Parameters by Namespace

namespace: cj

util/cj_detonation:

parameter

description

default value

smallx

1.e-10

small_temp

1.e5

small_dens

1.e5

namespace: conductivity

CONDUCTIVITY_DIR=constant:

parameter

description

default value

const_conductivity

constant value of the conductivity, in erg/s/cm/K

1.0e0

CONDUCTIVITY_DIR=constant_opacity:

parameter

description

default value

const_opacity

opacity value, in units of cm**2/g

7.0e-2

CONDUCTIVITY_DIR=powerlaw:

parameter

description

default value

cond_coeff

proportionality constant, C, in k = C T**m

1.0

cond_exponent

temperature exponent, m, in k = C T**m

1.0

namespace: eos

EOS_DIR=breakout:

parameter

description

default value

eos_gamma

0.e0

EOS_DIR=gamma_law:

parameter

description

default value

eos_gamma

ratio of specific heats

5.e0/3.e0

eos_assume_neutral

when computing mu / Abar, do we assume that the composition is atoms or ionized, and therefore include the electron contributions separately?

1

EOS_DIR=helmholtz:

parameter

description

default value

use_eos_coulomb

use the Coulomb corrections

1

eos_input_is_constant

Force the EOS output quantities to match input

1

eos_ttol

Tolerance for iterations with respect to temperature

1.0e-8

eos_dtol

Tolerance for iterations with respect to density

1.0e-8

prad_limiter_rho_c

Density target for radiation pressure smoothing (negative means smoothing is disabled)

-1.0e0

prad_limiter_delta_rho

Density gradient for radiation pressure smoothing (negative means smoothing is disabled)

-1.0e0

EOS_DIR=metal_chem:

parameter

description

default value

eos_gamma_default

1.4

species_1_name

define the specie names, and their masses and gammas

“co_total”

species_1_gamma

5./3.

species_1_mass

0.0

species_2_name

“h2o_total”

species_2_gamma

5./3.

species_2_mass

0.0

species_3_name

“elec”

species_3_gamma

5./3.

species_3_mass

9.10938188e-28

species_4_name

“hp”

species_4_gamma

5./3.

species_4_mass

1.67262158e-24

species_5_name

“h”

species_5_gamma

5./3.

species_5_mass

1.67353251819e-24

species_6_name

“hm”

species_6_gamma

5./3.

species_6_mass

1.67444345638e-24

species_7_name

“dp”

species_7_gamma

5./3.

species_7_mass

3.34512158e-24

species_8_name

“d”

species_8_gamma

5./3.

species_8_mass

3.34603251819e-24

species_9_name

“h2p”

species_9_gamma

1.4

species_9_mass

3.34615409819e-24

species_10_name

“dm”

species_10_gamma

5./3.

species_10_mass

3.34694345638e-24

species_11_name

“h2”

species_11_gamma

1.4

species_11_mass

3.34706503638e-24

species_12_name

“hdp”

species_12_gamma

1.4

species_12_mass

5.01865409819e-24

species_13_name

“hd”

species_13_gamma

1.4

species_13_mass

5.01956503638e-24

species_14_name

“hepp”

species_14_gamma

5./3.

species_14_mass

6.69024316e-24

species_15_name

“hep”

species_15_gamma

5./3.

species_15_mass

6.69115409819e-24

species_16_name

“he”

species_16_gamma

5./3.

species_16_mass

6.69206503638e-24

species_17_name

“cp”

species_17_gamma

5./3.

species_17_mass

2.007528417094e-23

species_18_name

carbon cannot be declared as c because it conflicts with namespace C used for physical constants

“carbon”

species_18_gamma

5./3.

species_18_mass

2.0076195109128e-23

species_19_name

“ch”

species_19_gamma

1.4

species_19_mass

2.1749727627316e-23

species_20_name

“ch2”

species_20_gamma

1.4

species_20_mass

2.3423260145503998e-23

species_21_name

“ch3”

species_21_gamma

1.4

species_21_mass

.5096792663692e-23

species_22_name

“op”

species_22_gamma

5./3.

species_22_mass

2.6767349207316e-23

species_23_name

“o”

species_23_gamma

5./3.

