๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

The Sudbury Neutrino Observatory

โœ Scribed by G.T. Ewan


Publisher
Elsevier Science
Year
1992
Tongue
English
Weight
766 KB
Volume
314
Category
Article
ISSN
0168-9002

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


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.

Measurement of Atmospheric Neutrinos at
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

Results from the Sudbury Neutrino Observ
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)