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