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update massive star test suites #613

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13 changes: 7 additions & 6 deletions CODEOWNERS
Original file line number Diff line number Diff line change
Expand Up @@ -18,7 +18,7 @@ gyre/ @rhdtownsend @warrickball
hdfio5 @rhdtownsend
interp_1d/ @rhdtownsend
interp_2d/ @rhdtownsend
kap/ @fxt44
kap/ @fxt44 @Debraheem
linters/
turb/
math/ @rhdtownsend
Expand Down Expand Up @@ -88,6 +88,7 @@ star/test_suite/make_he_wd @evbauer @fxt44
star/test_suite/make_metals @fxt44
star/test_suite/make_o_ne_wd @fxt44 @evbauer
star/test_suite/make_planets @fxt44
star/test_suite/make_pre_ccsn_13bvn @Debraheem
star/test_suite/make_sdb @evbauer
star/test_suite/make_zams @fxt44
star/test_suite/make_zams_low_mass @fxt44
Expand Down Expand Up @@ -126,11 +127,11 @@ star/test_suite/wd_he_shell_ignition @wmwolf
star/test_suite/wd_nova_burst @wmwolf
star/test_suite/wd_stable_h_burn @wmwolf

star/test_suite/12M_pre_ms_to_core_collapse
star/test_suite/20M_pre_ms_to_core_collapse
star/test_suite/split_burn_big_net
star/test_suite/zams_to_cc_80
star/test_suite/20M_z2m2_high_rotation
star/test_suite/12M_pre_ms_to_core_collapse @Debraheem
star/test_suite/20M_pre_ms_to_core_collapse @Debraheem
star/test_suite/split_burn_big_net
star/test_suite/zams_to_cc_80 @Debraheem
star/test_suite/20M_z2m2_high_rotation


binary/test_suite/double_bh @orlox
Expand Down
16 changes: 14 additions & 2 deletions docs/source/changelog.rst
Original file line number Diff line number Diff line change
Expand Up @@ -87,10 +87,22 @@ section (see documentation at :ref:`reference/controls:phase_separation_option`)
The phase diagram for O/Ne separation comes from
`Blouin & Daligault (2021b) <https://ui.adsabs.harvard.edu/abs/2021ApJ...919...87B/abstract>`_.

Massive Star test_suite Updates
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

The ``12Msun_pre_ms_to_core_collapse``, ``20Msun_pre_ms_to_core_collapse``, and ``zams_to_cc_80``
test_suites have each been updated and now fully evolve models at solar metallicities to core
collapse while keeping their surface boundaries at tau = 1. The models offer a framework which
has been tested to function with large reaction networks containing > 200 isotopes thanks to
'op_split_burn'. This updates includes the revival of the ``make_pre_ccsn_13bvn`` test_suite
as seen in section 6.9 of MESA IV.


.. _Bug Fixes main:

Bug Fixes
---------

The ZAMS model data used to generate the initial model for simulations with
``create_pre_main_sequence_model = .false.`` and ``load_saved_model = .false.``
had an issue where stars between 1.0 and 1.58 Msun would have a starting
Expand All @@ -100,8 +112,8 @@ and now all pre-computed ZAMS models have a central hydrogen mass fraction very
near 0.697.

The ``fixed_Teff``, ``fixed_Tsurf``, ``fixed_Psurf``, and ``fixed_Psurf_and_Tsurf``
atmosphere options have been reimplemented, although we caution users that their
implementation might conflict with mlt_option = ``TDC``.
atmosphere options were removed in r15140. We have reimplemented them although we
caution users that their implementation could conflict with ``mlt_option = 'TDC'``.

Changes in r23.05.1
===================
Expand Down
4 changes: 2 additions & 2 deletions star/test_suite/12M_pre_ms_to_core_collapse/README.rst
Original file line number Diff line number Diff line change
Expand Up @@ -24,10 +24,10 @@ This test case has six parts.

* Part 4 (``inlist_to_end_core_c_burn``) takes the model to core carbon depletion.

* Part 5 (``inlist_to_lgTmax``) evolves the model until the core temperature reaches log T =9.55 (approximately silicon burning)
* Part 5 (``inlist_to_lgTmax``) evolves the model until the core temperature reaches log T =9.60 (approximately silicon burning)

* Part 6 (``inlist_to_cc``) evolves until core collapse.


Last-Updated: 04Aug2023 by EbF
Last-Updated: 18Dec2023 by EbF

Original file line number Diff line number Diff line change
Expand Up @@ -249,9 +249,9 @@
!log_extra_L ! log10 extra_L

!## neutrino losses
!log_Lneu ! log10 power emitted in neutrinos, nuclear and thermal (in Lsun units)
!log_Lneu_nuc ! log10 power emitted in neutrinos, nuclear sources only (in Lsun units)
!log_Lneu_nonnuc ! log10 power emitted in neutrinos, thermal sources only (in Lsun units)
log_Lneu ! log10 power emitted in neutrinos, nuclear and thermal (in Lsun units)
log_Lneu_nuc ! log10 power emitted in neutrinos, nuclear sources only (in Lsun units)
log_Lneu_nonnuc ! log10 power emitted in neutrinos, thermal sources only (in Lsun units)

!mass_loc_of_max_eps_nuc ! (in Msun units)
!mass_ext_to_max_eps_nuc ! (in Msun units)
Expand Down
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