From: Bill P. <pa...@ki...> - 2010-06-30 17:57:29
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On Jun 30, 2010, at 8:24 AM, Michelle Dolan wrote: > late stages of evolution of giant stars Hi Shelley, It takes a rather long time for mesa to evolve a massive star from pre-ms to onset of core collapse. Perhaps it would be useful to have a model that was saved about 1000 steps or so before collapse. You can play with that a bit to see how things go before you do the entire evolution yourself. Here's a model that started at 20 Msun and has evolved for 42000 timesteps. You can use it as a starting model by editing your inlist_massive: load_saved_model = .true. !saved_model_name = '25m_z2m2_pre_ms.mod' saved_model_name = '20_z2m2_si_burn.mod' then just do ./rn you should get a terminal line saying load saved model 20_z2m2_si_burn.mod and then it will start with output something like the following: step lg_Tcntr Teff lg_LH lg_Lnuc Mass H_rich H_cntr N_cntr Y_surf X_avg eta_cntr pts retry lg_dt_yr lg_Dcntr lg_Rsurf lg_L3a lg_Lneu lg_Mdot H_poor He_cntr O_cntr Z_surf Y_avg gam_cntr jacs bckup age_yr lg_Pcntr lg_L lg_LZ lg_Psurf lg_Dsurf He_poor C_cntr Ne_cntr Si_cntr Z_avg v_div_cs dt_limit __________________________________________________________________________________________________________________________________________________ 42023 9.817492 3178.888 18.726917 26.365246 15.499273 9.327864 0.000000 0.000000 0.386320 0.353310 5.811636 1426 0 -7.851571 9.034721 3.098539 15.152327 13.568666 -99.000000 6.171409 0.000917 0.000003 0.019955 0.383153 5.146621 10 0 8.9557E+06 26.713394 5.159661 26.365246 2.503420 -8.754533 0.000000 0.000000 0.000000 0.000001 2.635E-01 0.189E+02 varcontrol This plot shows the abundances and this one shows that the infall velocity is about 1 km/sec -- the run will automatically stop when that reaches 1000 km/sec. I hope that will be useful! Cheers, Bill |