  In order to study the structure of neutralino star and dark galaxy, we
consider dynamical interactions due to boson-exchange in the neutralino matter.
Taking into account interactions of neutralinos with bosons, we derive the
equation of state (EOS) of neutralino stars in terms of the relativistic mean
field approach. Then we apply the resulting EOS to investigate properties of
the neutralino star such as its density profile and mass limit. For example, if
the neutralino mass is around 1 TeV, the Oppenheimer mass limit of the
neutralino star is obtained as $6.06\times 10^{-7}M_\odot$, and the
corresponding radius is about 7.8 mm. Actually, due to an increasing
annihilation rate as indicated by our calculation, this dense state can never
be realized in practice. Our results also show that the low density neutralino
star may be a possible aggregation of the cold dark matter.
