Grids of Stellar Evolution Models Presupernova Structure of
Magnetic Rotating Stars
Data from Heger, Woosley, & Spruit (2005)
Version 6 -- Sun Sep 26 04:14:16 UTC 2004
Hydro / EOS data explanation
column |
data |
unit |
grid |
cell number |
--- |
cell outer total mass |
mass coordinate at the cell top interface |
g |
cell outer radius |
radius coordinate at the cell top interface |
cm |
cell outer velocity |
velocity of the cell top interface |
cm s-1 |
cell density |
average density of the cell |
g cm-3 |
cell temperature |
average temperature of the cell |
K |
cell pressure |
average pressure of the cell |
dyn cm-2 |
cell specific energy |
average specific energy of the cell |
erg g-1 |
cell specific entropy |
average specific entropy of cell |
kB baryon-1 |
cell angular velocity |
average angular velocity of the cell |
rad s-1 |
cell A_bar |
average mean mass number of nuclei in the cell |
1 |
cell Y_e |
average electrons per baryon in the cell |
1 |
stability |
hydrodynamic stability of outer cell boundary |
--- |
B_r |
poloidal magnetic field at outer cell boundary |
Gauss |
B_phi |
azimuthal magnetic field at outer cell boundary |
Gauss |
Network data explanation
APPROX : |
approximative 19 isotope network |
QSE : |
Quasi Statitstical Equilibrium isotopes treated in three NSE subgroups
which are connected by "bottleneck" reactions 137 isotope network for weak rates |
NSE : |
Nuclear Statistical Equilibrium 137 isotope network for weak rates |
column |
network |
unit |
APPROX |
QSE / NSE |
neutrons |
neutrons |
neutrons |
(mass fraction) |
H1 |
1H |
protons |
(mass fraction) |
He3 |
3He |
--- |
(mass fraction) |
He4 |
4He |
1 < A < 6 |
(mass fraction) |
C12 |
12C |
--- |
(mass fraction) |
N14 |
14N |
--- |
(mass fraction) |
O16 |
16O |
16O (unburned yet) |
(mass fraction) |
Ne20 |
20Ne |
--- |
(mass fraction) |
Mg24 |
24Mg |
22 < A < 29, excluding 28Si |
(mass fraction) |
Si28 |
28Si |
28Si |
(mass fraction) |
S32 |
32S |
28 < A < 36 |
(mass fraction) |
Ar36 |
36Ar |
35 < A < 40 |
(mass fraction) |
Ca40 |
40Ca |
39 < A < 44 |
(mass fraction) |
Ti44 |
44Ti |
43 < A < 48 |
(mass fraction) |
Cr48 |
48Cr |
47 < A < 52 |
(mass fraction) |
Fe52 |
52Fe |
--- |
(mass fraction) |
Fe54 |
54Fe (+56Fe) |
A approximately 2*Z+2, Iron Peak |
(mass fraction) |
Ni56 |
56Ni |
A < 2*Z+2, Iron Peak |
(mass fraction) |
Fe56 |
--- |
56Fe only |
(mass fraction) |
'Fe' |
--- |
A > 2*Z + 3, Iron Peak, excluding 56Fe |
(mass fraction) |
The Data
Standard Model: Initial solar metallicity, 200
km/s ZAMS equatorial rotation, rotation according to Heger, Langer, & Woosley (2000), magnetic fields according to Spruit
(2002); Heger, Woosley, & Spruit (2004)
Full Nucleosynthesis Data
Models similar to those of Rauscher, Heger, Hoffman, & Woosley
(2002). Full nucleosynthesis data is given only outside the iron core.
Movies
Animation of the evolution of rotation profile and magnetic fields,
solar composition, 200 km/s ZAMS equatorial rotation (from Version 5)
Explosion Models, 100s (preliminary & unpublished)
Note that part of the data sets provided below may be preliminary
and that part of them could change without notice. We would appreciate if you contact us before using the data on this
site for your publications.
Standard Model: Initial solar metallicity, 200
km/s ZAMS equatorial rotation, rotation according to Heger, Langer, & Woosley (2000), magnetic fields according to Spruit
(2002); Heger, Woosley, & Spruit (2004). The data files in this section contain only the APPROX 19 isotope network.
APPROX Network data explanation
column |
description |
unit |
nt1 |
neutrons |
(mass fraction) |
h1 |
1H |
(mass fraction) |
pn1 |
protons (photodisintegration) |
(mass fraction) |
he3 |
3He |
(mass fraction) |
he4 |
4He |
(mass fraction) |
c12 |
12C |
(mass fraction) |
n14 |
14N |
(mass fraction) |
o16 |
16O |
(mass fraction) |
ne20 |
20Ne |
(mass fraction) |
mg24 |
24Mg |
(mass fraction) |
si28 |
28Si |
(mass fraction) |
s32 |
32S |
(mass fraction) |
ar36 |
36Ar |
(mass fraction) |
ca40 |
40Ca |
(mass fraction) |
ti44 |
44Ti |
(mass fraction) |
cr48 |
48Cr |
(mass fraction) |
fe52 |
52Fe |
(mass fraction) |
fe54 |
54Fe (+56Fe) |
(mass fraction) |
ni56 |
56Ni |
(mass fraction) |
0.6 B Explosion Energy
1.2 B Explosion Energy
2.4 B Explosion Energy
|