[mesa-users] MESA3 paper 7_binary_with_rot

[Roni Waldman]

Sure, and I will.

‫בתאריך יום ג׳, 16 ביוני 2015 ב-10:28 מאת ‪Pablo Marchant‬‏ <‪
pamarca at gmail.com‬‏>:‬

> No, but the use_other_tsync option is there for you to play with it ;)
>
> On Tue, Jun 16, 2015 at 9:10 AM, Roni Waldman <roni181066 at gmail.com>
> wrote:
>
>> Thanks Pablo.
>> Do you happen to have a subroutine for the Tassoul formula?
>> I'm trying to compare to Yoon et al 2010.
>>
>> Roni
>>
>> ‫בתאריך יום ג׳, 16 ביוני 2015 ב-10:04 מאת ‪Pablo Marchant‬‏ <‪
>> pamarca at gmail.com‬‏>:‬
>>
>>> My bad, here it is. Will update the ones on mesastar
>>>
>>> On Tue, Jun 16, 2015 at 8:37 AM, Roni Waldman <roni181066 at gmail.com>
>>> wrote:
>>>
>>>> Hi,
>>>> More on this one.
>>>> The inlist_project has:
>>>>    ! use_other_tsync will use the Zahn timescale as defined in
>>>> run_binary_extras.f
>>>>    !use_other_tsync = .true.
>>>>
>>>> I dont't see any other_tsync in the default run_binary_extras.f, and
>>>> there's no special run_binary_extras.f in the 7_binary_with_rot
>>>> directory.
>>>>
>>>> Roni
>>>>
>>>>
>>>> ‫בתאריך יום ב׳, 15 ביוני 2015 ב-21:11 מאת ‪Roni Waldman‬‏ <‪
>>>> roni181066 at gmail.com‬‏>:‬
>>>>
>>>>> Same here.
>>>>>
>>>>> ‫בתאריך יום ב׳, 15 ביוני 2015 ב-19:37 מאת ‪Willie Strickland‬‏ <‪
>>>>> cwskas at gmail.com‬‏>:‬
>>>>>
>>>>>> Thanks for the confirmation.  I thought they were probably for
>>>>>> debugging, but didnt see obvious way to turn them off.
>>>>>>
>>>>>> Willie
>>>>>>
>>>>>>
>>>>>> On Jun 15, 2015, at 11:13 AM, Pablo Marchant <pamarca at gmail.com>
>>>>>> wrote:
>>>>>>
>>>>>> The w > w_crit messages come from the implicit method that increases
>>>>>> the wind strength so the star does not evolve avobe critical rotation.
>>>>>> Maybe they could be turned off, I mainly used that info for debugging. And
>>>>>> your results are the same as mine.
>>>>>>
>>>>>> On Mon, Jun 15, 2015 at 5:59 PM, Willie Strickland <cwskas at gmail.com>
>>>>>> wrote:
>>>>>>
>>>>>>> Did you get a lot of w > w_crit lines in the rotating one?  I got
>>>>>>> the same results as you it sounds like, but had all these redo lines.
>>>>>>>
>>>>>>> 8,821 lines fix w > w_crit: bisect mdots and redo
>>>>>>>      89 lines w > w_crit: revise mdot and redo
>>>>>>>
>>>>>>> My run finished at step 6429, age 1.254e7, 2.45 mass1, 18.7 mass2.
>>>>>>>
>>>>>>> accretor photosphere has reached its Roche Lobe
>>>>>>>                                      accretor (r-rl)/rl        6429
>>>>>>>    5.0151227593021562D-02
>>>>>>>
>>>>>>> Willie
>>>>>>>
>>>>>>>
>>>>>>>
>>>>>>>
>>>>>>> On Jun 15, 2015, at 7:49 AM, Roni Waldman <roni181066 at gmail.com>
>>>>>>> wrote:
>>>>>>>
>>>>>>> Hi Pablo,
>>>>>>>
>>>>>>> Oops... right, I put the file in the wrong place.
>>>>>>> Rerunning, and let's see what happens.
>>>>>>>
>>>>>>> I also ran the rotating binary example.
>>>>>>> Ended up with donor mass 2.45 Msun and accretor reaching Roche-lobe.
>>>>>>> Does that sound right?
>>>>>>>
>>>>>>> Thanks,
>>>>>>> Roni
>>>>>>>
>>>>>>> ‫בתאריך יום ב׳, 15 ביוני 2015 ב-14:11 מאת ‪Pablo Marchant‬‏ <‪
>>>>>>> pamarca at gmail.com‬‏>:‬
>>>>>>>
>>>>>>>> Roni, together with the inlists there is a run_star_extras.f
>>>>>>>> provided (and in the inlists it is said that you need it). Are you using
