Abstract
During the last few years a significant number of neutrino interactions has been recorded in large underground detectors, mainly nucleon decay detectors. A good understanding of these neutrino events is a requisite in nucleon decay analyses, where they are the most important background, giving 3 x 10-31 interactions per nucleon per year. A decisive contribution to the measurements of neutrinos and antineutrinos from cosmic ray interactions in the atmosphere comes from these underground experiments, which made analyses with emphasis on the GeV energy range.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
T.K. Gaisser et al., Bartol Research Institute report, BA-88-1, 1988
K.S. Hirata et al., Phys. Lett. B205. 416 (1988)
L.V. Volkova and T.K. Gaisser, private communications.
Ch. Berger et al., Nucl. Instr. and Meth. A262. 463 (1987)
C Longuemare, in Proceedings of IX Workshop on Grand Unification, (Aix-les-Bains, France, 1988) ; to be published
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1989 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
Arpesella, C. (1989). Flavor Composition of Atmospheric Neutrinos in Underground Detectors. In: Kotthaus, R., Kühn, J.H. (eds) XXIV International Conference on High Energy Physics. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-74136-4_153
Download citation
DOI: https://doi.org/10.1007/978-3-642-74136-4_153
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-74138-8
Online ISBN: 978-3-642-74136-4
eBook Packages: Springer Book Archive