Neutrino
Physics & Experiment
Neutrino physics has had an interesting history. In 1930
Pauli postulated the existence of the (electron) neutrino, in
1956 this was confirmed by Reines and Cowan using a nuclear
reactor source of antineutrinos. In 1962, a second distinct
(muon) neutrino was shown to exist in a BNL experiment. For
that discovery Nobel Prize was awarded to Lederman, Schwartz
and Steinberger. In 1995, the third, (tau) neutrino was
detected at FNAL. In parallel, Ray Davis' studies of solar
neutrinos confirmed understanding of stellar dynamics modulo
a 2/3 flux deficit that later was recognized as a result of
neutrino oscillations among the three flavors of neutrinos.
properties of those oscillations were further unveiled with
followup solar, atmospheric, reactor and accelerator neutrino
studies . The discovery of oscillations, detection of 19
neutrino events from supernova 1987a by the old IMB and
Kamiokande water cerenkov detectors confirmed the theory of
supernova explosions. The WMAP experiment has started to see
imprints of neutrino mass effects on the cosmic microwave
background radiation left from the Big Bang, etc.
Introduction
An intense neutrino facility allows probing of the
neutrino mixing angles, mass hierarchy, and leptonic CP
violation. Physics potential, for making precision
measurements of all neutrino oscillation parameters. using a
wide band nu_µ beam from BNL , to a VLB (very long baseline) 2540
km baseline (with 0.5 megaton) detector at Homestake Mine in
South Dakota was our first study. Potentials of intense
neutrino beams from BNL (later from FNAL) to Long Baseline
Detectors at Homestake (SD), later Henderson (Co) and
Cascades (WA) were studied. Large Detectors located in a low
background underground environment(s) would provide
additional physics capabilities for proton decay and
continuous observation of natural sources of neutrinos such
as supernova. HOMESTAKE is the selected DUSEL Site, Detector
R & D is underway, and some of our neutrino to VLB simulations
illustrated below.
Zohreh Parsa
parsa@bnl.gov
www.neutrino.bnl.gov
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BNL, FNAL and 3 possible
DUSEL Detector Sites, Homestake
(SD), Henderson (CO), cascades(WA). DUSEL selected
site is the Homestake Mine in South Dakota, a distance of
2540 km from BNL and close to 1300 km from FNAL. |
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Super Kamiokande, a Water Cerenkov Detector
Ribon Cutting with Dr. Al Mann
at the

HOMESTAKE, Sanford Underground Laboratory

Drs. Z. Parsa, W. Marciano & W. Wilson in Henderson (a
DUSEL possible) UNDERGROUND Lab site in Colorodo.

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