Parameter List by Number
Number |
Name |
Format |
Unit |
Synopsis |
|---|---|---|---|---|
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|
KEPLER timestep. |
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|
|
Number of zones. |
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|
|
KEPLER timestep used for the previous cycle. |
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|
KEPLER cycle number. |
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|
|
Maximum fractional zonal radius change since the last iteration. |
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|
|
Maximum fractional zonal temperature change since the last iteration. |
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|
|
Number of iterations taken for convergence. |
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|
Time at the beginning of the last timestep. |
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|
|
Total maximum fractional zonal radius change during current cycle. |
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|
Total maximum fractional zonal temperature change during current cycle. |
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|
Maximum fractional zonal luminosity change since the last iteration. |
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|
Total maximum fractional zonal luminosity change since the last iteration. |
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|
|
|
Symbol of the ion most limiting the current KEPLER timestep. |
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|
|
Total number of ions in the APPROX network (usually |
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|
|
|
Number of ion networks specified. |
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|
|
Total number of ions specified in the generator (usually |
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|
|
Current total amount of mass in the problem (incl. summ0 (p 61)). |
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|
Number of nuclear reactions edited (ions only – usually |
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|
|
Total number of iterations since problem generation. |
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|
Zone with largest fractional radius change since the last iteration. |
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Zone with largest fractional temperature change since the last iteration. |
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|
Zone with largest fractional luminosity change since the last iteration. |
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|
|
Current nuclear energy generation rate from last call to subroutine
|
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|
Neutrino deposition coefficient derived from the values of parameters jshell0 (p 93), jshell1 (p 94), and eexplode (p 95) and the current zonal of the star. |
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|
Neutrino luminosity. |
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|
Total initial internal energy. |
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Total initial kinetic energy. |
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Total initial potential energy. |
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|
Total initial energy |
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|
|
|
Total energy deposited so far from input “source”. See xlum0 (p 62). |
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|
Total internal energy. |
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|
|
Total kinetic energy. |
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|
Total potential energy. |
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|
Total current energy |
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|
|
Total net energy produced so far by nuclear reactions less neutrino losses. |
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|
|
Total non-neutrino energy that has so far escaped from the star’s surface. |
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|
|
Energy check. |
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|
|
Rate of energy deposition by input “source”. See xlum0 (p 62). |
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|
|
Rate of change in the total internal energy. |
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|
Rate of change in the total kinetic energy. |
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Rate of change in the total potential energy. |
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|
Rate of change in the total energy. |
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|
Total rate of nuclear energy production less neutrino losses. |
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|
|
|
Total rate of energy escape from the star (in photons). |
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|
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|
Total rate of change in the energy check. |
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|
|
Surface luminosity in electromagnetic radiation ( |
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|
|
|
Photospheric radius corresponding to radius with |
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|
|
|
Effective surface temperature at radius (q 47). |
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|
Current cycle number used by the BURN coprocessor (should be same as ncyc). |
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|
|
Number of cycles since BURN co-processing was initiated (usually = ncyc). |
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|
|
Number of zones co-processed by BURN during current KEPLER cycle. |
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|
|
|
Total number of zones co-processed by BURN since problem generation. |
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|
|
Number of isotopes in the currently specified BURN network (typically |
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|
Number of specified BURN isotopic networks (usually 1). |
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|
Total number of isotopes specified in the BURN generator (typically |
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|
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|
Number of zones at the end of the last KEPLER cycle. |
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Maximum zone number for which BURN co-processing is now being done. |
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|
Length of a BURN co-processing/BURN ion convection subcycle (see nsubcycm (p 264)). |
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Index of the piston position now being used (see :ref:’link’ and |
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|
Total number of piston positions specified in the LINK file (see Link Input File). |
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|
|
Velocity of inner problem boundary due to specified piston (see Link Input File). |
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|
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Core bounce time. Set by the nflux card in the LINK file (see Link Input File). |
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Neutrino flux parameter. Set by the nflux card in the LINK file (see Link Input File). |
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Neutrino flux parameter. Set by the nflux card in the LINK file (see Link Input File). |
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|
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Neutrino flux parameter. Set by the nflux card in the LINK file (see Link Input File). |
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|
|
Neutrino flux parameter. Set by the nflux card in the LINK file (see Link Input File). |
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|
|
Neutrino flux parameter. Set by the nflux card in the LINK file (see Link Input File). |
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|
|
Neutrino flux parameter. Set by the nflux card in the LINK file (see Link Input File). |
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|
|
Neutrino flux parameter. Set by the nflux card in the LINK file (see Link Input File). |
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|
|
Index of the LINK-specified Ye now being utilized (see Link Input File and subroutine |
|
|
|
|
Total number of ye-card-specified |
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Integer index of the next dump time (dump cycle number in subroutine |
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|
Number of distinct mass coordinates used so far in describing zoning ( |
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|
Number of ylib entries (see nylib (q 73)) at the end of the last qq dump cycle. |
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Current number of zonal edit variables to be dumped(see subroutines |
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Location of the next open track in the current ‘qq’ dump file (see subroutine |
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Current number of specified ‘look’ variables (see subroutine |
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|
Initial rotational energy. |
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|
Current rotational energy. |
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|
Initial angular momentum. |
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|
Current total angular momentum. |
