[mesa-users] Evolving a white dwarf on the cooling sequence

Jing Luan jingluan at caltech.edu
Mon Jan 9 18:58:14 EST 2012

On 1/9/12 1:39 PM, Francesca Valsecchi wrote:
> Hi all,
> I would like to use MESA to create white dwarf models of different 
> masses and temperatures.
> I created a He white dwarf using one of the test_suite runs and I am 
> trying to evolve it on the cooling sequence.
> I have tried using the test_suite called wd_cool, reading in input the 
> He white dwarf model created, but I did not have success.
> Is there any documentations on the various test_suite that deal with 
> white dwarfs? Also any paper that used MESA to study white dwarfs 
> would be useful.
> Thank you very much!
> Francesca
> ------------------------------------------------------------------------------
> Ridiculously easy VDI. With Citrix VDI-in-a-Box, you don't need a complex
> infrastructure or vast IT resources to deliver seamless, secure access to
> virtual desktops. With this all-in-one solution, easily deploy virtual
> desktops for less than the cost of PCs and save 60% on VDI infrastructure
> costs. Try it free! http://p.sf.net/sfu/Citrix-VDIinabox
> _______________________________________________
> mesa-users mailing list
> mesa-users at lists.sourceforge.net
> https://lists.sourceforge.net/lists/listinfo/mesa-users

I remember I once used mesa to deal with wd cooling and it worked well. 
Actually you do not necessarily need to go to test_suite. Here is my 
suggestion: copy a work directory, edit the inlist_project file to let 
mesa start with the model you already created, and let mesa run. When 
the T and P are too low for further nuclear fusion, the He WD is now on 
its cooling trace. There should be a variable indicating the luminosity 
resulted from nuclear burning ( maybe called Lnuc or something, you can 
check the file mesa/star/public/star_data.dek for the variable name), as 
long as Lnuc<< the total luminosity, the He WD is cooling down. MESA 
will continue running until the equation of state of the central matter 
is uncertain ( I remember it is when lgQ>some critical value, you can 
also check what lgQ is in MESA's document, probably also in the 
star_data.dek file).

Good luck!


Ph.D candidate at physics.caltech
email: jingluan at caltech.edu
address: MC350-17,Caltech,1200 E.California Blvd
          Pasadena, CA 91125

-------------- next part --------------
An HTML attachment was scrubbed...
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20120109/efbf27f7/attachment.html>

More information about the Mesa-users mailing list