16M_conv_premix
This test suite example re-creates the 16-solar mass main-sequence evolution with the inclusion of convective premixing (using the Ledoux criterion), as detailed in Section 5.3 of the MESA V instrument paper (Paxton et al 2019).
This test case has two parts. Click to see a larger view of a plot.
Part 1 (
inlist_start
) creates a 16 Msun pre-main-sequence model and evolves it for 10 time steps.Part 2 (
inlist_16M_conv_premix
) continues the evolution until core hydrogen depletion (mass fraction h1_center < 1e-6).
A Kippenhahn diagram shows the evolution of a retreating convective core on the main sequence, the blue region between model numbers 240 and 385. This can be compared to Figure 41 in the MESA V instrument paper, and the predictive mixing Kippenhahn diagram in 16M_predictive_mix.
pgstar commands used for the plots above:
&pgstar
file_white_on_black_flag = .true. ! white_on_black flags -- true means white foreground color on black background
file_device = 'png' ! png
file_extension = 'png'
!file_device = 'vcps' ! postscript
!file_extension = 'ps'
pgstar_interval = 10
file_digits = 8
Kipp_win_flag = .true.
! window properties
Kipp_win_width = 12
Kipp_win_aspect_ratio = 0.75
Kipp_txt_scale = 0.9
Kipp_title = ''
! y axis limits
Kipp_mass_max = 16.0
Kipp_mass_min = 0
Kipp_show_mass_boundaries = .true.
! x axis limits
Kipp_xaxis_name = 'model_number'
Kipp_xmax = -101 ! maximum step number. negative means use default.
Kipp_xmin = 0 ! minimum step number. negative means use default.
Kipp_show_mixing = .true.
Kipp_show_burn = .true.
Kipp_show_luminosities = .true.
! file output
Kipp_file_flag = .true.
Kipp_file_dir = 'kipp_png'
Kipp_file_prefix = 'kipp_'
Kipp_file_interval = 10 ! output when mod(model_number,file_interval)==0
Kipp_file_width = 12 ! (inches) negative means use same value as for window
Kipp_file_aspect_ratio = -1 ! negative means use same value as for window
/ ! end of pgstar namelist
Last-Updated: 27May2021 (MESA ebecc10) by fxt