[mesa-users] sdB
Jan-Torge Schindler
jtschindler at email.arizona.edu
Mon May 22 14:12:10 EDT 2017
Dear Rahou,
I have simulated sdB stars with an older version of MESA.
I am not aware that MESA currently has capabilities to simulate the
complicated two star evolution that produces sdB stars.
However my approach was 'mimicking' it by
1.) Start a single star evolution with the initial mass of your sdB
progenitor star.
2.) Run the evolution and then write out a model at the point in time
where you would like the mass transfer to happen. (Somewhat close to but
before the He-flash.
3.) Start the saved model but specify a M_new and let MESA take mass off
from the outside of the star. But beware, you must be careful not too
take off too much mass. Physically, the mass transfer will quench the
H-shell burning and then the mass transfer will stop as well. So never
let MESA take off mass below the H-shell burning zone.
Unfortunately, I am currently travelling and I don't have much time to
elaborate. I did find the old inlists I used with version 7184. Be aware
much has changed since then, but they should give you a head start.
One more advice, turn off wind for the sdB evolution. This let's you
control the total mass better in the beginning and you can turn them on
later for a more 'realistic' simulation ( not sure how realistic the
wind parameters are constraint for sdBs).
At last have a look at our paper from 2015, where I describe how we
modelled sdB stars.
Cheers,
Jan-Torge
On 05/21/2017 08:56 PM, kaoutar lahlou wrote:
> Hi mesa users:
>
> I am traying to figure out the EHB or sdB. I read in an article that
> we need to make simulation between two stars: M _ initial and M _new.
>
> On mesa -binary, what i should make for initial condition ie for M1
> and M2.
>
> Who will be the donor and accretor ?
>
> Thanks
>
> Rahou
>
>
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! inlist_pre_sdB
! contains the parameters controlling this job
! This inlist contains the minimum of information to create a pre_sdB model
&star_job ! this is the star_job namelist
mesa_dir = '/home/jtschindler/MESA/mesa-r7184' ! serenity
create_pre_main_sequence_model = .true.
change_net = .true. ! switch nuclear reaction network
new_net_name = 'pp_cno_extras_o18_ne22.net' ! including all possible processes for hydrogen and helium burning
eos_file_prefix = 'mesa' !equation of state combining HELM,OPAL and SCVH
kappa_file_prefix = 'gs98' ! opacity mix, Grevesse & Sauval 1998
save_model_number = 16700
save_model_filename = '1.0_progenitor_16700.data'
pgstar_flag = .true. !show the pg plots
/ !end of star_job
&controls
max_model_number = 27000
! starting specifications
initial_mass = 1.0d0 ! in Msun units
!using defaults for initial abundances z=0.02,y=0.30,x=68
initial_z = 0.02 !
! output to files and terminal
photostep = 100
profile_interval = 250
history_interval = 1
terminal_interval = 10
write_header_frequency = 10
star_history_name = 'progenitor_history.data'
! mass gain or loss
RGB_wind_scheme = 'Reimers'
AGB_wind_scheme = 'Blocker'
RGB_to_AGB_wind_switch = 1d-4 ! this is the default value
Reimers_wind_eta = 0.5d0
Blocker_wind_eta = 0.5d0
!opacity controls
use_Type2_opacities = .true.
Zbase = 0.02
kap_Type2_full_off_X = 0.71d0
kap_Type2_full_on_X = 0.70d0
! mesh
max_allowed_nz = 64000
mesh_delta_coeff = 1
!MLT
mixing_length_alpha = 2
!overshooting
min_overshoot_q = 1d-3
D_mix_ov_limit = 1d2
overshoot_f_above_nonburn = 0.0
overshoot_f_below_nonburn = 0.0
overshoot_f_above_burn_h = 0.0
overshoot_f_below_burn_h = 0.0
overshoot_f_above_burn_he = 0.0
overshoot_f_below_burn_he = 0.0
overshoot_f_above_burn_z = 0.0
overshoot_f_below_burn_z = 0.0
!Ledoux criterion & semiconvection, thermohaline and semiconvection only applies if ledoux is true
use_Ledoux_criterion = .false.
alpha_semiconvection = 0
thermohaline_option = 'Kippenhahn'
!element diffusion
show_diffusion_info = .true.
do_element_diffusion = .true.
diffusion_calculates_ionization = .true.
/
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! inlist_pre_sdB
! contains the parameters controlling this job
! This inlist contains the minimum of information to create a pre_sdB model
&star_job ! this is the star_job namelist
mesa_dir = '/home/jtschindler/MESA/mesa-r7184' ! serenity
create_pre_main_sequence_model = .false.
change_net = .true. ! switch nuclear reaction network
new_net_name = 'pp_cno_extras_o18_ne22.net' ! including all possible processes for hydrogen and helium burning
eos_file_prefix = 'mesa' !equation of state combining HELM,OPAL and SCVH
kappa_file_prefix = 'gs98' ! opacity mix, Grevesse & Sauval 1998
load_saved_model=.true.
saved_model_name='1.0_Msun_16700_progenitor.data'
relax_mass=.true.
new_mass=0.48
!save_model_number =
!save_model_filename = ''
pgstar_flag = .true. !show the pg plots
/ !end of star_job
&controls
max_model_number = 35000
! starting specifications
initial_mass = 1.0d0 ! in Msun units
!using defaults for initial abundances z=0.02,y=0.30,x=68
initial_z = 0.02 ! solar metallicity
! output to files and terminal
photostep = 100
profile_interval = 100
history_interval = 1
terminal_interval = 10
write_header_frequency = 10
star_history_name = 'sdB_history.data'
! mass gain or loss
RGB_wind_scheme = 'Reimers'
AGB_wind_scheme = 'Blocker'
RGB_to_AGB_wind_switch = 1d-4 ! this is the default value
Reimers_wind_eta = 0.5d0
Blocker_wind_eta = 0.5d0
! mesh
max_allowed_nz = 64000
mesh_delta_coeff = 1
!opacity controlling
use_Type2_opacities = .true.
Zbase = 0.02
kap_Type2_full_off_X = 0.71d0
kap_Type2_full_on_X = 0.70d0
!MLT
mixing_length_alpha = 2
!overshooting
min_overshoot_q = 1d-3
D_mix_ov_limit = 1d2
overshoot_f_above_nonburn = 0.0
overshoot_f_below_nonburn = 0.0
overshoot_f_above_burn_h = 0.0
overshoot_f_below_burn_h = 0.0
overshoot_f_above_burn_he = 0.0
overshoot_f_below_burn_he = 0.0
overshoot_f_above_burn_z = 0.0
overshoot_f_below_burn_z = 0.0
!Ledoux criterion & semiconvection, thermohaline and semiconvection only applies if ledoux is true
use_Ledoux_criterion = .false.
alpha_semiconvection = 0
thermohaline_option = 'Kippenhahn'
!element diffusion
show_diffusion_info = .true.
do_element_diffusion = .true.
diffusion_calculates_ionization = .true.
/
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