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Current mass loss rate. |
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|
Computed metallicity multiplier on mass loss rate. |
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|
Total neutrino energy lost from the star. |
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|
Total energy input by the piston. |
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|
Energy input rate by the piston. |
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|
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Opacity at effective radius. |
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|
Mass lost in the “wind”. |
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|
|
Radius outside of which no convection is allowed. |
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|
|
Number of BURN matrix inversions in last cycle. |
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|
Number of negative abundance backups in subroutine |
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|
Number mass non-conservation backups in subroutine |
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Number of excess abundance change backups in subroutine |
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|
Number if ISE non-convergence backups in subroutine |
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|
|
Rate of change of thermal (“heat”) energy content. |
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|
|
Boundary pressure due to accretion. |
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|
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|
This quantity is for fallback test only. |
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|
Fallback accretion rate. |
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|
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|
Total fallback mass. |
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Cycle of problem generation or last restart. |
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|
Initial central |
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|
Rate of change of rotational energy during last step. |
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|
|
”Time-of-day” seconds of last plot. |
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|
Time/date when problem was generated. |
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|
Time/date when dump was generated. |
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|
Total energy removed from problems by cutsurf. |
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Internal energy removed from problems by cutsurf. |
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Kinetic energy removed from problems by cutsurf. |
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Potential energy removed from problems by cutsurf. |
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|
Rotational energy removed from problems by cutsurf. |
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|
|
Total angular momentum removed from problems by cutsurf. |
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|
|
Total angular momentum lost due to wind. |
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|
Total momentum of inertia of the star. |
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WIMP spin-emph{indepenedent} capture rate. |
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|
WIMP spin-emph{depenedent} capture rate. |
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|
|
|
WIMP annihilation radius scale. |
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|
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|
WIMP capture & annihilation equilibrium time scale. |
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|
|
|
WIMP annihilation rate (two WIMPs annihilate in one annihilation “event”). |
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|
|
|
Total WIMP annihilation luminosity as computed by WIMP subroutine in. |
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WIMP energy deposition rate in star. |
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Total energy deposited in star by WIMP annihilation. |
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|
WIMP annihilation luminosity emph{outside} star. |
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|
Total energy produced by wimps OUTSIDE star by WIMP annihilation. |
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|
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Total amount of mass accreted in. |
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|
Mass accreted in last time step in. |
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Mass losing zone. |
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Accretion zone. |
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Mass lost in last time step in. |
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|
Total mass removed from bottom. |
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|
Total mass removed from bottom and not added to substrate. |
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|
Mass removed in last time step. |
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|
Accretion rate. |
|
|
|
|
Initial |
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|
Initial metallicity. |
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|
Current advection luminosity. |
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|
Volume change due to mass loss. |
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|
Volume change due to mass accretion. |
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|
Volume change due to mass decretion (from bottom). |
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Total viscous energy dissipated. |
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Viscous energy dissipation rate in last time step. |
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|
Total viscous energy dissipation check. |
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|
|
Viscous energy dissipation rate check in last time step. |
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Energy depositied by pulsar. |
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|
Energy deposition rate by pulsar. |
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Energy depositied by |
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|
Energy deposition rate by |
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Total rate of energy deposition by extra heating. |
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|
Total energy deposition by extra heating. |
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|
Maximum zone for which accretion advection luminosity is added. |
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Atmosphere surface boundary pressure resulting from use of isurf (p 523). |
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X-component of current total angular momentum. |
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Y-component of current total angular momentum. |
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Z-component of current total angular momentum. |
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X-component of angular momentum removed from problems by cutsurf. |
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Y-component of angular momentum removed from problems by cutsurf. |
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Z-component of angular momentum removed from problems by cutsurf. |
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X-component of angular momentum lost due to wind. |
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|
Y-component of angular momentum lost due to wind. |
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|
Z-component of angular momentum lost due to wind. |
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|
Current iteration counter for problem termination. |
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Luminosity at effective radius. |
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|
Angular momentum decretion. |
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|
X-angular momentum decretion. |
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|
Y-angular momentum decretion. |
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|
Z-angular momentum decretion. |
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|
|
X-component of initial total angular momentum. |
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|
Y-component of initial total angular momentum. |
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|
Z-component of initial total angular momentum. |
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|
Weighed adiabatic index (gamma1) of star. |
|
|
|
|
Track cycle when mixing was last done. |
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|
|
|
Velocity at effective radius. |
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|
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|
Angular velocity at effective radius. |
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|
Angular velocity in |
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|
Angular velocity in |
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|
Angular velocity in |
enesd).
optical depth.
values in the LINK file (see
decay.
-direction at effective radius.
-direction at effective radius.
-direction at effective radius.