DocumentCode :
2544413
Title :
Simulations of the cosmic-ray-induced neutron background
Author :
Becchetti, Marc F. ; Ide, Kiyotaka ; Poitrasson-Riviere, Alexis ; Hamel, Michael C. ; Polack, J.K. ; Scarpelli, Matthew L. ; Clarke, Shaun D. ; Flaska, M. ; Pozzi, S.A.
Author_Institution :
Dept. of Nucl. Eng. & Radiol. Sci., Univ. of Michigan, Ann Arbor, MI, USA
fYear :
2012
fDate :
Oct. 27 2012-Nov. 3 2012
Firstpage :
211
Lastpage :
214
Abstract :
A method for simulating the cosmic-ray-induced neutron background at ground level has been developed. This method was used to obtain the expected pulse height distributions, net neutron rates, and angular distribution using EJ-309 liquid scintillators, and has been validated using outdoor measurements. The simulations were carried out using the Monte Carlo transport code MCNPX-PoliMi combined with the source subroutine CRY. The absolute count rates for neutrons were then obtained from the simulations using an empirical scaling formula from literature. Preliminary measurements of the angular distribution of background neutrons were done using a collimated EJ-309 liquid scintillator, showing fair agreement with simulations.
Keywords :
Monte Carlo methods; cosmic ray neutrons; liquid scintillation detectors; neutron detection; pulse height analysers; subroutines; CRY; EJ-309 liquid scintillators; MCNPX-PoliMi; Monte Carlo transport code; absolute count rates; angular distribution; collimated EJ-309 liquid scintillator; cosmic-ray-induced neutron background simulations; empirical scaling formula; net neutron rates; outdoor measurements; pulse height distributions; source subroutine;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Nuclear Science Symposium and Medical Imaging Conference (NSS/MIC), 2012 IEEE
Conference_Location :
Anaheim, CA
ISSN :
1082-3654
Print_ISBN :
978-1-4673-2028-3
Type :
conf
DOI :
10.1109/NSSMIC.2012.6551095
Filename :
6551095
Link To Document :
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