@@ -28,6 +28,15 @@ Previously we had logic to determine if a extra history value should be saved
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as an int or a float (users can only provide data as a float). This was error
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prone, so now we save extra history values as floats.
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+ Asteroseismic scaling relations
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+ ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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+
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+ The default values of the parameters ``delta_nu_sun `` and ``nu_max_sun `` used in the asteroseismic scaling relations
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+ have been updated to the values reported by `Lund et al. (2017) <https://ui.adsabs.harvard.edu/abs/2017ApJ...835..172L/abstract >`_
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+ (:math: `\Delta \nu _\odot = \mathrm {134.91 }\,\mu \mathrm {Hz}` and :math: `\nu _{\mathrm {max},\odot } = \mathrm {3078 }\,\mu \mathrm {Hz}`).
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+ The parameter ``Teff_sun `` has been renamed ``astero_Teff_sun `` to avoid confusion
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+ with the fixed constant ``Teffsun `` in the ``const `` module. ``astero_Teff_sun ``'s
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+ default value has been set to 5772 K, as in `IAU 2015 Resolution B3 <https://ui.adsabs.harvard.edu/abs/2015arXiv151007674M >`_.
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.. _New Features main :
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@@ -47,7 +56,6 @@ to a ``rates_list`` file, or by using the option ``filename_of_special_rate``.
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Several examples in the test suite now make use of these rates, such as
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massive stars and models for building white dwarfs.
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-
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Maximum net size
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~~~~~~~~~~~~~~~~
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@@ -87,10 +95,22 @@ section (see documentation at :ref:`reference/controls:phase_separation_option`)
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The phase diagram for O/Ne separation comes from
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`Blouin & Daligault (2021b) <https://ui.adsabs.harvard.edu/abs/2021ApJ...919...87B/abstract >`_.
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+ Massive Star test_suite Updates
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+ ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
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+
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+ The ``12Msun_pre_ms_to_core_collapse ``, ``20Msun_pre_ms_to_core_collapse ``, and ``zams_to_cc_80 ``
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+ test_suites have each been updated and now fully evolve models at solar metallicities to core
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+ collapse while keeping their surface boundaries at tau = 1. The models offer a framework which
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+ has been tested to function with large reaction networks containing > 200 isotopes thanks to
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+ 'op_split_burn'. This updates includes the revival of the ``make_pre_ccsn_13bvn `` test_suite
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+ as seen in section 6.9 of MESA IV.
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+
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+
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.. _Bug Fixes main :
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Bug Fixes
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---------
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+
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The ZAMS model data used to generate the initial model for simulations with
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``create_pre_main_sequence_model = .false. `` and ``load_saved_model = .false. ``
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had an issue where stars between 1.0 and 1.58 Msun would have a starting
@@ -100,8 +120,8 @@ and now all pre-computed ZAMS models have a central hydrogen mass fraction very
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near 0.697.
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The ``fixed_Teff ``, ``fixed_Tsurf ``, ``fixed_Psurf ``, and ``fixed_Psurf_and_Tsurf ``
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- atmosphere options have been reimplemented, although we caution users that their
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- implementation might conflict with mlt_option = `` TDC ``.
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+ atmosphere options were removed in r15140. We have reimplemented them although we
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+ caution users that their implementation could conflict with `` mlt_option = ' TDC' ``.
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Changes in r23.05.1
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===================
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