Thursday, April 3, 2008, 3:00 pm — Small Seminar Room, Bldg. 510
The measurements made in Solar Neutrino physics have produced some of
the most exciting results in physics in the past decade. Yet over 99%
of the solar neutrino flux, those coming from proton-proton fusion
reactions in the sun, have not been detected in real-time. This talk
will outline the design of a novel new detector which is being developed
to measure these low energy neutrinos from the sun. This tracking
detector will use Cryogenic Noble Fluids, and the properties of
'electron bubbles' to detect these elusive particles.
Hosted by: David Jaffe
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