Coming Attractions


Old UCI Page

Announcement

Paper
(submitted to
Phys.Rev.Lett)

Clinton on
Neutrinos

FAQ

Links

Future studies of the neutrino and its mass

A number of experiments are planned or soon to be underway in neutrino physics; all of these will be crucial tests for the newly-discovered neutrino mass.

Sudbury Neutrino Observatory (SNO)sno.gif (42941 bytes)

Sudbury is revolutionary experiment, using a heavy-water target to measure not only the flux of electron neutrinos from the Sun, but using a reaction channel not available in light water, also the total number of neutrinos of all flavors. Clearly an eagerly awaited experiment by all concerned with neutrino oscillations and neutrino mass.

Should SNO find the usual deficit of electron neutrinos, but the predicted total number of neutrinos, it would be not only the solution to the 30-year old solar neutrino problem but ironclad confirmation of neutrino oscillations and neutrino mass

If, on the other hand, SNO finds a neither enough electron neutrinos, nor the muon or tau neutrinos these are thought to oscillate into, it would call for a fourth (exotic) "sterile" neutrino and/or a re-examination of solar models.

K2K

The K2K ("KEK to Kamiokande") experiment will the first of several so-called long-baseline experiments to attempt to replicate the atmospheric neutrino anomaly using a more controlled neutrino beam from an accelerator. Two detectors positioned near the beampipe will measure the muon neutrino flux as it emerges, and Super-Kamiokande, 250 km distant, will look for disappearance of these muon neutrinos. K2K should begin operation in 1999.

MINOS

MINOS is a long-baseline experiment similar in concept to K2K. MINOS' advantages would be a much more intense neutrino beam, and a longer neutrino flight distance to the Soudan-II experiment in Minnesota. With the high luminosity and a fine-grained iron detector at the far end, MINOS may be able to detect the production of tau particles by tau neutrinos - confirming the hypotheses of neutrino mass and oscillation, as well as discovering (directly observing) the tau neutrino as well!

 

Up

Dave Casper