diff --git a/EOS/gamma_law/_parameters b/EOS/gamma_law/_parameters index 0b90daa7a8..70338bec79 100644 --- a/EOS/gamma_law/_parameters +++ b/EOS/gamma_law/_parameters @@ -1,4 +1,9 @@ @namespace: eos +# ratio of specific heats eos_gamma real 5.e0/3.e0 -eos_assume_neutral bool 1 + +# when computing mu / Abar, do we assume that the composition is atoms +# or ionized, and therefore include the electron contributions +# separately? +eos_assume_neutral bool 1 diff --git a/EOS/multigamma/_parameters b/EOS/multigamma/_parameters index 9176e98c2b..bda6bf2344 100644 --- a/EOS/multigamma/_parameters +++ b/EOS/multigamma/_parameters @@ -1,14 +1,25 @@ @namespace: eos +# default ratio of specific heats used for all components unless specified +# explicitly as species a, b, or c eos_gamma_default real 1.4 +# name of species "a" species_a_name string "" + +# ratio of specific heats for species "a" species_a_gamma real 1.4 +# name of species "b" species_b_name string "" + +# ratio of specific heats for species "b" species_b_gamma real 1.4 +# name of species "c" species_c_name string "" + +# ratio of specific heats for species "c" species_c_gamma real 1.4 diff --git a/EOS/polytrope/_parameters b/EOS/polytrope/_parameters index 449d87245e..122594afa8 100644 --- a/EOS/polytrope/_parameters +++ b/EOS/polytrope/_parameters @@ -1,7 +1,17 @@ @namespace: eos +# polytrope type: 1 is non-relativistic, fully degenerate electron +# gas; 2 is fully-relativistic, fully degenerate gas. If these are +# set, then only pulytrope_mu_e needs to be set. polytrope_type int 0 + +# density exponent for pressure, P = K rho**gamma polytrope_gamma real 0.0e0 + +# proportionality constant in EOS, P = K rho**gamma polytrope_K real 0.0e0 + +# mean molecular weight per electron for the cases when polytrope_type +# is 1 or 2. In that case, we have P = K (rho / mu_e)**gamma polytrope_mu_e real 2.0e0 diff --git a/EOS/rad_power_law/_parameters b/EOS/rad_power_law/_parameters index fe4681225e..ed61e9bdb7 100644 --- a/EOS/rad_power_law/_parameters +++ b/EOS/rad_power_law/_parameters @@ -1,5 +1,10 @@ @namespace: eos +# specific heat proportionality constant, K, c_v = K rho**m T**(-n) eos_const_c_v real -1.e0 + +# specific heat density exponent, m, c_v = K rho**m T**(-n) eos_c_v_exp_m real 0.e0 + +# specific heat (negative) temperature exponent, n, c_v = K rho**m T**(-n) eos_c_v_exp_n real 0.e0 diff --git a/EOS/tillotson/_parameters b/EOS/tillotson/_parameters index 5931e33d16..6e25b1744f 100644 --- a/EOS/tillotson/_parameters +++ b/EOS/tillotson/_parameters @@ -1,13 +1,27 @@ -@namespace: eos + @namespace: eos eos_la real 0.5 + eos_lb real 1.3 + +# minimum energy eos_e_0 real 1.6e11 + +# reference density eos_rho_0 real 2.7 + + eos_A real 1.8e11 + eos_B real 1.8e11 + eos_e_s real 3.5e10 + eos_e_s_prime real 1.8e11 + eos_alpha real 5.0 + eos_beta real 5.0 + +# specific heat eos_c_v real 7.9e6 diff --git a/conductivity/constant/_parameters b/conductivity/constant/_parameters index 3982bc86cc..01c83e233a 100644 --- a/conductivity/constant/_parameters +++ b/conductivity/constant/_parameters @@ -1,5 +1,6 @@ @namespace: conductivity +# constant value of the conductivity, in erg/s/cm/K const_conductivity real 1.0e0 diff --git a/conductivity/constant_opacity/_parameters b/conductivity/constant_opacity/_parameters index 5740b675ee..4d7bd58120 100644 --- a/conductivity/constant_opacity/_parameters +++ b/conductivity/constant_opacity/_parameters @@ -1,5 +1,6 @@ @namespace: conductivity +# opacity value, in units of cm**2/g const_opacity real 7.0e-2 diff --git a/conductivity/powerlaw/_parameters b/conductivity/powerlaw/_parameters index 7d46bc80d4..60e03e2d33 100644 --- a/conductivity/powerlaw/_parameters +++ b/conductivity/powerlaw/_parameters @@ -1,6 +1,9 @@ @namespace: conductivity +# proportionality constant, C, in k = C T**m cond_coeff real 1.0 + +# temperature exponent, m, in k = C T**m cond_exponent real 1.0 diff --git a/integration/_parameters b/integration/_parameters index eac2654ab9..a11b5f3ea8 100644 --- a/integration/_parameters +++ b/integration/_parameters @@ -21,10 +21,17 @@ burner_verbose bool 0 # Tolerances for the solver (relative and absolute), for the # species and energy equations. + +# relative tolerance for species rtol_spec real 1.e-12 + +# relative tolerance for energy rtol_enuc real 1.e-6 +# absolute tolerance for species atol_spec real 1.e-8 + +# absolute tolerance for energy atol_enuc real 1.e-6 # Whether to renormalize the mass fractions at each step in the evolution @@ -69,10 +76,17 @@ retry_swap_jacobian bool 1 # Tolerances for the solver (relative and absolute), for the # species and energy equations. If set to < 0, then the same # value as the first attempt is used. + +# relative tolerance for species on retry retry_rtol_spec real -1 + +# relative tolerance for energy on retry retry_rtol_enuc real -1 +# absolute tolerance for species on retry retry_atol_spec real -1 + +# absolute tolerance for energy on retry retry_atol_enuc real -1 # in the clean_state process, do we clip the species such that they diff --git a/networks/primordial_chem/_parameters b/networks/primordial_chem/_parameters index c70b4eaf2c..d272dbbb38 100644 --- a/networks/primordial_chem/_parameters +++ b/networks/primordial_chem/_parameters @@ -3,5 +3,6 @@ # cutoff for species mass fractions small_x real 1.e-100 + # assumed redshift for primordial chem (Pop III star formation) redshift real 30e0