[mesa-users] Lithium

[Matteo Cantiello]

Hi Bruno,
The evolution of (surface) Li for low-mass stars on the RGB and AGB is of course a broad, complex topic. This is mostly due to the sensitivity of Li to temperature. 
Which in turns makes it very sensitive to the (poorly constrained) physics of internal mixing.
If you wanna play around, you can start (for example) with the test_suites 1.5M_with_diffusion and 1M_Thermohaline 

Check Paxton et al. 2013 (Sec 4) and refs therein for more details. 

Cheers,
-M

Matteo Cantiello  |  http://matteocantiello.com/ 
Specialist in Astrophysics  | Kavli Institute for Theoretical Physics
Chief Scientist and Board Member, Authorea  |  https://www.authorea.com/

> On Feb 1, 2016, at 1:03 PM, Bruno Lustosa <bruno.moura.pesquisa at gmail.com> wrote:
> 
> Thank you...
> 
> In fact the behavior of lithium with age, teff, with log g for RGB and AGB stars, for example. I thank everyone.
> 
> 
> 
> 
> 2016-02-01 17:59 GMT-03:00 Aaron Dotter <aaron.dotter at gmail.com <mailto:aaron.dotter at gmail.com>>:
> Hi Bruno,
> 
> What aspect of lithium in stars are you interested in? Let's narrow it down so that people can make useful suggestions.
> 
> Aaron
> 
> 
> On Tuesday, February 2, 2016, Bruno Lustosa <bruno.moura.pesquisa at gmail.com <mailto:bruno.moura.pesquisa at gmail.com>> wrote:
> Hello everyone.
> I am still new in the MES but I'm crawling. Is there any example with lithium and other parameters? I could not find the test_suite something. Help me please.
> 
> 
> Bruno
> 
> 
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