Multiarm star polymers represent a valuable model system for investigating
the dynamics of tethered chains, spherical brushes, or grafted colloidal sp
heres. Because of their topology, the multiarm stars exhibit a nonuniform m
onomer density distribution leading to a core-shell morphology, which is re
sponsible for their rich dynamic structure. When the stars interpenetrate,
they exhibit liquidlike (macrocrystalline) order due to the enhanced osmoti
c pressure which balances the entropic stretching of the near-core segments
and the excluded volume effects. Using dynamic light scattering, we probe
three relaxation modes in the semidilute regime: (i) the fast cooperative d
iffusion, which is characteristic of their polymeric nature (entangled shel
l arms); (ii) the self-diffusion of the stars (essentially cores), probed b
ecause of finite functionality polydispersity, as confirmed by independent
pulsed-field gradient NMR measurements; and (iii) the structural mode, whic
h corresponds to rearrangements of the ordered stars. We develop a mean-fie
ld scaling theory, which captures all features observed experimentally with
good quantitative agreement. The two slow modes, ii and iii, are reminisce
nt of the behavior of interacting hard colloidal spheres and are governed e
ssentially by the same physics. We propose these model soft spheres as appr
opriate vehicles for unifying the descriptions of the dynamics of polymers
and soft colloidal dispersions.