Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3445..121h&link_type=abstract
Proc. SPIE Vol. 3445, p. 121-131, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, Oswald H. Siegmund; Mark A. Gummin
Astronomy and Astrophysics
Astronomy
Scientific paper
The importance of shields for suppressing neutron-induced background in new classes of (gamma) -ray detectors such as CZT has been emphasized for a variety of reasons. These include high cross-sections for neutron interactions in detector materials and inefficient vetoing of neutrons in conventional active shields. We previously demonstrated through Monte-Carlo simulation how our new approach, supershields, is superior to the monolithic, biatomic neutron shields which have been developed in the past. Here we show the construction of several prototype models for supershields using B and H. We verify the performance of these supershields through lab experiments using radioactive sources and monoenergetic neutron beam at the Radiological Research Accelerator Facility, and compare the results with monolithic neutron shields. We also discuss the implications of this experiment for designs of supershields in general.
Craig William W.
Hailey Charles J.
Hong Jaesub
No associations
LandOfFree
Development of neutron shields for gamma-ray detectors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Development of neutron shields for gamma-ray detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Development of neutron shields for gamma-ray detectors will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-805435