species_23_mass

2.6768260145504e-23

species_24_name

“ch4”

species_24_gamma

1.4

species_24_mass

2.677032518188e-23

species_25_name

“ohp”

species_25_gamma

1.4

species_25_mass

2.8440881725504e-23

species_26_name

“oh”

species_26_gamma

1.4

species_26_mass

2.8441792663692003e-23

species_27_name

“h2op”

species_27_gamma

1.4

species_27_mass

3.0114414243692e-23

species_28_name

“h2o”

species_28_gamma

1.4

species_28_mass

3.011532518188e-23

species_29_name

“h3op”

species_29_gamma

1.4

species_29_mass

3.178794676188e-23

species_30_name

“cop”

species_30_gamma

1.4

species_30_mass

4.6843544316444e-23

species_31_name

“co”

species_31_gamma

1.4

species_31_mass

4.6844455254632e-23

species_32_name

“o2p”

species_32_gamma

1.4

species_32_mass

5.353560935282e-23

species_33_name

“o2”

species_33_gamma

1.4

species_33_mass

5.3536520291008e-23

species_34_name

“co2”

species_34_gamma

1.4

species_34_mass

7.3612715400136e-23

EOS_DIR=multigamma:

parameter

description

default value

eos_gamma_default

default ratio of specific heats used for all components unless specified explicitly as species a, b, or c

1.4

species_a_name

name of species “a”

“”

species_a_gamma

ratio of specific heats for species “a”

1.4

species_b_name

name of species “b”

“”

species_b_gamma

ratio of specific heats for species “b”

1.4

species_c_name

name of species “c”

“”

species_c_gamma

ratio of specific heats for species “c”

1.4

EOS_DIR=polytrope:

parameter

description

default value

polytrope_type

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.

0

polytrope_gamma

density exponent for pressure, P = K rho**gamma

0.0e0

polytrope_K

proportionality constant in EOS, P = K rho**gamma

0.0e0

polytrope_mu_e

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

2.0e0

EOS_DIR=primordial_chem:

parameter

description

default value

eos_gamma_default

1.4

species_1_name

define the specie names, and their masses and gammas

“elec”

species_1_gamma

5./3.

species_1_mass

9.10938188e-28

species_2_name

“hp”

species_2_gamma

5./3.

species_2_mass

1.67262158e-24

species_3_name

“h”

species_3_gamma

5./3.

species_3_mass

1.67353251819e-24

species_4_name

“hm”

species_4_gamma

5./3.

species_4_mass

1.67444345638e-24

species_5_name

“dp”

species_5_gamma

5./3.

species_5_mass

3.34512158e-24

species_6_name

“d”

species_6_gamma

5./3.

species_6_mass

3.34603251819e-24

species_7_name

“h2p”

species_7_gamma

1.4

species_7_mass

3.34615409819e-24

species_8_name

“dm”

species_8_gamma

5./3.

species_8_mass

3.34694345638e-24

species_9_name

“h2”

species_9_gamma

1.4

species_9_mass

3.34706503638e-24

species_10_name

“hdp”

species_10_gamma

1.4

species_10_mass

5.01865409819e-24

species_11_name

“hd”

species_11_gamma

1.4

species_11_mass

5.01956503638e-24

species_12_name

“hepp”

species_12_gamma

5./3.

species_12_mass

6.69024316e-24

species_13_name

“hep”

species_13_gamma

5./3.

species_13_mass

6.69115409819e-24

species_14_name

“he”

species_14_gamma

5./3.

species_14_mass

6.69206503638e-24

EOS_DIR=rad_power_law:

parameter

description

default value

eos_const_c_v

specific heat proportionality constant, K, c_v = K rho**m T**(-n)

-1.e0

eos_c_v_exp_m

specific heat density exponent, m, c_v = K rho**m T**(-n)

0.e0

eos_c_v_exp_n

specific heat (negative) temperature exponent, n, c_v = K rho**m T**(-n)

0.e0

EOS_DIR=tillotson:

parameter

description

default value

eos_la

0.5

eos_lb

1.3

eos_e_0

minimum energy

1.6e11

eos_rho_0

reference density

2.7

eos_A

1.8e11

eos_B

1.8e11

eos_e_s

3.5e10

eos_e_s_prime

1.8e11

eos_alpha

5.0

eos_beta

5.0

eos_c_v

specific heat

7.9e6

namespace: integrator

parameter

description

default value

call_eos_in_rhs

Normally we update the temperature during a burn to be consistent with the current internal energy. This is done with an EOS call, which can be turned off if desired. This will freeze the temperature and specific heat to the values at the beginning of the burn, which is inaccurate but cheaper.

1

integrate_energy

Allow the energy integration to be disabled by setting the RHS to zero.

1

jacobian

Whether to use an analytical or numerical Jacobian. 1 == Analytical 2 == Numerical

1

burner_verbose

Should we print out diagnostic output after the solve?

