“…( 1), we treat one neutron branching to an excited state in 180 Ta followed by the detection of two γ rays, γ 1 and γ 2 , out of m γ rays in coincidence as represented by m C 2 =m(m − 1)/2. When one performs an experiment with the chaser detector of Type I or Type II at 10 MeV with a flux of 10 5 photons/s [22,23] and a Ta foil of 100 µm thickness under the conditions listed in Table 1, one finds the event rate summarized in Table 2. In this estimate, we assumed for simplicity that the neutron energy E n =1 MeV, the γ-ray energy E γ =200 keV, the branching ratio b= 0.2, and the neutron multiplicity m=7.…”