Intrinsic neutron background of nuclear emulsions for directional Dark Matter searches

• Published in: Astroparticle physics 2016-07, Vol.80, p.16-21
• Main Authors: Alexandrov, A., Asada, T., Buonaura, A., Consiglio, L., D’Ambrosio, N., De Lellis, G., Di Crescenzo, A., Di Marco, N., Di Vacri, M.L., Furuya, S., Galati, G., Gentile, V., Katsuragawa, T., Laubenstein, M., Lauria, A., Loverre, P.F., Machii, S., Monacelli, P., Montesi, M.C., Naka, T., Pupilli, F., Rosa, G., Sato, O., Strolin, P., Tioukov, V., Umemoto, A., Yoshimoto, M.
• Format: Article
• Language: English
• Subjects: Background radiation; Compatibility; Dark matter; Neutron background; Nuclear emulsions; Radiopurity; Recoil; Searching; Simulation; Tracking
• ISSN: 0927-6505; 1873-2852
• DOI: 10.1016/j.astropartphys.2016.03.003

Recent developments of the nuclear emulsion technology led to the production of films with nanometric silver halide grains suitable to track low energy nuclear recoils with submicrometric length. This improvement opens the way to a directional Dark Matter detection, thus providing an innovative and complementary approach to the on-going WIMP searches. An important background source for these searches is represented by neutron-induced nuclear recoils that can mimic the WIMP signal. In this paper we provide an estimation of the contribution to this background from the intrinsic radioactive contamination of nuclear emulsions. We also report the neutron-induced background as a function of the read-out threshold, by using a GEANT4 simulation of the nuclear emulsion, showing that it amounts to about 0.06 per year per kilogram, fully compatible with the design of a 10 kg × year exposure.