Published July 1, 2002
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Journal Article
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Estimates of weak and electromagnetic nuclear decay signatures for neutrino reactions in Super-Kamiokande
- Creators
- Kolbe, E.
- Langanke, K.
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Vogel, P.
Chicago
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Abstract
We estimate possible delayed β decay signatures of the neutrino induced reactions on 16O in a two-step model: the primary neutrino (ν,l) process, where l is the lepton in the final state, is described within the random phase approximation, while the subsequent decay of the excited nuclear state in the final channel is treated within the statistical model. We calculate partial reaction cross sections leading to β unstable nuclei. We consider neutrino energies up to 500 MeV, relevant for atmospheric neutrino detection in Super-Kamiokande, and supernova neutrino spectra.
Additional Information
©2002 The American Physical Society Received 2 October 2001; revised 26 April 2002; published 24 July 2002 Discussions with R. Shrock are gratefully acknowledged. The work has been partly supported by the Danish Research Council. P.V. thanks the Institute of Physics and Astronomy at the University of Aarhus for its hospitality.Files
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Additional details
- Eprint ID
- 6344
- Resolver ID
- CaltechAUTHORS:KOLprd02
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2006-12-04Created from EPrint's datestamp field
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