[Mesa-users] Questions about (step)Overshooting
Matheus Bernini
matheus.b.peron at gmail.com
Fri Sep 28 11:00:32 EDT 2018
Hi Richard,
Indeed, at some points they are too squared (but the gray track it wasn't
made by me, it is one of the public avaliable GENEC tracks, which I
downloaded from Ekström's website). I used ~10000 mesh points,
mesh_delta_coeff = 1.0 and set varcontrol_target = 1.0d-4 .Is this enough
to have a converged state? Actually, is there a practical, or "standard
way" to know if my models are properly converged?
Thanks
Em sex, 28 de set de 2018 às 10:25, RICHARD H D TOWNSEND <
townsend at astro.wisc.edu> escreveu:
> Hi Matheus --
>
> Your tracks in the HR diagram look rather jagged, and it may be that your
> calculations aren't properly converged. Have you tried running with shorter
> timesteps and/or a finer spatial grid?
>
> cheers,
>
> Rich
>
> > On Sep 27, 2018, at 6:39 PM, Matheus Bernini via Mesa-users <
> mesa-users at lists.mesastar.org> wrote:
> >
> > Hello,
> >
> > I'm an undergraduate student and I'm studying evolution of massive stars
> using MESA.
> >
> > I was "playing around" with step overshooting initial values (
> overshoot_f0_...) for hydrogen helium and nonburn core/shell and I noticed
> that slightly changes on f0 (but always keeping f - f0 = 0.1) caused great
> changes on the post-MS phases [figure].
> >
> >
> > overshoot_f0_above_burn_h_core = 0.035
> > step_overshoot_f_above_burn_h_core = 0.135
> >
> > vs.
> >
> > overshoot_f0_above_burn_h_core = 0.030
> > step_overshoot_f_above_burn_h_core = 0.130
> >
> > *For completeness, there was also an exponential overshooting on all of
> the models of 0.001 on helium and hydrogen core/shell
> >
> > If I understood correctly, the f0 is the starting point for the
> overshoot inward the region (core or shell) because the mixing coefficient
> is 0 on the edge of the region, not allowing the computations to happen.
> So, if f0 is just a "trick" to allow the computation of the overshoot, why
> changing it a little causes important changes on the evolution?
> >
> > Thanks :)
> >
> > -----------------------------------------------------------------
> > Matheus Bernini Peron
> > Undergraduate student
> > Observatório do Valongo,
> > Universidade Federal do Rio de Janeiro
> > Ladeira do Pedro Antônio, 43 - Saúde
> > Rio de Janeiro - RJ - CEP 20080-090
> > Brasil
> > ___________________________________________________________
> > Evolution 32Msun, no rotation, Z_init = 0.014, Y_init = 0.266
> > red: 0.135 - 0.035
> > blue: 0.130 - 0.030
> > gray: GENEC (Ekstrom+2012)
> > <image.png>
> >
> <inlist_massive_defaults><inlist_32M0><run_star_extras.f>_______________________________________________
> > mesa-users at lists.mesastar.org
> > https://lists.mesastar.org/mailman/listinfo/mesa-users
> >
>
>
-------------- next part --------------
An HTML attachment was scrubbed...
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20180928/703abbee/attachment.html>
More information about the Mesa-users
mailing list