Fast neutron measurements were performed on the VESUVIO beam-line at the ISIS spallation source using a new telescope proton recoil spectrometer. Neutrons interact on a plastic target. Proton production is mainly due to elastic scattering on hydrogen nuclei and secondly due to interaction with carbon nuclei. Recoil protons are measured by a proton spectrometer, which uses in coincidence a 2.54 cm thick YAP scintillator and a 500μm thick silicon detector, measuring the full proton recoil energy and the partial deposited energy in transmission, respectively. Recoil proton spectroscopy measurements (up to E<inf>p</inf> = 60 MeV) have been interpreted by using Monte Carlo simulations of the beam-line. This instrument is of particular interest for the characterization of the ChipIr beam-line at ISIS, which was designed to feature an atmospheric-like neutron spectrum for the irradiation of micro-electronics.
Cazzaniga, C., Rebai, M., Tardocchi, M., Croci, G., Nocente, M., Ansell, S., et al. (2015). A telescope proton recoil spectrometer for fast neutron beam-lines. PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS, 2015(7) [10.1093/ptep/ptv096].
A telescope proton recoil spectrometer for fast neutron beam-lines
REBAI, MARICASecondo
;TARDOCCHI, MARCO;CROCI, GABRIELE;NOCENTE, MASSIMO;GORINI, GIUSEPPEUltimo
2015
Abstract
Fast neutron measurements were performed on the VESUVIO beam-line at the ISIS spallation source using a new telescope proton recoil spectrometer. Neutrons interact on a plastic target. Proton production is mainly due to elastic scattering on hydrogen nuclei and secondly due to interaction with carbon nuclei. Recoil protons are measured by a proton spectrometer, which uses in coincidence a 2.54 cm thick YAP scintillator and a 500μm thick silicon detector, measuring the full proton recoil energy and the partial deposited energy in transmission, respectively. Recoil proton spectroscopy measurements (up to EI documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.