• Title of article

    -Ray background sources in the VESUVIO spectrometer at ISIS spallation neutron source

  • Author/Authors

    Pietropaolo، نويسنده , , A. and Perelli Cippo، نويسنده , , E. and Gorini، نويسنده , , G. and Tardocchi، نويسنده , , M. and Schooneveld، نويسنده , , E.M. and Andreani، نويسنده , , C. and Senesi، نويسنده , , R.، نويسنده ,

  • Pages
    4
  • From page
    121
  • To page
    124
  • Abstract
    An investigation of the gamma background was carried out in the VESUVIO spectrometer at the ISIS spallation neutron source. This study, performed with a yttrium–aluminum–perovskite (YAP) scintillator, follows high resolution pulse height measurements of the gamma background carried out on the same instrument with the use of a high-purity germanium detector. In this experimental work, a mapping of the gamma background was attempted, trying to find the spatial distribution and degree of directionality of the different contributions identified in the previous study. It is found that the gamma background at low times is highly directional and mostly due to the gamma rays generated in the moderator–decoupler system. The other contributions, consistently to the findings of a previous experiment, are identified as a nearly isotropic one due to neutron absorption in the walls of the experimental hall, and a directional one coming from the beam dump.
  • Keywords
    Gamma background , Spallation neutron source , Neutron instrumentation
  • Journal title
    Astroparticle Physics
  • Record number

    2024464