Chandrasekhar Limit Set Results

White Dwarf &/or Supernova Core Set Condition Code Key

0 = newtonian gravitation, 1 = general relativity

2 = newtonian,
es-screened, 3 = gen rel, es-screened

4 = newton, w neutronization, 5 = gr,
w neutronization

6 = newton, w screening and neutronization

7 = gr, w
screening and neutronization

8 = gr, w purely neutrons

9 =
Harrison-Wheeler, newtonian

10 = Harrison-Wheeler, gen. rel.

11 =
Harrison-Wheeler, gen.rel., screening.

12 = Baym-Bethe EOS

13 =
Bowers&Deeming non-rel. degen neutron gas

14 = Bowers&Deeming
non-rel. degen n. gas w quark lim

15 = Neutron object as non-screened
D-Quark gas

16 = Neutron object as U-quark-screened D-Quark gas

17 =
Relativistic Neutron gas with Chandra-like EOS

Model Number of Models = 1

model=0 condition code = 2

step differential dr = 1.000000e+05 cm

dr
x steps[m] = 1.280000e+08 cm, 1.280000e+05 km

central density = 1.000000e+10
gr/cm3, Z[start] = 26, A = 56.000000

rp = 1.840552e-03 solar radii =
1.281000e+03 km

Pressure < epsilon on exit from integration.

M [upper
limit] = 1.350375e+00 solar masses

M [lower limit] = 1.342485e+00 solar
masses

structure file stored = 1

steps = 1280

binding energy =
1.200254e+51 ergs

internal thermal energy = 2.111102e+41 ergs

moment of
inertia [cgs] = 4.518403e+48

angular rev/sec = 0.000000

ang.velocity =
0.000000e+00 rad/sec

polar R in km = 1.281000e+03

equitorial R in km =
1.281000e+03 ellipticity e = 0.000000

flyapart = 0

redshift =
1.556235e-03

Looplim = 2001

Step divisor = 5, rotate = 1

Quark EOS above 1.44 x
10**16 = 0

INITIAL SETUP. 1 models in the set.

model 0 ro0 = 1.000000e+10, condition_code = 2 Z = 26, A = 56.000000

calstruc = 1, rev/sec = 0.000000