[mesa-users] negative age and rotation values in "OSC" file

RICHARD H D TOWNSEND townsend at astro.wisc.edu
Fri Feb 10 13:29:24 EST 2017


Hi Juan-Carlos —

Very interesting! Can you remind me which version of MESA you’re running with?

cheers,

Rich

> On Feb 10, 2017, at 12:26 PM, Juan Carlos Suárez <jcsuarez at iaa.es> wrote:
> 
> 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> 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> 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
> --------------------------------------------------------------------------------------------------------------------
> 
> 
> 
> <inlist_project>



More information about the Mesa-users mailing list