0

rtol_spec

relative tolerance for species

1.e-12

rtol_enuc

relative tolerance for energy

1.e-6

atol_spec

absolute tolerance for species

1.e-8

atol_enuc

absolute tolerance for energy

1.e-6

renormalize_abundances

Whether to renormalize the mass fractions at each step in the evolution so that they sum to unity.

0

SMALL_X_SAFE

The absolute cutoff for species – note that this might be larger than small_x, but the issue is that we need to prevent underflow issues and keep mass fractions positive in the integrator. You may have to increase the floor to, e.g. 1.e-20 if your rates are large.

1.0e-30

MAX_TEMP

The maximum temperature for reactions in the integration.

1.0e11

react_boost

boost the reaction rates by a factor > 1

-1.e0

ode_max_steps

maximum number of timesteps for the integrator

150000

ode_max_dt

maximum timestep for the integrator

1.e30

use_jacobian_caching

Whether to use Jacobian caching in VODE

1

nonaka_i

Inputs for generating a Nonaka Plot (TM)

0

nonaka_j

0

nonaka_k

0

nonaka_level

0

nonaka_file

“nonaka_plot.dat”

use_burn_retry

do we retry a failed burn with different parameters?

0

retry_swap_jacobian

do we swap the Jacobian (from analytic to numerical or vice versa) on a retry?

1

retry_rtol_spec

relative tolerance for species on retry

-1

retry_rtol_enuc

relative tolerance for energy on retry

-1

retry_atol_spec

absolute tolerance for species on retry

-1

retry_atol_enuc

absolute tolerance for energy on retry

-1

do_species_clip

in the clean_state process, do we clip the species such that they are in [0, 1]?

1

use_number_densities

flag for turning on the use of number densities for all species

0

subtract_internal_energy

flag for tuning on the subtraction of internal energy

1

scale_system

do we scale the ODE system we integrate to make it O(1)? for Strang, this simply means scaling e by the initial energy?

0

nse_deriv_dt_factor

for SDC+NSE, when estimating the derivatives of the NSE table quantities, what fraction of dt do we use for the finite-difference estimate

0.05

nse_include_enu_weak

for NSE update, do we include the weak rate neutrino losses?

1

linalg_do_pivoting

for the linear algebra, do we allow pivoting?

1

INTEGRATOR_DIR=BackwardEuler:

parameter

description

default value

max_iter

Maximum number of iterations for the Newton solve

25

tol

tolerance for the Newton solve

1.e-10

do_single_step

toggle single-step BackwardEuler integration and ignoring error tolerance

0

INTEGRATOR_DIR=ForwardEuler:

parameter

description

default value

maximum_timestep_change_factor

Maximum amount any quantity can change by in a timestep

1.001

INTEGRATOR_DIR=QSS:

parameter

description

default value

predictor_corrector_tolerance

Allowable difference between the predictor and corrector

0.01

tolerance_safety_factor

Threshold factor on the error criterion used in timestep selection

10.0

num_timestep_iters

Maximum number of iterations on the timestep constraint loop

10

num_corrector_iters

Maximum number of iterations on the corrector loop

1

dt_max_change_factor

Maximum factor that dt is allowed to grow per timestep

1.05

dt_cut_factor

Multiply the timestep by this factor when we outright reject it

0.5

species_tolerance

Reject a species update if X < -tol or X > 1.0 + tol

0.01

dt_init_fraction

Scale factor for initial timestep

0.01

INTEGRATOR_DIR=RKC:

parameter

description

default value

scale_system

do we scale the ODE system we integrate to make it O(1)? for Strang, this simply means scaling e by the initial energy?

1

use_circle_theorem

use the Gershgorin circle theorem to estimate the spectral radius? note: requires integrator.scale_system = 1

1

INTEGRATOR_DIR=VODE:

parameter

description

default value

X_reject_buffer

for the step rejection logic on mass fractions, we only consider species that are > X_reject_buffer * atol_spec

1.0

NETWORK_DIR=rprox:

parameter

description

default value

atol_spec

override the default tolerances for backwards compatibility

1.0e-11

rtol_spec

1.0e-12

atol_enuc

1.0e-8

rtol_enuc

1.0e-8

jacobian

override so that the default is an analytical Jacobian

1

NETWORK_DIR=triple_alpha_plus_cago:

parameter

description

default value

atol_spec

override the default tolerances for backwards compatibility

1.0e-12

rtol_spec

1.0e-12

atol_enuc

1.0e-8

rtol_enuc

1.0e-6

jacobian

override so that the default is an analytical Jacobian

1

namespace: network

parameter

description

default value

rho_nse

density above which to assume we are in NSE

3.e8

T_nse

temperature above which to assume we are in NSE

3.e9

C_nse

upper-limit for C + N mass fraction required for NSE

0.01

O_nse

upper-limit for O mass fraction required for NSE

0.01

Si_nse

upper-limit for Si mass fraction required for NSE

0.01

He_Fe_nse

lower-limit for the He + iron-group mass fraction required for NSE

0.88

T_always_nse

temperature above which we always assume NSE, regardless of composition note: rho_nse is still considered.

