[Mesa-users] Abundance from pre-zams to zams model

Norhasliza Yusof norhaslizay at um.edu.my
Wed Apr 7 11:47:27 UTC 2021


Hi Frank,

Thanks for the info! I have figured out the root cause of my problem.

Best,

Liza

Dr. Norhasliza Yusof, PhD
Senior Lecturer
Department of Physics
University of Malaya
50603 Kuala Lumpur, MALAYSIA
Tel : +60379674238 (office)



On Tue, Apr 6, 2021 at 12:17 PM Francis Timmes <fxt44 at mac.com> wrote:

> hi liza,
>
> there is not enough information provided to offer much help,
> at least as i'm interpreting your message. if the li7 column is
> always in the history file, and its mass fraction begins as
> non-zero and evolves to zero, then perhaps the model is getting
> hot enough and convective enough to destroy the fragile li7.
> you can diagnose the situation by exploring a few pgstar plots
> while the model is running.
>
> fxt
>
>
>
>
>
> > On Apr 5, 2021, at 8:20 AM, Norhasliza Yusof via Mesa-users <
> mesa-users at lists.mesastar.org> wrote:
> >
> > Hello Mesa users,
> >
> > May I know why the list of surface abundances (for example Li7) in the
> pre-zams model produced in the history_column_list is not transferred into
> the history list in zams model. I did some tests in the 1M_prems_to_wd test
> suite and observed the Li7 abundance written in the history_column_list
> (age 1.0E5, Li7 = 3.0681864861534193E-011) during pre_zams and immediately
> after age  ~ 1.2E5, the values for Li7 at both surface and center are zero?
> I just changed the network to pp_cno_extras.net in the original inlist.
> >
> >
> > Best,
> >
> > Liza
> >
> > Dr. Norhasliza Yusof, PhD
> > Senior Lecturer
> > Department of Physics
> > University of Malaya
> > 50603 Kuala Lumpur, MALAYSIA
> > Tel : +60379674238 (office)
> >
>
>

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