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Responses from Neutrino Physicists


Boris Kayser (National Science Foundation, Washington):

"For years, physicists have dreamed of neutrino mass. Now Super-Kamiokande
has very likely found it. Understanding its origin will take us into new
physics realms."

Alexei Smirnov (International Center for Theoretical Physics,
Trieste, Italy):

"This result is the strongest evidence for neutrino oscillations we
have ever had, although further careful checks of consistency of existing
experimental data are needed."

John Bahcall (Institute for Advanced Study, Princeton):

"The Super-K results are beautiful and provide strong additional
evidence that neutrinos oscillate."

Jean-Marc Gaillard (CERN, Geneva, Switzerland):

"The beauty of Super-Kamiokande was to find the first hard evidence
of neutrino oscillations by covering the complete interference range.
The implications for the neutrino masses will have a great impact on
further experimental exploration and theoretical developments."

Paul Langacker (University of Pennsylvania):

"The exquisite zenith angle distributions observed by Super-K almost
certainly establish the existence of neutrino mass. Small neutrino
masses constitute a subtle probe of particle physics at ultrashort
distances, and may have profound consequences for cosmology and neutrino

Lincoln Wolfenstein (Carnegie-Mellon University, Pittsburgh):

"The most interesting explanation is the 'seesaw mechanism' in grand
unified theories. This could be the first window into new physics at
very high energies inaccessible to particle accelerators. It resulted
from the study of atmospheric neutrinos pioneered by Fred Reines, whose
recent death we mourn."

Pierre Ramond (University of Florida, Gainesville):

"The Super-Kamiokande measurements strongly suggest neutrino oscillations
with parameters (masses and mixing angle) that imply, through the
seesaw mechanism, the existence of a scale commensurate with that
at which the gauge couplings unify. This is in line with the
string/grand-unified view of the world at short distances, and provides
additional evidence for low energy supersymmetry."

Gary Feldman (Harvard University):

"The Super-K results are exciting precisely because they are a priori
unexpected. The complete or almost complete mixing breaks the pattern
seen in the quarks and suggests that we are going to learn something
fundamental about the origin of masses when we finally sort out all of
the lepton masses and mixings."

Rabi Mohapatra (University of Maryland, College Park):

"Nonzero neutrino mass implied by the Super-K results has the profound
consequence that weak interactions must conserve parity at high energies,
making it more like other interactions."

Michael Turner (University of Chicago):

"This is a very exciting result--a neutrino mass of around 0.1 eV means
that neutrinos contribute as much mass density to the Universe as stars
and have an important effect on the development of structure in the Universe."

Gordy Kane (University of Michigan, Ann Arbor):

"I'm writing my first paper ever on neutrino masses.


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