In a core of fresh fuel, as is the case in the first cycle, and usually in the second cycle, where the max burnup is low, yes one uses startup sources to provide sufficient neutrons to the detection systems.
In fresh or first cycles cores, there are primary neutron sources, e.g., PuBe, RaBe, AmBe or more commonly these days Cf(252)Be, that use (α,n) reactions, in which an alpha from Pu, Ra, Am or Cf fuses with the Be nucleus to form an excited C
13, which then emits a neutron and becomes a C
12 nucleus.
http://en.wikipedia.org/wiki/Startup_neutron_source
The added benefit of Cm is spontaneous fission.
After at least 3 annual cycles, or 2 18-mo or 24-mo cycles, there is sufficient TU elements, or radioisotopes of Pu, Am, Cm to have sufficient spontaneous fissions to produce the necessary neutron activity to monitor the approach to criticality.
Otherwise there is a secondary source of neutrons (Sb-Be) which uses activation of Sb-123 to produce Sb-124, which decays to Te-124, and in the process a 1.7 MeV gamma is emitted which induces photoneutron emission. The secondary source produces neutrons during the second and third cycles of a young reactor, until there is sufficient TU inventory.