Author:
Zhou Weixin,Cui Tongyuan,Zhang Zhi,Yang Yigang,Yi Han,Hou Donghui
Abstract
Abstract
The CLYC(Ce) (Cs2LiYCl6:Ce3+) scintillator can
identify different particles with various specific energy losses and
is capable of measuring the fast neutron energy via the
35Cl(n,p)35S reaction. Thus, it is rational to expect
using this detector for monitoring the on-site neutron dose rate for
astronauts or equipments working at a spacecraft, which may undergo
the irradiation of cosmic rays of energetic protons or alpha
particles that could induce the production of spallation
neutrons. However, as the spallation neutrons, as well as the
moderated neutrons, have an energy distribution from the thermal
region to several hundred MeV, the direct measurement of the neutron
spectrum, which helps calculate the exact value of dose rate in the
spacecraft, requires that the energy response matrices should be
known in advance. In this study, we calibrated a
Φ38 mm × 38 mm CLYC(Ce) scintillator detector with
the Back-n beamline at the China Spallation Neutron Source (CSNS),
acquiring its energy response matrices (ERM) ranging from 0.1 MeV
to 100 MeV. To verify the CLYC(Ce) scintillator detector's
capability for measuring neutrons with such a wide region, using the
ERM, the energy spectrum of the Back-n beamline was reconstructed
and the result conformed to the CSNS-measured result well; a good
conformation between the reconstructed spectrum and the standard
Watt fission neutron spectrum of 252Cf was also observed. This
calibrated detector then was used to measure the cosmic-ray induced
neutron spectra at five different sites in China of various
altitudes. The measured neutron fluxes at five different sites
conformed to results predicted by the EXcel based Program
Atmospheric Cosmic-ray Spectrum (EXPACS). The results presented in
this study indicate that the CLYC(Ce) scintillator detector is
promising to be used in spacecraft as a neutron monitor with a wide
energy range.
Subject
Mathematical Physics,Instrumentation
Cited by
19 articles.
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