9.e9

nse_relax_factor

factor (< 1) by which to relax the criteria for entering NSE. This is only applied after a failed burn.

1.0

nse_table_interp_linear

do we do tri-linear or tri-cubic interpolation on the table?

0

small_x

cutoff for species mass fractions

1.e-30

use_tables

Should we use rate tables if they are present in the network?

0

use_c12ag_deboer17

Should we use Deboer + 2017 rate for c12(a,g)o16?

0

NETWORK_DIR=he-burn/ase:

parameter

description

default value

disable_p_C12_to_N13

0

disable_He4_N13_to_p_O16

0

NETWORK_DIR=he-burn/he-burn-19am:

parameter

description

default value

disable_p_C12_to_N13

0

disable_He4_N13_to_p_O16

0

NETWORK_DIR=metal_chem:

parameter

description

default value

small_x

cutoff for species mass fractions

1.e-100

redshift

redshift for metal chem (Pop II/I star formation)

0e0

metallicity

metallicity for metal chem (Pop II/I star formation)

1e0

dust2gas_ratio

dust to gas ratio relative to solar

1e0

crate

Cosmic ray ionization rate (per s)

0e0

Av

Av

0e0

ionH

H ionization rate (per s)

0e0

ionH2

H2 ionization rate (per s)

0e0

dissH2

H2 dissociation rate (per s)

0e0

ionC

C ionization rate (per s)

0e0

ionO

O ionization rate (per s)

0e0

dissCO

CO dissociation rate (per s)

0e0

NETWORK_DIR=powerlaw:

parameter

description

default value

rtilde

the coefficient for the reaction rate

1.e0

nu

exponent for the temperature

4.e0

specific_q_burn

reaction specific q-value (in erg/g)

10.e0

T_burn_ref

reaction thresholds (for the power law)

1.0e0

rho_burn_ref

1.0e0

f_act

1.0e0

NETWORK_DIR=primordial_chem:

parameter

description

default value

small_x

cutoff for species mass fractions

1.e-100

redshift

assumed redshift for primordial chem (Pop III star formation)

30e0

namespace: neutrino_cooling

parameter

description

default value

include_recomb

0

namespace: nse

parameter

description

default value

max_nse_iters

max iterations for NSE Newton-Raphson Solver

500

use_hybrid_solver

Choose NSE solver. 1 == hybrid powell 0 == Newton- Raphson

1

solve_nse_e_mode

Different modes for solving (rho, e, Ye) input 1 == Solve for (rho, T, Ye), then do iteration to find e. 2 == Solve for e altogether with mu_p and mu_n.

1

ase_tol

Tolerance used in the NSE-Grouping process

0.1

nse_abs_tol

Tolerances for molar fraction comparison

0.005

nse_rel_tol

0.2

nse_dx_independent

Whether NSE depends on the size of the cell. This is the requirement that the reaction timescale must be smaller than the sound crossing time 1 == independent 0 == dependent

0

nse_molar_independent

Whether to use NSE mass fractions for NSE grouping This makes NSE Grouping process solely dependent on the thermodynamic condition

0

nse_skip_molar

Whether the initial molar fraction check is skipped when integration failed.

0

T_nse_net

Set this to a positive number to make use simple temperature threshold of determining NSE after the initial molar fraction check.

-1.0

T_min_nse

Minimum Temperature required for NSE

4.0e9

namespace: opacity

OPACITY_DIR=rad_power_law:

parameter

description

default value

const_kappa_p

Opacity constant (Planck)

-1.0e0

kappa_p_exp_m

Density exponent (Planck)

0.0e0

kappa_p_exp_n

Temperature exponent (Planck)

0.0e0

kappa_p_exp_p

Frequency exponent (Planck)

0.0e0

const_kappa_r

Opacity constant (Rosseland)

-1.0e0

kappa_r_exp_m

Density exponent (Rosseland)

0.0e0

kappa_r_exp_n

Temperature exponent (Rosseland)

0.0e0

kappa_r_exp_p

Frequency exponent (Rosseland)

0.0e0

const_scatter

Opacity constant (scattering)

0.0e0

scatter_exp_m

Density exponent (scattering)

0.0e0

scatter_exp_n

Temperature exponent (scattering)

0.0e0

scatter_exp_p

Frequency exponent (scattering)

