-users at lists.mesastar.org
> > https://lists.mesastar.org/mailman/listinfo/mesa-users
> > 
>