! profile_columns.list -- determines the contents of star model profiles ! you can use a non-standard version by setting profile_columns_file in your inlist ! units are cgs unless otherwise noted. ! reorder the following names as desired to reorder columns. ! comment out the name to omit a column (fewer columns => less IO => faster running). ! remove '!' to restore a column. ! if you have a situation where you want a non-standard set of columns, ! make a copy of this file, edit as desired, and give the new filename in your inlist ! as profile_columns_file. if you are just adding columns, you can 'include' this file, ! and just list the additions in your file. note: to include the standard default ! version, use include '' -- the 0 length string means include the default file. ! if you need to have something added to the list of options, let me know.... ! the first few lines of the profile contain general info about the model. ! for completeness, those items are described at the end of this file. ! note: you can include another list by doing ! include 'filename' ! include '' means include the default standard list file ! the following lines of the profile contain info for 1 zone per row, surface to center. zone ! numbers start with 1 at the surface logT ! log10(temperature) at center of zone logRho ! log10(density) at center of zone logP ! log10(pressure) at center of zone logR ! log10(radius/Rsun) at outer boundary of zone luminosity ! luminosity at outer boundary of zone (in Lsun units) logL ! log(max(1d-6,L/Lsun)) velocity ! velocity at outer boundary of zone -- 0 if no velocity variable entropy ! specific entropy divided by (avo*kerg) conv_mixing_type ! mixing types are defined in mesa/const csound ! sound speed v_div_csound ! velocity divided by sound speed !binding_energy ! v^2/2 - G m / r + E + P/rho (ergs/gm). negative if bound. v_div_r ! velocity divided by radius !scale_height ! pressure scale height; P / (g rho) (in Rsun units) eta ! electron degeneracy parameter (eta >> 1 for significant degeneracy) mu ! mean molecular weight per gas particle (ions + free electrons) logdq ! log10(dq) dq_ratio ! dq(k-1)/dq(k) q ! fraction of star mass interior to outer boundary of this zone radius ! radius at outer boundary of zone (in Rsun units) temperature ! temperature at center of zone tau ! optical depth logtau ! log10(optical depth) at center of zone pressure ! total pressure at center of zone (pgas + prad) !pgas ! gas pressure at center of zone (electrons and ions) pgas_div_ptotal ! pgas/pressure logPgas ! log10(pgas) !prad ! radiation pressure at center of zone !energy ! internal energy (ergs/g) !logE ! log10(specific internal energy) at center of zone grada ! dlnT_dlnP at constant S !dE_dRho ! at constant T !cv ! specific heat at constant volume !cp ! specific heat at constant total pressure logS ! log10(specific entropy) !gamma1 ! dlnP_dlnRho at constant S !gamma3 ! gamma3 - 1 = dlnT_dlnRho at constant S !theta_e ! electron degeneracy factor for graboske screening !gam ! plasma interaction parameter (> 160 or so means starting crystallization) free_e ! free_e is mean number of free electrons per nucleon !logfree_e ! log10(free_e), free_e is mean number of free electrons per nucleon !chiRho ! dlnP_dlnRho at constant T !chiT ! dlnP_dlnT at constant Rho abar ! average atomic weight (g/mole) !zbar ! average charge !z2bar ! average charge^2 ye ! average charge per baryon = proton fraction !opacity ! opacity measured at center of zone log_opacity ! log10(opacity) eps_nuc ! ergs/g/sec from nuclear reactions (neutrinos subtracted) non_nuc_neu ! non-nuclear-reaction neutrino losses !nonnucneu_plas ! plasmon neutrinos (for collective reactions like gamma_plasmon => nu_e + nubar_e) !nonnucneu_brem ! bremsstrahlung (for reactions like e- + (z,a) => e- + (z,a) + nu + nubar) !nonnucneu_phot ! photon neutrinos (for reactions like e- + gamma => e- + nu_e + nubar_e) !nonnucneu_pair ! pair production (for reactions like e+ + e- => nu_e + nubar_e) extra_heat !logPvisc ! log10 artificial viscosity pressure eps_grav ! heat from gravitational contraction (negative for expansion) mlt_mixing_length ! mixing length for mlt (cm) mlt_mixing_type log_D_mix ! log10 diffusion coefficient in units of cm^2/second (Eulerian) log_conv_vel ! log10 convection velocity (cm/sec) conv_vel_div_csound ! convection velocity divided by sound speed log_mlt_D_mix ! log10 cdc from mlt (cm^2/sec) !use_gradr_for_gradT ! if = 1, then zone has been forced radiative in spite of mlt results. pressure_scale_height ! in Rsun units gradT ! mlt value for required temperature gradient dlnT/dlnP gradr ! dlnT/dlnP required for purely radiative transport dlnd_dt ! time derivative of log(density) at fixed mass coordinate (Langranian) dlnT_dt ! time derivative of log(temperature) at fixed mass coordinate (Langranian) !dv_dt ! time derivative of velocity at fixed mass coordinate (Langranian) !accel_div_grav ! dv_dt/grav -- only if v_flag is true. 0 otherwise. mass ! m/Msun. mass coordinate of outer boundary of cell. mmid ! mass at midpoint of cell (average of mass coords of the cell boundaries) Msun units. !logM ! log10(m/Msun) !xm ! mass exterior to point (Msun units) !dq ! mass of zone as a fraction of total star mass logxq ! log10(1-q) add_abundances ! this adds all of the isos that are in the current net ! NOTE: you can list specific isotopes by giving their names (from chem_def) !h1 !he3 !he4 !c12 !n14 !o16 ! change in particular abundances during hydro solve !xadot h1 !xadot he3 ! particular abundances before hydro solve !xaprev h1 !xaprev he3 ! ergs/g/sec for reaction categories add_reaction_categories ! this adds all the reaction categories ! NOTE: you can list specific categories by giving their names (from net_def) !pp !cno !tri_alfa ! ergs/g/sec for specific reactions (names from rates_def) !rpp ! misc gradr_sub_grada ! gradr - grada; > 0 => Schwarzschild unstable for convection !dlnR_dm ! for structure equation !dlnP_dm ! for structure equation !dlnT_dm ! for structure equation !dL_dm ! for structure equation !delta_r ! r(outer edge) - r(inner edge); radial extent of cell in cm. !delta_v ! v(inner edge) - v(outer edge); rate at which delta_r is shrinking (cm/sec). !dt_dv_div_dr ! dt*delta_v/delta_r; need to have this << 1 for every cell !cno_div_z ! abundance of c12, n14, and o16 as a fraction of total z !dlog_h1_dlogP ! (log(h1(k)) - log(h1(k-1)))/(log(P(k)) - log(P(k-1))) !dlog_he3_dlogP !dlog_he4_dlogP !dlog_c12_dlogP !dlog_c13_dlogP !dlog_n14_dlogP !dlog_o16_dlogP !dlog_ne20_dlogP !dlog_mg24_dlogP !dlog_si28_dlogP !dlog_pp_dlogP !dlog_cno_dlogP !dlog_3alf_dlogP !dlog_burn_c_dlogP !dlog_burn_n_dlogP !dlog_burn_o_dlogP !dlog_burn_ne_dlogP !dlog_burn_na_dlogP !dlog_burn_mg_dlogP !dlog_cc_dlogP !dlog_co_dlogP !dlog_oo_dlogP !dlog_burn_si_dlogP !dlog_burn_s_dlogP !dlog_burn_ar_dlogP !dlog_burn_ca_dlogP !dlog_burn_ti_dlogP !dlog_burn_cr_dlogP !dlog_burn_fe_dlogP !dlog_pnhe4_dlogP !dlog_photo_dlogP !dlog_other_dlogP !brunt_N2 ! brunt-vaisala frequence squared. only positive values shown. !brunt_Astar ! Astar := r N^2 / g. only positive values shown. !brunt_B ! the composition gradient term in the brunt N^2 calculation !chiY ! dlnP/dlnY used in calculate of brunt_B term !dlnY_dlnP ! the actual dlnY/dlnP in the model as used in brunt_B logQ ! logQ = logRho - 2*logT + 12 !cs_at_cell_bdy ! sound speed at cell boundary (csound is at cell center) !dlnmu_dr ! for salt-finger mixing !semiconvection_criterion ! positive means stable ! 1/chiRho - dlnT_dlnP*chiT/chiRho - dlnRho_dlnP ! the first few lines of the profile contain general info about the model. ! for completeness, those items are described here. ! initial mass and Z ! initial_mass ! initial_z ! general properties of the current state ! model_number ! num_zones ! star_age ! time_step ! properties at the photosphere ! Teff ! photosphere_L ! photosphere_r ! properties at the outermost zone of the model ! log_surface_L ! log_surface_radius ! log_surface_temp ! properties near the center of the model ! log_center_temp ! log_center_density ! log_center_P ! center_eta ! abundances near the center ! center_h1 ! center_he3 ! center_he4 ! center_c12 ! center_n14 ! center_o16 ! center_ne20 ! information about total mass ! star_mass ! star_mdot ! star_mass_h1 ! star_mass_he3 ! star_mass_he4 ! star_mass_c12 ! star_mass_n14 ! star_mass_o16 ! star_mass_ne20 ! locations of abundance transitions ! h1_boundary_mass ! he4_boundary_mass ! c12_boundary_mass ! location of optical depths 10 and 100 ! tau10_mass ! tau10_radius ! tau100_mass ! tau100_radius ! time scales ! dynamic_time ! kh_timescale ! nuc_timescale ! various kinds of total power ! power_nuc_burn ! power_h_burn ! power_he_burn ! power_neu ! a few control parameter values ! h1_boundary_limit ! he4_boundary_limit ! c12_boundary_limit ! burn_min1 ! burn_min2