0.0e0

kappa_floor

Opacity floor

0.0e0

rad_temp_floor

Temperature floor

1.e-10

namespace: screening

parameter

description

default value

enable_chabrier1998_quantum_corr

0

enable_debye_huckel_skip

0

debye_huckel_skip_threshold

1.01e0

namespace: unit_test

parameter

description

default value

primary_species_1

“”

primary_species_2

“”

primary_species_3

“”

X1

1.0e0

X2

0.0e0

X3

0.0e0

X4

0.0e0

X5

0.0e0

X6

0.0e0

X7

0.0e0

X8

0.0e0

X9

0.0e0

X10

0.0e0

X11

0.0e0

X12

0.0e0

X13

0.0e0

X14

0.0e0

X15

0.0e0

X16

0.0e0

X17

0.0e0

X18

0.0e0

X19

0.0e0

X20

0.0e0

X21

0.0e0

X22

0.0e0

X23

0.0e0

X24

0.0e0

X25

0.0e0

X26

0.0e0

X27

0.0e0

X28

0.0e0

X29

0.0e0

X30

0.0e0

X31

0.0e0

X32

0.0e0

X33

0.0e0

X34

0.0e0

X35

0.0e0

X36

0.0e0

X37

0.0e0

X38

0.0e0

X39

0.0e0

X40

0.0e0

X41

0.0e0

X42

0.0e0

X43

0.0e0

X44

0.0e0

X45

0.0e0

X46

0.0e0

X47

0.0e0

X48

0.0e0

X49

0.0e0

X50

0.0e0

X51

0.0e0

X52

0.0e0

X53

0.0e0

X54

0.0e0

X55

0.0e0

X56

0.0e0

X57

0.0e0

X58

0.0e0

X59

0.0e0

X60

0.0e0

X61

0.0e0

X62

0.0e0

X63

0.0e0

X64

0.0e0

X65

0.0e0

X66

0.0e0

X67

0.0e0

X68

0.0e0

X69

0.0e0

X70

0.0e0

X71

0.0e0

X72

0.0e0

X73

0.0e0

X74

0.0e0

X75

0.0e0

X76

0.0e0

X77

0.0e0

X78

0.0e0

X79

0.0e0

X80

0.0e0

X81

0.0e0

X82

0.0e0

X83

0.0e0

X84

0.0e0

X85

0.0e0

X86

0.0e0

X87

0.0e0

X88

0.0e0

X89

0.0e0

X90

0.0e0

X91

0.0e0

X92

0.0e0

X93

0.0e0

X94

0.0e0

X95

0.0e0

X96

0.0e0

X97

0.0e0

X98

0.0e0

X99

0.0e0

X100

0.0e0

X101

0.0e0

X102

0.0e0

X103

0.0e0

X104

0.0e0

X105

0.0e0

X106

0.0e0

X107

0.0e0

X108

0.0e0

X109

0.0e0

X110

0.0e0

X111

0.0e0

X112

0.0e0

X113

0.0e0

X114

0.0e0

X115

0.0e0

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0.0e0

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0.0e0

X118

0.0e0

X119

0.0e0

X120

0.0e0

X121

0.0e0

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0.0e0

X123

0.0e0

X124

0.0e0

X125

0.0e0

X126

0.0e0

X127

0.0e0

X128

0.0e0

X129

0.0e0

X130

0.0e0

X131

0.0e0

X132

0.0e0

X133

0.0e0

X134

0.0e0

X135

0.0e0

X136

0.0e0

X137

0.0e0

X138

0.0e0

X139

0.0e0

X140

0.0e0

X141

0.0e0

X142

0.0e0

X143

0.0e0

X144

0.0e0

X145

0.0e0

X146

0.0e0

X147

0.0e0

X148

0.0e0

X149

0.0e0

X150

0.0e0

X151

0.0e0

X152

0.0e0

X153

0.0e0

X154

0.0e0

X155

0.0e0

X156

0.0e0

X157

0.0e0

X158

0.0e0

X159

0.0e0

X160

0.0e0

X161

0.0e0

X162

0.0e0

X163

0.0e0

X164

0.0e0

X165

0.0e0

X166

0.0e0

X167

0.0e0

X168

0.0e0

X169

0.0e0

X170

0.0e0

X171

0.0e0

X172

0.0e0

X173

0.0e0

X174

0.0e0

X175

0.0e0

X176

0.0e0

X177

0.0e0

X178

0.0e0

X179

0.0e0

X180

0.0e0

X181

0.0e0

X182

0.0e0

X183

0.0e0

X184

0.0e0

X185

0.0e0

X186

0.0e0

X187

0.0e0

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0.0e0

X189

0.0e0

X190

0.0e0

X191

0.0e0

X192

0.0e0

X193

0.0e0

X194

0.0e0

X195

0.0e0

X196

0.0e0

X197

0.0e0

X198

0.0e0

X199

0.0e0

X200

0.0e0

X201

0.0e0

X202

0.0e0

X203

0.0e0

X204

0.0e0

X205

0.0e0

X206

0.0e0

X207

0.0e0

X208

0.0e0

X209

0.0e0

X210

0.0e0

X211

0.0e0

X212

0.0e0

X213

0.0e0

X214

0.0e0

X215

0.0e0

X216

0.0e0

X217

0.0e0

X218

0.0e0

X219

0.0e0

X220

0.0e0

X221

0.0e0

