Oscillating scalar-field dark matter in supergravity
arXiv:hep-ph/0109276 · doi:10.1088/1126-6708/2001/09/032
Abstract
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.
LaTeX JHEP-format, to appear in JHEP