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A study of relative efficiencies of ...
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Ouellet, Christian Van.
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A study of relative efficiencies of photomultiplier tubes in the Sudbury Neutrino Observatory.
Record Type:
Electronic resources : Monograph/item
Title/Author:
A study of relative efficiencies of photomultiplier tubes in the Sudbury Neutrino Observatory./
Author:
Ouellet, Christian Van.
Description:
89 p.
Notes:
Source: Masters Abstracts International, Volume: 43-06, page: 2255.
Contained By:
Masters Abstracts International43-06.
Subject:
Physics, General. -
Online resource:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=MR01058
ISBN:
0494010584
A study of relative efficiencies of photomultiplier tubes in the Sudbury Neutrino Observatory.
Ouellet, Christian Van.
A study of relative efficiencies of photomultiplier tubes in the Sudbury Neutrino Observatory.
- 89 p.
Source: Masters Abstracts International, Volume: 43-06, page: 2255.
Thesis (M.Sc.)--Queen's University at Kingston (Canada), 2005.
The Sudbury Neutrino Observatory (SNO) is a spherical heavy water Cerenkov-light detector built to understand neutrino physics. In particular it is credited with solving the "missing" solar neutrino problem. The SNO project uses a laser light with a diffuser, called a "laserball", to determine all the optical properties of the SNO detector from attenuation lengths in the water to individual photo-multiplier tube (PMT) characteristics. One such characteristic is the quantum efficiency, and it is the purpose of this study to investigate this quantity. A characteristic of laserball data is that one does not measure quantum efficiency but rather relative efficiencies. This thesis is a systematic analysis of the efficiencies extracted from pre-existing calibration code. Knowing the relative efficiencies increases the understanding of the detector's behavior in a previously unexamined area. Introduction of the PMT-to-PMT variations in efficiency into the pre-existing mathematical Monte-Carlo model of SNO has demonstrated better agreement between the observed and modeled energy resolution of the detector. The implications of this last Monte-Carlo adjustment may impact current published SNO results and further constrain theoretical models for neutrino oscillations.
ISBN: 0494010584Subjects--Topical Terms:
1018488
Physics, General.
A study of relative efficiencies of photomultiplier tubes in the Sudbury Neutrino Observatory.
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Source: Masters Abstracts International, Volume: 43-06, page: 2255.
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The Sudbury Neutrino Observatory (SNO) is a spherical heavy water Cerenkov-light detector built to understand neutrino physics. In particular it is credited with solving the "missing" solar neutrino problem. The SNO project uses a laser light with a diffuser, called a "laserball", to determine all the optical properties of the SNO detector from attenuation lengths in the water to individual photo-multiplier tube (PMT) characteristics. One such characteristic is the quantum efficiency, and it is the purpose of this study to investigate this quantity. A characteristic of laserball data is that one does not measure quantum efficiency but rather relative efficiencies. This thesis is a systematic analysis of the efficiencies extracted from pre-existing calibration code. Knowing the relative efficiencies increases the understanding of the detector's behavior in a previously unexamined area. Introduction of the PMT-to-PMT variations in efficiency into the pre-existing mathematical Monte-Carlo model of SNO has demonstrated better agreement between the observed and modeled energy resolution of the detector. The implications of this last Monte-Carlo adjustment may impact current published SNO results and further constrain theoretical models for neutrino oscillations.
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http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=MR01058
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