Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001neph.conf..214a&link_type=abstract
NEUTRINO PHYSICS Its Impact on Particle Physics, Astrophysics and Cosmology. Proceedings of the Carolina Symposium on Neutrino P
Astronomy and Astrophysics
Astrophysics
Scientific paper
ORLaND, the Oak Ridge Laboratory for Neutrino Detectors, is a proposed underground laboratory adjacent to the target station of the Spallation Neutron Source (SNS) under construction at the Oak Ridge National Laboratory (ORNL). The neutrons, copious πmesons, and hence neutrinos, will be generated by a 1.3 GeV proton beam (2 MW) impinging on a mercury target with 600 ns wide pulses at 60 Hz. The neutrino production rates are predicted to be: R(ν e) = R(ν μ ) = R(bar {ν }μ ) = 9.4 × 1014 sec-1. Fluxes from this source will be adequate to support a broad program of neutrino-nucleus cross-sections important in nuclear physics, nuclear astrophysics, and elementary particle physics. A broad selection of possible experiments is discussed.
Avignone Frank T.
Efremenko Yuri V.
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