Development of a low-background neutron detector array

Abstract

A low-background neutron detector array was developed to measure the cross section of the $$^{13}$$ C( $$\alpha$$ ,n) $$^{16}$$ O reaction, which is the neutron source for the s-process in AGB stars, in the Gamow window ( $$E_\text {c.m.}$$ = 190 ± 40 keV) at the China Jinping Underground Laboratory (CJPL). The detector array consists of 24 $$^{3}$$ He proportional counters embedded in a polyethylene cube. Owing to the deep underground location and a borated polyethylene shield around the detector array, a low background of 4.5(2)/h was achieved. The $$^{51}$$ V(p, n) $$^{51}$$ Cr reaction was used to determine the neutron detection efficiency of the array for neutrons with energies $$E_\text {n}<$$ 1 MeV. Geant4 simulations are shown to effectively reproduce the experimental results. They were used to extrapolate the detection efficiency to higher energies for neutrons emitted in the $$^{13}$$ C( $$\alpha$$ ,n) $$^{16}$$ O reaction. The theoretical angular distributions of the $$^{13}$$ C( $$\alpha$$ ,n) $$^{16}$$ O reaction were shown to be important in the estimation of the uncertainties of the detection efficiency.