>>>>>>>> it? From you output it seems not. This implements the switch from a
>>>>>>>> Kudritski wind to a Hamann one as described in Wellstein & Langer 1999.
>>>>>>>>
>>>>>>>> I guess changing this will make it consistent with that of the
>>>>>>>> paper. Your model is doing some crazy things though.
>>>>>>>>
>>>>>>>> On Mon, Jun 15, 2015 at 9:06 AM, Roni Waldman <roni181066 at gmail.com
>>>>>>>> > wrote:
>>>>>>>>
>>>>>>>>> Hi Pablo,
>>>>>>>>> Too big for one email, will send several.
>>>>>>>>> Thanks,
>>>>>>>>> Roni
>>>>>>>>>
>>>>>>>>> ‫בתאריך יום א׳, 14 ביוני 2015 ב-22:55 מאת ‪Pablo Marchant‬‏ <‪
>>>>>>>>> pamarca at gmail.com‬‏>:‬
>>>>>>>>>
>>>>>>>>>> Roni, can you send me your history.data for each star and
>>>>>>>>>> binary_history.data to compare?
>>>>>>>>>>
>>>>>>>>>> On Sun, Jun 14, 2015 at 8:35 PM, Roni Waldman <
>>>>>>>>>> roni181066 at gmail.com> wrote:
>>>>>>>>>>
>>>>>>>>>>> Hi,
>>>>>>>>>>>
>>>>>>>>>>> I downloaded the inlists of the MESA3 paper, and ran the example
>>>>>>>>>>> 6_massive_binary, without changing anything in the inlists or the code,
>>>>>>>>>>> version 7624.
>>>>>>>>>>> The run ends with the donor having 2Msun, the accretor filling
>>>>>>>>>>> its Roche-lobe, and the time steps being super small (1e-12).
>>>>>>>>>>> This not what seems to happen in the paper.
>>>>>>>>>>> Am I doing anything wrong?
>>>>>>>>>>>
>>>>>>>>>>> Roni
>>>>>>>>>>>
>>>>>>>>>>>
>>>>>>>>>>>
>>>>>>>>>>> ------------------------------------------------------------------------------
>>>>>>>>>>>
>>>>>>>>>>> _______________________________________________
>>>>>>>>>>> mesa-users mailing list
>>>>>>>>>>> mesa-users at lists.sourceforge.net
>>>>>>>>>>> https://lists.sourceforge.net/lists/listinfo/mesa-users
>>>>>>>>>>>
>>>>>>>>>>>
>>>>>>>>>>
>>>>>>>>>>
>>>>>>>>>> --
>>>>>>>>>> Pablo Marchant Campos
>>>>>>>>>> M.Sc on Astrophysics, Universidad Católica de Chile
>>>>>>>>>> PhD student, Argelander-Institut für Astronomie
>>>>>>>>>>
>>>>>>>>>
>>>>>>>>
>>>>>>>>
>>>>>>>> --
>>>>>>>> Pablo Marchant Campos
>>>>>>>> M.Sc on Astrophysics, Universidad Católica de Chile
>>>>>>>> PhD student, Argelander-Institut für Astronomie
>>>>>>>>
>>>>>>>
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>>>>>>> _______________________________________________
>>>>>>> mesa-users mailing list
>>>>>>> mesa-users at lists.sourceforge.net
>>>>>>> https://lists.sourceforge.net/lists/listinfo/mesa-users
>>>>>>>
>>>>>>>
>>>>>>>
>>>>>>
>>>>>>
>>>>>> --
>>>>>> Pablo Marchant Campos
>>>>>> M.Sc on Astrophysics, Universidad Católica de Chile
>>>>>> PhD student, Argelander-Institut für Astronomie
>>>>>>
>>>>>>
>>>>>>
>>>>>> ------------------------------------------------------------------------------
>>>>>> _______________________________________________
>>>>>> mesa-users mailing list
>>>>>> mesa-users at lists.sourceforge.net
>>>>>> https://lists.sourceforge.net/lists/listinfo/mesa-users
>>>>>>
>>>>>
>>>
>>>
>>> --
>>> Pablo Marchant Campos
>>> M.Sc on Astrophysics, Universidad Católica de Chile
>>> PhD student, Argelander-Institut für Astronomie
>>>
>>
>
>
> --
> Pablo Marchant Campos
> M.Sc on Astrophysics, Universidad Católica de Chile
> PhD student, Argelander-Institut für Astronomie
>
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