[mesa-users] evolving higher mass (e..g. 3Msun) through agb to wd
Bill Paxton
paxton at kitp.ucsb.edu
Fri Jan 18 13:43:45 EST 2013
On Jan 18, 2013, at 10:30 AM, Dave Spiegel wrote:
> I can run a 1-Msun star through the post-MS stages and get a WD at the end within a day or only a little longer. But, for higher-mass stars (e.g., 3-Msun), MESA cranks away for more than a week, doing hundreds of thermal pulses, and still hasn't gotten to a WD when I'm forced by frustration to hit ctrl-c. Is there something I could do differently to end up with a WD at the end of a high-mass-star run in a reasonable amount of time?
Hi Dave,
The only solution I've found is shown in test_suite/make_co_wd --- get the run_star_extras in addition to the inlist.
It runs with "okay_to_reduce_gradT_excess" (aka, MLT++), and after the 1st thermal pulse on the agb, it
turns up the wind to get rid of the envelope. Seems that just as we need something extra when we go from
20 Msun to 30 Msun to get past he burning, we also need help on the agb when we go beyond about 2 Msun.
Good luck!
Cheers,
Bill
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