run DATE: 2025-03-17 TIME: 15:39:41 reading user weak rate file /n/netscratch/conroy_lab/Lab/ebauer/mesa-git-tests/tmp.zDg8EOGzAt/data/rates_data/rate_tables/S13_r_be7_wk_li7.h5 version_number 3d00b4d set_initial_number_retries 0 net name basic.net kap_option gs98 kap_CO_option gs98_co kap_lowT_option lowT_fa05_gs98 OMP_NUM_THREADS 8 initial_bh_spin is larger than one. It has been set to one. m2 1.0000000000000000D+01 m1 2.0000000000000000D+01 initial_period_in_days 1.5000000000000000D+00 initial_separation_in_Rsun 1.7134537316182040D+01 jdot_multiplier 1.0000000000000000D+00 fr 5.0000000000000003D-02 The binary terminal output contains the following information 'step' is the number of steps since the start of the run, 'lg_dt' is log10 timestep in years, 'age_yr' is the simulated years since the start run, 'M1+M2' is the total mass of the system (Msun), 'M1' is the mass of the primary (Msun) 'M2' is the mass of the secondary (Msun) 'separ' is the semi-major axis of the orbit (Rsun), 'R1' is the radius of the primary (Rsun) 'R2' is the radius of the secondary (Rsun) 'Porb' is the orbital period (days), 'P1' is the rotation period of star 1 (days, zero if not modeling rotation), 'P2' is the rotation period of star 2 (days, zero if not modeling rotation), 'e' orbital eccentricity, 'dot_e' time derivative of e (1/yr), 'Eorb' orbital energy G*M1*M2/2*separation (ergs), 'M2/M1' mass ratio, 'vorb1' orbital velocity of star 1 (km/s), 'vorb2' orbital velocity of star 2 (km/s), 'pm_i' index of star evolved as point mass, zero if both stars are modeled, 'RL1' Roche lobe radius of star 1 (Rsun), 'Rl2' Roche lobe radius of star 2 (Rsun), 'donor_i' index of star taken as donor, 'RL_gap1' (R1-Rl1)/Rl1, 'RL_gap2' (R2-Rl2)/Rl2, 'dot_Mmt', mass transfer rate (Msun/yr), 'dot_M1', time derivative for the mass of star 1 (Msun/yr), 'dot_M2', time derivative for the mass of star 2 (Msun/yr), 'eff', mass transfer efficiency, computed as -dot_M2/dot_M1 (zero if dot_M1=0), 'dot_Medd', Eddington accretion rate (Msun/yr), 'L_acc', accretion luminosity when accreting to a point mass (ergs/s), 'Jorb', orbital angular momentum (g*cm^2/s) 'spin1', spin angular momentum of star 1 (g*cm^2/s), 'spin2', spin angular momentum of star 2 (g*cm^2/s), 'dot_J', time derivative of Jorb (g*cm^2/s^2), 'dot_Jgr', time derivative of Jorb due to gravitational waves (g*cm^2/s^2), 'dot_Jml', time derivative of Jorb due to mass loss (g*cm^2/s^2), 'dot_Jmb', time derivative of Jorb due to magnetic braking (g*cm^2/s^2), 'dot_Jls', time derivative of Jorb due to spin-orbit coupling (g*cm^2/s^2), 'rlo_iters', number of iterations for implicit calculation of mass transfer, All this and more can be saved in binary_history.data during the run. __________________________________________________________________________________________________________________________________________________ step lg_Tmax Teff lg_LH lg_Lnuc_tot Mass H_rich H_cntr N_cntr Y_surf eta_cntr zones retry lg_dt_yrs lg_Tcntr lg_R lg_L3a lg_Lneu lg_Mdot He_core He_cntr O_cntr Z_surf gam_cntr iters age_yrs lg_Dcntr lg_L lg_LZ lg_Lphoto lg_Dsurf CO_core C_cntr Ne_cntr Z_cntr v_div_cs dt_limit __________________________________________________________________________________________________________________________________________________ binary_step rlo_iter di ch_fact curr_mdot next_mdot mdot_up mdot_low rl_gap1 rl_gap2 f result ________________________________________________________________________________________________________________________________ 1 1 1 1.5000 0.000E+00 2.224-112 1.798+308 -1.798+308 -2.360E-01 -1.000E+00 1.000E+00 OK (explicit) ERROR: BH is accreting above Eddington DATE: 2025-03-17 TIME: 15:39:44 finished ******************** wind_fed_bhhmxb failed: does not match test string ********************