[Mesa-users] Minimum requirement for blue loops for supergiants
Jeremy Sakstein
sakstein at sas.upenn.edu
Wed Apr 10 17:58:11 EDT 2019
Hi everyone,
One final question if you don’t mind. I’m trying to go to higher masses and
the loops seem to be hit or miss. Does anyone have any intuition for how I
should vary the over shooting, semi convection, and mixing length
parameters as I go up in mass?
Cheers,
Jeremy
On Wed, Apr 10, 2019 at 2:16 PM Jeremy Sakstein <sakstein at sas.upenn.edu>
wrote:
> Hi Aaron,
>
> I do indeed have some extra code but the extra control parameter being
> zero essentially switches it off.
>
> Cheers,
>
> Jeremy
>
>
>
> On Wed, Apr 10, 2019 at 2:14 PM Aaron Dotter <aaron.dotter at gmail.com>
> wrote:
>
>> Hi Jeremy,
>>
>> In addition to Koushik's very helpful response, I noticed that you have
>>
>> use_other_cgrav=.true.
>>
>> in your inlist. If you have some other code that we can't see, it may be
>> partially responsible for the problems you're encountering.
>>
>> Cheers,
>> Aaron
>>
>> On Wed, Apr 10, 2019 at 12:33 PM Koushik Sen via Mesa-users <
>> mesa-users at lists.mesastar.org> wrote:
>>
>>> Hi Jeremy,
>>>
>>> I ran your inlist in Mesa r10108. I have attached my plot with the mail.
>>>
>>> 1) You need to set Zbase equal to initial_z in the inlist since you are
>>> using Type2opacities.
>>>
>>> 2) I ran two models: one with alpha_mlt = 1.73 and the other 1.3. The
>>> models are till the end of He-burning. I do see a blue loop for 1.3 and a
>>> blue hook for 1.73.
>>>
>>> It seems to stop due to too many backups high up the Hyashi track.
>>>>
>>>
>>> I did not get any problems like this though, the code ran smoothly.
>>>
>>> Cheers,
>>> Koushik
>>>
>>>
>>>
>>>>
>>>> On Wed, Apr 10, 2019 at 10:40 AM Koushik Sen <senkoushik1995 at gmail.com>
>>>> wrote:
>>>>
>>>>> Hi Jeremy,
>>>>>
>>>>> I am not an expert on Cepheid variable stars or the instability strip.
>>>>> However, as far as I know, in the stellar models, it is mainly the mixing
>>>>> length parameter that controls the temperature of the Hayashi line
>>>>> (Kippenhahn & Weigert 1990).
>>>>>
>>>>> I could not understand what you meant by very long simulations. You
>>>>> should get blue loops in the core He-burning phase of the stars. So, your
>>>>> stopping condition should be at least till the end of He burning. You can
>>>>> also share the inlists you are using so that we can reproduce your models
>>>>> ourselves.
>>>>>
>>>>> Cheers,
>>>>> Koushik
>>>>>
>>>>> On Wed, 10 Apr 2019 at 16:22, Jeremy Sakstein <sakstein at sas.upenn.edu>
>>>>> wrote:
>>>>>
>>>>>> Thanks Koushik!
>>>>>>
>>>>>> I just tried with alpha_semiconvenction = 10 and so far I am not
>>>>>> seeing any loops. The Hyashi track also seems to be inside the instability
>>>>>> strip? One thing I noticed is that the time-step is very small. Do I need
>>>>>> very long simulations to see these loops?
>>>>>>
>>>>>> Cheers,
>>>>>>
>>>>>> Jeremy
>>>>>>
>>>>>> On Wed, Apr 10, 2019 at 4:31 AM Koushik Sen <senkoushik1995 at gmail.com>
>>>>>> wrote:
>>>>>>
>>>>>>> Hi Jeremy,
>>>>>>>
>>>>>>> You need efficient semi-convection (alpha_semiconvection=1 or
>>>>>>> higher, preferably 10) to get blue loops in this mass range. More efficient
>>>>>>> semiconvection implies more mixing above the He-core, the hydrogen gradient
>>>>>>> gets steeper and steeper H gradients favour more BSGs. The overshooting
>>>>>>> parameter that you are using is fine. The lesser overshooting you use, the
>>>>>>> smaller will be the He core formed, and you'll be more likely to get BSG
>>>>>>> solutions, but even step_overshoot_f_above_burn_h_core=0.11 should be good
>>>>>>> enough if you use alpha_semiconvection = 10. For more details on
>>>>>>> how overshooting and semi-convection affects the evolution of massive
>>>>>>> stars, you can have a look at this paper:
>>>>>>> http://adsabs.harvard.edu/abs/2019arXiv190310423S.
>>>>>>>
>>>>>>> Hope this helps,
>>>>>>>
>>>>>>> Cheers,
>>>>>>> Koushik
>>>>>>>
>>>>>>> On Tue, 9 Apr 2019 at 21:14, Jeremy Sakstein <sakstein at sas.upenn.edu>
>>>>>>> wrote:
>>>>>>>
>>>>>>>> Hi Everyone,
>>>>>>>>
>>>>>>>> I've been trying to get blue loops for supergiant stars (13M and
>>>>>>>> higher) by starting from a preMS model and evolving. My inlist works
>>>>>>>> perfectly for lower mass stars but I don't see the loops for higher masses.
>>>>>>>>
>>>>>>>> I know that these loops are very sensitive to things like
>>>>>>>> overshooting so I was wondering if anyone had an idea of what the minimum
>>>>>>>> controls I need are to see these loops?
>>>>>>>>
>>>>>>>> I am using the default X and Y with initial Z=0.0006. At the
>>>>>>>> moment, I am just turning the Ledoux criterion on and setting
>>>>>>>> alpha_semiconvection=0.1. I tried several different mixing lengths and
>>>>>>>> overshoot fractions (in the range 0.01 to 0.1) but so far I see nothing.
>>>>>>>>
>>>>>>>> I'd be very grateful for any help you can give.
>>>>>>>>
>>>>>>>> Cheers,
>>>>>>>>
>>>>>>>> Jeremy
>>>>>>>> _______________________________________________
>>>>>>>> mesa-users at lists.mesastar.org
>>>>>>>> https://lists.mesastar.org/mailman/listinfo/mesa-users
>>>>>>>>
>>>>>>>> _______________________________________________
>>> mesa-users at lists.mesastar.org
>>> https://lists.mesastar.org/mailman/listinfo/mesa-users
>>>
>>>
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