[mesa-users] MESA3 paper 7_binary_with_rot

[Pablo Marchant]

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
>>>>>
>>>>
>>>> ------------------------------------------------------------------------------
>>>> _______________________________________________
>>>> 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
-------------- next part --------------
An HTML attachment was scrubbed...
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20150616/51d8689e/attachment.html>
-------------- next part --------------
A non-text attachment was scrubbed...
Name: run_binary_extras.f
Type: text/x-fortran
Size: 3408 bytes
Desc: not available
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20150616/51d8689e/attachment.bin>