Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
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...
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| Materialtyp: | Artikel |
| Språk: | en_US |
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Elsevier B.V.
2009
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| Länkar: | http://hdl.handle.net/1721.1/49855 https://orcid.org/0000-0002-3757-9883 |