X222

0.0e0

X223

0.0e0

X224

0.0e0

X225

0.0e0

X226

0.0e0

X227

0.0e0

X228

0.0e0

X229

0.0e0

X230

0.0e0

X231

0.0e0

X232

0.0e0

X233

0.0e0

X234

0.0e0

X235

0.0e0

X236

0.0e0

X237

0.0e0

X238

0.0e0

X239

0.0e0

X240

0.0e0

X241

0.0e0

X242

0.0e0

X243

0.0e0

X244

0.0e0

X245

0.0e0

X246

0.0e0

X247

0.0e0

X248

0.0e0

X249

0.0e0

X250

0.0e0

X251

0.0e0

X252

0.0e0

X253

0.0e0

X254

0.0e0

X255

0.0e0

X256

0.0e0

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0.0e0

X258

0.0e0

X259

0.0e0

X260

0.0e0

X261

0.0e0

X262

0.0e0

X263

0.0e0

X264

0.0e0

X265

0.0e0

X266

0.0e0

X267

0.0e0

X268

0.0e0

X269

0.0e0

X270

0.0e0

X271

0.0e0

X272

0.0e0

X273

0.0e0

X274

0.0e0

X275

0.0e0

X276

0.0e0

X277

0.0e0

X278

0.0e0

X279

0.0e0

X280

0.0e0

X281

0.0e0

X282

0.0e0

X283

0.0e0

X284

0.0e0

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0.0e0

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0.0e0

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0.0e0

X288

0.0e0

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0.0e0

X290

0.0e0

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0.0e0

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0.0e0

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0.0e0

X294

0.0e0

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0.0e0

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0.0e0

X297

0.0e0

X298

0.0e0

X299

0.0e0

X300

0.0e0

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0.0e0

X302

0.0e0

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0.0e0

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0.0e0

X305

0.0e0

X306

0.0e0

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0.0e0

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0.0e0

X309

0.0e0

X310

0.0e0

X311

0.0e0

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0.0e0

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0.0e0

X314

0.0e0

X315

0.0e0

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0.0e0

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0.0e0

X318

0.0e0

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0.0e0

X320

0.0e0

X321

0.0e0

X322

0.0e0

X323

0.0e0

X324

0.0e0

X325

0.0e0

X326

0.0e0

X327

0.0e0

X328

0.0e0

X329

0.0e0

X330

0.0e0

X331

0.0e0

X332

0.0e0

X333

0.0e0

X334

0.0e0

X335

0.0e0

X336

0.0e0

X337

0.0e0

X338

0.0e0

X339

0.0e0

X340

0.0e0

X341

0.0e0

X342

0.0e0

X343

0.0e0

X344

0.0e0

X345

0.0e0

X346

0.0e0

X347

0.0e0

X348

0.0e0

X349

0.0e0

X350

0.0e0

X351

0.0e0

X352

0.0e0

X353

0.0e0

X354

0.0e0

X355

0.0e0

X356

0.0e0

X357

0.0e0

X358

0.0e0

X359

0.0e0

X360

0.0e0

X361

0.0e0

X362

0.0e0

X363

0.0e0

X364

0.0e0

X365

0.0e0

X366

0.0e0

X367

0.0e0

X368

0.0e0

X369

0.0e0

X370

0.0e0

X371

0.0e0

X372

0.0e0

X373

0.0e0

X374

0.0e0

X375

0.0e0

X376

0.0e0

X377

0.0e0

X378

0.0e0

X379

0.0e0

X380

0.0e0

X381

0.0e0

X382

0.0e0

X383

0.0e0

X384

0.0e0

X385

0.0e0

X386

0.0e0

X387

0.0e0

X388

0.0e0

X389

0.0e0

X390

0.0e0

X391

0.0e0

X392

0.0e0

X393

0.0e0

X394

0.0e0

X395

0.0e0

X396

0.0e0

X397

0.0e0

X398

0.0e0

X399

0.0e0

X400

0.0e0

uniform_xn

do we set all of the mass fractions equal (to 1/NumSpec)?

