[Mesa-users] Stationary model
g.mirouh at surrey.ac.uk
g.mirouh at surrey.ac.uk
Tue Nov 13 09:08:06 EST 2018
Hello everyone,
On 13/11/2018 06:04, Pablo Marchant wrote:
> Hi,
>
> depending on what exactly you're trying to do your message could be
> interpreted in different ways. Something that might be close to what
> you're looking, is to fix the composition of the star by setting
>
> dxdt_nuc_factor = 0d0
> mix_factor = 0d0
>
> the first option will keep the energy input from nuclear reactions,
> while ignoring the corresponding changes in composition. The second
> one will remove composition changes due to mixing. You don't want to
> turn off nuclear reactions, because if you do that the star will
> simply lose energy and evolve to higher central temperatures in a
> Kelvin-Helmholtz timescale. If you use these option, you will freeze
> the evolution of the star if you are dealing with phases in thermal
> equilibrium. If the starting model is not in thermal equilibrium, then
> it's trickier.
Thank you Pablo. I implemented these two commands in my inlist, but my
model is not fixed: when I force the dx/dt to 0, the core brutally
expands to find some material to burn... and that's not my aim here.
What I want is simply to completely freeze my model at a given
composition and have it not change anymore. So yes, as you said, I
literally want to fix the structure variables in the star. I guess it
sounds simpler than it is actually...
Thanks a lot to anyone who can help.
--
Gio.
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