Optimised neutron yield calculations from (α,n) reactions with the modified SOURCES4 code

The sensitivity of underground experiments searching for rare events such as dark matter, neutrino interactions or several beyond the standard model phenomena is often limited by the background caused by neutrons from spontaneous fission and (α,n) reactions. A number of codes exist to calculate neutron yields and energy spectra due to these processes. In this paper we present new calculations of neutron production using the modified SOURCES4 code with recently updated cross-sections for (α,n) reactions and the comparison of the results with available experimental data. The cross-sections for (α,n) reactions in SOURCES4 have been taken from reliable experimental data where possible, complemented by the calculations with EMPIRE 2.19/3.2.3, TALYS 1.96 or evaluated data library JENDL-5 where experimental data were scarce or unavailable. We present here our choice of the most reliable cross-sections for such calculations that match experimental data from alpha beams and radioactive decays.