0

small_temp

lowest temperature allowed in the EOS

1.e5

small_dens

lowest density allowed in the EOS

1.e5

nse_solver/make_table:

parameter

description

default value

rho_min

1.e6

rho_max

1.e10

nrho

5

T_min

1.e9

T_max

1.e10

nT

5

Ye_min

0.4

Ye_max

0.7

nye

7

nse_solver/nse_compatibility:

parameter

description

default value

run_prefix

“”

tmax

the final time to integrate to

1.e-1

tfirst

first output time – we will output in nsteps logarithmically spaced steps between [tfirst, tmax]

0.0

nsteps

number of steps (logarithmically spaced)

100

rho

density

1.e7

T

temperature

6.e9

mu_p

Initial guess for proton chemical potential

-3.0

mu_n

Initial guess for neutron chemical potential

-12.0

unit_test/burn_cell:

parameter

description

default value

tmax

the final time to integrate to

1.e-2

tfirst

first output time – we will output in nsteps logarithmically spaced steps between [tfirst, tmax]

0.0

nsteps

number of steps (logarithmically spaced)

100

density

1.e7

temperature

3.e9

skip_initial_normalization

0

unit_test/burn_cell_metal_chem:

parameter

description

default value

run_prefix

“burn_cell_metal_chem”

small_temp

floor values of temperature and density

1.e1

small_dens

1.e-30

tmax

the final time to integrate to

1.e20

tff_reduc

tff_reduc reduces the calculated freefall time to accordingly increase the density during the single zone burn

1.e-1

tfirst

first output time – we will output in nsteps logarithmically spaced steps between [tfirst, tmax]

0.0

nsteps

number of steps for the single zone burn

1000

ninit

initial number density and temperature

1e-1

temperature

1e2

primary_species_1

list of species and their number densities used in the network (39 if including deuterium)

1.0e0

primary_species_2

0.0e0

primary_species_3

0.0e0

primary_species_4

0.0e0

primary_species_5

0.0e0

primary_species_6

0.0e0

primary_species_7

0.0e0

primary_species_8

0.0e0

primary_species_9

0.0e0

primary_species_10

0.0e0

primary_species_11

0.0e0

primary_species_12

0.0e0

primary_species_13

0.0e0

primary_species_14

0.0e0

primary_species_15

0.0e0

primary_species_16

0.0e0

primary_species_17

0.0e0

primary_species_18

0.0e0

primary_species_19

0.0e0

primary_species_20

0.0e0

primary_species_21

0.0e0

primary_species_22

0.0e0

primary_species_23

0.0e0

primary_species_24

0.0e0

primary_species_25

0.0e0

primary_species_26

0.0e0

primary_species_27

0.0e0

primary_species_28

0.0e0

primary_species_29

0.0e0

primary_species_30

0.0e0

primary_species_31

0.0e0

primary_species_32

0.0e0

primary_species_33

0.0e0

primary_species_34

0.0e0

unit_test/burn_cell_primordial_chem:

parameter

description

default value

run_prefix

“burn_cell_primordial_chem”

small_temp

floor values of temperature and density

1.e1

small_dens

1.e-30

tmax

the final time to integrate to

1.e20

tff_reduc

tff_reduc reduces the calculated freefall time to accordingly increase the density during the single zone burn

1.e-1

tfirst

first output time – we will output in nsteps logarithmically spaced steps between [tfirst, tmax]

0.0

nsteps

number of steps for the single zone burn

1000

temperature

initial temperature

1e2

primary_species_1

list of species and their number densities used in the network (14 if including deuterium)

1.0e0

primary_species_2

0.0e0

primary_species_3

0.0e0

primary_species_4

0.0e0

primary_species_5

0.0e0

primary_species_6

0.0e0

primary_species_7

0.0e0

primary_species_8

0.0e0

primary_species_9

0.0e0

primary_species_10

0.0e0

primary_species_11

0.0e0

primary_species_12

0.0e0

primary_species_13

0.0e0

primary_species_14

0.0e0

unit_test/burn_cell_sdc:

parameter

description

default value

tmax

the final time to integrate to

1.e-2

tfirst

first output time – we will output in nsteps logarithmically spaced steps between [tfirst, tmax]

0.0

nsteps

number of steps (logarithmically spaced)

100

recompute_aux

do we recompute the aux quantities? or do we take them as given in the inputs?

