[mesa-users] negative age and rotation values in "OSC" file
Juan Carlos Suárez
jcsuarez at iaa.es
Fri Feb 10 13:26:41 EST 2017
Dear Richard,
We have modified a little bit the previous “inlist” in order to include some atmosphere (the default simple atmosphere)
since we are interested in working with the photosphere radius. So we decided to include the following options in the
inlist (attached)
! if true, write atmosphere to pulse files
add_atmosphere_to_pulse_info = .TRUE.
! if true, add point for r=0 to pulse files
add_center_point_to_pulse_info = .FALSE.
! if true, add k=1 cell to pulse files
keep_surface_point_for_pulse_info = .false.
! add double points at discontinuities
add_double_points_to_pulse_info = .TRUE.
Curiously, it seems that now the problem of the negative ages and rotation values is solved, but we
do not know why.
On the other hand unfortunately the computation halted with an error
failed to open LOGS/profile686.data
star_finish_step ierr 28
after_step_loop ierr 28
That is, it halted at model 686, while without the above options MESA reached the 905 models with no errors.
In addition to this, with the above options it seems that MESA has doubled the number
of mesh points (from 4K to 8K). Is that what we should expect? The 4K additional
points are located at the atmosphere?
Thanks!
JC
> On 9 Feb 2017, at 20:38, Juan Carlos Suárez <jcsuarez at iaa.es> wrote:
>
> Yes here it is!
> JC
>> On 9 Feb 2017, at 20:05, RICHARD H D TOWNSEND <townsend at astro.wisc.edu <mailto:townsend at astro.wisc.edu>> wrote:
>>
>> Hi Juan —
>>
>> Can you post the inlist file(s) that you’re using?
>>
>> Many thanks,
>>
>> Rich
>>
>>> On Feb 9, 2017, at 12:43 PM, Juan Carlos Suárez <jcsuarez at iaa.es <mailto:jcsuarez at iaa.es>> wrote:
>>>
>>> Dear colleagues
>>>
>>> I am trying to compute a 1.5 Msun evolutionary model (with solar metallicity) from PMS to TAMS approx.
>>> We have set the options to obtain the .OSC files to be read by our oscillation codes.
>>>
>>> We found that for all the models the age provided has negative values.
>>>
>>> Moreover, although no option for rotation was included in the inlist (i.e. rotation should be zero)
>>> we obtain some models with rotation 0 but others with negative non-zero values
>>>
>>> Any idea?
>>>
>>> Thanks in advance!
>>>
--------------------------------------------------------------------------------------------------------------------
Dr. Juan Carlos Suárez
Ramon y Cajal fellow at Física Teórica y del Cosmos Dept. University of Granada
Facultad de Ciencias. 18071. Granada. Spain
jcsuarez at ugr.es | +34 958249056 | www.ugr.es/~fqm292/
Associate researcher at Stellar Physics Dept. IAA-CSIC
Glorieta de la Astronomia s/n. 18008. Granada. Spain
jcsuarez at iaa.es | +34 958230619 | www.iaa.es
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