[Mesa-users] Obtaining information inside __extras.f90 to use for a custom hook
Pablo Marchant
pamarca at gmail.com
Fri Feb 4 17:32:55 UTC 2022
Hi James,
mtransfer_rate is in CGS units (grams per second). b% m1 and b% m2 store
the values of the inlist options with the corresponding names, so they
refer to the initial values. You can access the current masses as b% m(1)
and b% m(2) (they are in grams).
Cheers
On Fri, Feb 4, 2022 at 3:19 PM James Munday via Mesa-users <
mesa-users at lists.mesastar.org> wrote:
> Hi all,
>
> I'm struggling to obtain the information I want when setting a custom hook
> (setting use_other_jdot_ml = .true. in the binary controls).
>
> For what I want to set it to, I need the mass transfer rate (b%
> mtransfer_rate or similar), the masses of the stars at every step and the
> orbital angular momentum, Jorb, at every step. When accessing it, the value
> of b% mtransfer_rate is of the order of ~10^17 for a transfer of 10^-9
> solar masses in pgplot/terminal.
>
> Trying b% m1 and b% m2 just gives what the masses were initialised to be
> in solar masses in inlist_project, and their units and magnitude are not
> consistent with this mtransfer_rate value - I would like the current m1 m2.
> To get Jorb, it is printed in the terminal and log, but I'm not sure how to
> access that live either. I can get b% jdot_gr or b% jdot_ml fine, which are
> identical values to those output in the terminal.
>
> So the options are:
> - Obtain all values in units that are consistent with b% mtransfer_rate
> and compute jdot_ml
> - Obtain all values in the format of those output in terminal and compute
>
> Would someone please give me a point in the right direction for how to do
> either of these options? My subroutine is attached below with comments for
> the desired steps.
>
> Ultimately, I'm trying to get
> jdot_ml_term = Jorb * SQRT(rh*(1.0+mass1/mass2)) * mdot/mass1 ; with rh a
> function of mass1 and mass2 only.
>
> Many thanks in advance for any help,
> James
>
>
> subroutine jdot_extra_jdot_routine(binary_id, ierr)
> integer, intent(in) :: binary_id
> integer, intent(out) :: ierr
> double precision :: mass1, mass2, jdot_ml_term, rh, mdot
> type (binary_info), pointer :: b
> ierr = 0
> call binary_ptr(binary_id, b, ierr)
> if (ierr /= 0) then
> write(*,*) 'failed in binary_ptr'
> return
> end if
>
> mass1 = b% m1 !* m1 here is the donor
> mass2 = b% m2
> !masses above only get the initial mass (in solar masses) set in
> inlist_project, not the current mass from star. think I want to access
> something in s%
> rh = 0.0883 + 0.04858*LOG10(mass2 / mass1) + 0.11489*LOG10(mass2
> / mass1)*LOG10(mass2 / mass1) - 0.020475*LOG10(mass2 / mass1)*LOG10(mass2 /
> mass1)*LOG10(mass2 / mass1)
>
> mdot = b% mtransfer_rate
>
> jdot_ml_term = SQRT(rh*(1.0+mass1/mass2)) * mdot/mass1 ! * Jorb
> <- this is needed
>
> ! WANT Jdot_ml_term = Jorb * SQRT((1+mass1/mass2) * rh ) * mdot
> / mass1
> ! to do this, want the value of M1 and M2 at each step
> ! and the current Jorb
>
>
>
>
> Overall for a run, values have (from reading terminal, mass
> transferring):
> binary_step M1+M2 separ Porb e M2/M1
> pm_i donor_i dot_Mmt eff Jorb dot_J dot_Jmb
> lg_dt M1 R1 P1 dot_e vorb1
> RL1 Rl_gap1 dot_M1 dot_Medd spin1 dot_Jgr dot_Jls
> age_yr M2 R2 P2 Eorb vorb2
> RL2 Rl_gap2 dot_M2 L_acc spin2 dot_Jml rlo_iters
>
> __________________________________________________________________________________________________________________________________________________
>
> bin 540 0.891000 0.093317 0.003498 0.000E+00 3.665089
> 2 1 -1.667E-09 0.942808 2.614E+50 -1.082E+37 0.000E+00
> 2.125646 0.190993 0.025569 0.000000 0.000E+001060.298005
> 0.025568 3.888E-05 -1.667E-09 2.702E-08 0.000E+00 -1.082E+37 0.000E+00
> 1.0624E+07 0.700007 0.000000 0.000000 -2.717E+48 289.296627
> 0.046074 -1.000E+00 1.572E-09 5.399E+36 0.000E+00 -2.419E+32 5
>
> _______________________________________________
> mesa-users at lists.mesastar.org
> https://lists.mesastar.org/mailman/listinfo/mesa-users
>
>
--
Pablo Marchant Campos
M.Sc on Astrophysics, Universidad Católica de Chile
PhD on Astrophysics, Argelander-Institut für Astronomie, Universität Bonn
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