0

density

1.e7

temperature

3.e9

rhoe

-1.e0

Aux1

0.0e0

Aux2

0.0e0

Aux3

0.0e0

Adv_rho

0.0e0

Adv_rhoe

0.0e0

Adv_X1

0.0e0

Adv_X2

0.0e0

Adv_X3

0.0e0

Adv_X4

0.0e0

Adv_X5

0.0e0

Adv_X6

0.0e0

Adv_X7

0.0e0

Adv_X8

0.0e0

Adv_X9

0.0e0

Adv_X10

0.0e0

Adv_X11

0.0e0

Adv_X12

0.0e0

Adv_X13

0.0e0

Adv_X14

0.0e0

Adv_X15

0.0e0

Adv_X16

0.0e0

Adv_X17

0.0e0

Adv_X18

0.0e0

Adv_X19

0.0e0

Adv_X20

0.0e0

Adv_X21

0.0e0

Adv_X22

0.0e0

Adv_X23

0.0e0

Adv_X24

0.0e0

Adv_X25

0.0e0

Adv_X26

0.0e0

Adv_X27

0.0e0

Adv_X28

0.0e0

Adv_X29

0.0e0

Adv_X30

0.0e0

Adv_X31

0.0e0

Adv_X32

0.0e0

Adv_X33

0.0e0

Adv_X34

0.0e0

Adv_X35

0.0e0

Adv_Aux1

0.0e0

Adv_Aux2

0.0e0

Adv_Aux3

0.0e0

mu_p

-5.0

mu_n

-12.0

unit_test/eos_cell:

parameter

description

default value

density

1.e7

temperature

3.e9

unit_test/jac_cell:

parameter

description

default value

density

1.e7

temperature

3.e9

skip_initial_normalization

0

unit_test/nse_net_cell:

parameter

description

default value

run_prefix

“”

density

1.e7

temperature

3.e9

ye

0.75

mu_p

-3.0

mu_n

-12.0

unit_test/nse_net_cell/make_table:

parameter

description

default value

rho_min

1.e6

rho_max

1.e10

nrho

5

T_min

4.0e9

T_max

1.e10

nT

10

Ye_min

0.49

Ye_max

0.7

nye

7

unit_test/nse_table_cell:

parameter

description

default value

density

1.23e9

temperature

5.18e9

ye

0.472

unit_test/part_func_cell:

parameter

description

default value

temperature

5.e9

unit_test/test_aprox_rates:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e12

metalicity_max

0.1e0

unit_test/test_conductivity:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e12

metalicity_max

0.1e0

unit_test/test_eos:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e12

unit_test/test_jac:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e15

uniform_xn

0

tmax

0.1e0

unit_test/test_neutrino_cooling:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e12

metalicity_max

0.1e0

unit_test/test_nse_interp:

parameter

description

default value

density

1.23e9

temperature

5.18e9

ye

0.472

unit_test/test_parameters:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e12

test_string

“test”

unit_test/test_react:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e15

tmax

0.1e0

unit_test/test_rhs:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e15

unit_test/test_screening_templated:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e12

metalicity_max

0.1e0

loops

1

unit_test/test_sdc:

parameter

description

default value

dens_min

1.e6

dens_max

1.e9

temp_min

1.e6

temp_max

1.e15

tmax

0.1e0

unit_test/test_sdc_vode_rhs:

parameter

description

default value

density

1.e7

temperature

3.e9

tmax

1.e-7

Aux1

0.0e0

Aux2

0.0e0

Aux3

0.0e0

Adv_rho

0.0e0

Adv_rhoe

0.0e0

Adv_X1

0.0e0

Adv_X2

0.0e0

Adv_X3

0.0e0

Adv_X4

0.0e0

Adv_X5

0.0e0

Adv_X6

0.0e0

Adv_X7

0.0e0

Adv_X8

0.0e0

Adv_X9

0.0e0

Adv_X10

0.0e0

Adv_X11

0.0e0

Adv_X12

0.0e0

Adv_X13

0.0e0

Adv_X14

0.0e0

Adv_X15

0.0e0

Adv_X16

0.0e0

Adv_X17

0.0e0

Adv_X18

0.0e0

Adv_X19

0.0e0

Adv_X20

0.0e0

Adv_X21

0.0e0

Adv_X22

0.0e0

Adv_X23

0.0e0

Adv_X24

0.0e0

Adv_X25

0.0e0

Adv_X26

0.0e0

Adv_X27

0.0e0

Adv_X28

0.0e0

Adv_X29

0.0e0

Adv_X30

0.0e0

Adv_Aux1

0.0e0

Adv_Aux2

0.0e0

Adv_Aux3

0.0e0