  We show that an oscillating scalar field in supergravity of mass of the order
of $\sim$ TeV with a nonzero vacuum expectation value ($\sim 10^{10}$ GeV) can
be a candidate of cold dark matter (CDM). To avoid the gravitino problem, we
need a low reheating temperature after the primordial inflation. Then, the
energy density of the oscillating scalar field satisfies all the requirements
for CDM at present in the universe.
