The network structure of radiation-cross-linked solutions of star mole
cules is analyzed theoretically and experimentally. We synthesize gels
via electron beam irradiation of aqueous solutions of high-functional
ity (f > 30) star PEO in the concentration regime where the molecules
exhibit extensive overlap. The expected network properties of the resu
lting gels are systematically varied by using PEO stars with different
arm lengths and functionalities and by adjusting the irradiation dose
and initial polymer concentration. The cross-link density in these ge
ls is analyzed three ways: (1) elastic modulus, (2) swelling equilibri
um, and (3) comparison to the cross-link density of linear gels prepar
ed in a comparable fashion. In order to predict the network structure
of cross-linked star molecules from swelling, Flory's equilibrium swel
ling theory is modified to include a bimodal distribution of cross-lin
k functionalities. The modified equation fits the trends in swelling b
ehavior of the series of radiation-cross-linked star PEO gels. The app
arent cross-link density of radiation-cross-linked star PEO gels obtai
ned by physical property measurement-swelling and elastic modulus-diff
er from the cross-link density expected based on comparison to linear
gels cross-linked under identical conditions. Cross-link densities bas
ed on the elastic modulus are lower than the expected values, suggesti
ng that a significant fraction of elastically ineffective cross-links
form between star af ms within the same molecule.