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The Sudbury Neutrino Observatory: Comparison of Phases

โœ Scribed by M.C. Chen

Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
337 KB
Volume
145
Category
Article
ISSN
0920-5632

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๐Ÿ“œ SIMILAR VOLUMES

The Sudbury Neutrino Observatory
The Sudbury Neutrino Observatory
โœ G.T. Ewan ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 766 KB
The Sudbury neutrino observatory
The Sudbury neutrino observatory
โœ G. Jonkmans ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 290 KB

The Sudbury Neutrino Observatory (SNO) is a second generation water cerenkov detector designed to study neutrino astrophysics. We will describe the SNO detector, nearing completion deep underground in INCO's Creighton Mine neaS Sudbury, Canada and the physics potential of the detector.

Results from the Sudbury Neutrino Observ
Results from the Sudbury Neutrino Observatory Phase III
โœ G. Prior ๐Ÿ“‚ Article ๐Ÿ“… 2009 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 209 KB

The third and last phase of the Sudbury Neutrino Observatory (SNO) used a technique independent of previous methods, to measure the rate of neutral-current interactions in heavy water and determine precisely the total active 8 B solar neutrino flux. The total flux obtained is 5.54 +0.33 -0.31 (stat)

Measurement of Atmospheric Neutrinos at
Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
โœ J.A. Formaggio ๐Ÿ“‚ Article ๐Ÿ“… 2009 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 174 KB

The Sudbury Neutrino Observatory consists of a 1 kiloton heavy water Cherenkov detector able to detect and reconstruct high-energy muons created from cosmic ray showers and atmospheric neutrino interactions. By measuring the flux of through-going muons as a function of zenith angle, the SNO experime