Mathematics
Scientific paper
Oct 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002phdt.........9a&link_type=abstract
Thesis (PhD). BROWN UNIVERSITY, Source DAI-B 63/04, p. 1888, Oct 2002, 232 pages.
Mathematics
7
Scientific paper
The Sudbury Neutrino Observatory (SNO) is a real time solar neutrino experiment. The detector utilizes 1,000 metric tons of heavy water to study the fundamental properties of neutrinos. The SNO detector has been designed to measure the flux and energy spectrum of electron-type solar neutrinos in addition to measuring the total flux of all active flavors of solar neutrinos. The primary objective of SNO is to resolve the Solar Neutrino Problem. The measurement of the neutron signal is critical to the success of SNO. Therefore, it is imperative that one thoroughly understands the various backgrounds to the neutron signal. Even though the rock overburden of 6,150 meter water equivalent provides a very good shield to cosmic muons, enough of them penetrate the detector to produce secondary particles, in particular neutrons. In this dissertation results from the study of through-going muons and neutron production due to muon spallation in the SNO detector has been presented. The following daily muon rate was found:
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