Some considerations about cosmogenic production of radioactive isotopes in Ar as target for the next neutrino experiments
arXiv:1712.04399 · doi:10.1016/j.radphyschem.2018.08.009
Abstract
The concept of the LAr TPC technology that is an excellent tracking - calorimeter detector will be used for the next generations of neutrino experiments. In this class of detectors both the scintillation light emitted and the charge produced by the ionization are used to detect and identify the characteristics of the primary particle. The reduction of the radioactive background, the knowledge of the sources and mechanisms of its production as well as the characteristics of the signals have as consequence the increase of the sensitivity of huge detectors and the capability to discriminate between various particles interacting with the detector. Cosmogenic sources of background or activation of different materials become more important in this context. The radioactivity induced by cosmogenic reactions in Ar is discussed by considering muon capture and reactions induced by neutrons as sources of background. The simulated cross sections for the considered nuclear reactions are obtained using TALYS and EMPIRE codes, highlighting the similarities and differences between the results of these nuclear codes and the level of concordance with the few existing experimental data.
References in corpus (10)
- Observation of Coherent Elastic Neutrino-Nucleus Scattering
- Muon simulation codes MUSIC and MUSUN for underground physics
- The scintillation of liquid argon
- Solar and Atmospheric Neutrinos: Background Sources for the Direct Dark Matter Searches
- WIMP Dark Matter Direct-Detection Searches in Noble Gases
- LBNO-DEMO: Large-scale neutrino detector demonstrators for phased performance assessment in view of a long-baseline oscillation experiment
- Photon emission and atomic collision processes in two-phase argon doped with xenon and nitrogen
- Mitigation of Ar/K background for the GERDA Phase II experiment
- Phenomenology of the muon-induced neutron yield
- On concentration of Ar in the Earth's atmosphere