Shielding of Neutron Emission Ratio Observer from Neutrons Produced by Cosmic Rays
CSEF · 2004 Physics & Astronomy
Overview
Objectives/Goals To investigate the cosmic ray neutron attenuation effects of passive and active shielding on the neutron emission ratio observer (NERO), a low-energy neutron detector. Methods/Materials Passive shielding consisted of water, boron carbide, and a combination of the two materials. Active shielding consisted of a VETO gate using the inputs of the neutron detector and a coincidental signal from two plastic scintillators. Results Boron carbide absorbed 13% of neutrons, water 42%, and a combination of the two, 48%. Active shielding was shown to reject NERO signals, and the rejected signals were shown to have been confined to the neutron-specific energy ranges. Conclusions/Discussion Both boron carbide, water, and a combination of the two were shown to be effective neutron attenuators. Active shielding was shown to be effective, but because of a short time window in which NERO signals were rejected, only about 0.7% of the total neutrons were rejected. This problem could be fixed by using a longer time window to account for the difference in processing speed between the scintillators and neutron detector.
Summary statement
My project tests the effectiveness of shielding a low-energy neutron detector from neutrons produced by cosmic rays.
Help received
Participant in Michigan State University High School Honors Science Program. Used lab equipment at National Superconducting Cyclotron Laboratory at Michigan State University under the supervision of Dr. Hendrik Schatz. NERO is sponsored by the Joint Institute for Nuclear Astrophysics.
Competition history
- CSEF 2004
Resources
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