Star chains composed of arms with uniform length were generated on a s
imple cubic lattice by the Monte Carlo method using the enrichment alg
orithm, which enabled us to obtain chains with total segment numbers (
N) up to 1200. The number of arms (f) ranged from 2 to 24. The radius
of gyration ([S-2](1/2)), the dimensionless intrinsic viscosity (E), a
nd the hydrodynamic radius (R-H) were evaluated as functions off and N
by averaging over more than 4000 samples. The calculations of E and R
-H were made according to Zimm's method. It was found that the radius
expansion factor (alpha(s)) for Star chains with long arms obeys the r
elation alpha(s)(2) = 1.53z(2/5), which is known for long flexible lin
ear chains, where z is the excluded volume parameter. The ratios of [S
-2], E, and R-H Of star chains to those for Linear chains were evaluat
ed as functions off. These ratios obtained and the Flory factors for t
he intrinsic viscosity and R-H extrapolated to N-1/2 --> 0 reproduced
experimental data well.