Abstract
A selection of opportunities for neutrino physics from a source generated from pions that decay in flight and at rest is described. The present source at LAMPF has a duty factor of about 6%; improvements in opportunities that emerge from a source using a pulse 0.25 μsec long from a proton storage ring are also described.
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References
K. S. Hirata et al., Phys. Rev. Lett. 65(1990)1297
J. N. Bahcall, Neutrino Astrophysics, Chapter 7, University Press, Cambridge, 1989
R. Davis, Jr., in Proceedings of the 21st International Cosmic-Ray Conference, Adelaide, Australia
J. J. Simpson, Phys. Rev. Lett. 54(1985)1891
D. Caldwell and P. Langacker, preprints UCSB-HEP-91–02 and UPR-0469T
L. A. Ahrens et al., Phys. Rev. D31(1985)2732
Proposal to search for neutrino oscillations in the appareance channels νμ → νe and ̄vμ → ̄ve, Los Alamos National Laboratory report LA-11842-P (1989)
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© 1992 Springer-Verlag
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White, D.H. (1992). Medium-energy neutrino physics. In: Jungmann, K., Hughes, V.W., zu Putlitz, G. (eds) The Future of Muon Physics. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-77960-2_30
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DOI: https://doi.org/10.1007/978-3-642-77960-2_30
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-77962-6
Online ISBN: 978-3-642-77960-2
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