Working Group Leaders:
Giorgio Gratta
Wick Haxton
The President's FY2003 National Science Foundation budget request
to Congress called for an NSF-sponsored conference to address
underground science (particularly neutrino physics). One motivation
is the effort by the science community to create a deep
National Underground Science and Engineering
Laboratory (NUSEL). This working group will organize the meeting's
parallel sessions on future double beta decay experiments and
related developments in ultra-low-level counting facilities.
Goals of the Parallel Sessions on Double Beta Decay and Low-Level Counting
Neutrinoless double beta decay is a direct test of lepton number
violation and, in most scenarios, probes the overall
scale of neutrino mass. Recent measurements of solar and
atmospheric neutrino oscillations, which depend on the differences
in the squares of the masses, suggest that neutrinoless double
beta decay might be observable in a new generation of experiments
approximately a factor of 100 larger than those currently mounted.
Such experiments will provide an important window on beyond-the-
standard-model physics that includes neutrino mass, the
Majorana/Dirac character of the neutrino, other mechanisms
for lepton number violation, and CP violation among neutrinos.
The double beta decay parallel sessions will focus on the physics
and astrophysics motivations for new experiments. The sessions
will include theory issues and presentations from proponents
of major experiments now under
development, including their background requirements and infrastructure
needs. Because materials purity is so essential to such
experiments, low-level counting facilities will be included in
these sessions.
Participation and Contributed Talks
Information on the meeting, including registration and housing,
can be found at the web site, http://www.physics.umd.edu/ness02/.
If you would like to present a talk in one of the double beta decay
working groups, please submit a contributed talk abstract. We do not yet know how much time we will be
allocated, but will do our best to schedule as many talks as is
feasible. Priority will be given to experimental talks on future
projects in which depth and other background requirements are
discussed.
We have compiled a list of community members we
believe are interested in double beta decay and low-level counting.
Please let the working group organizers know of other individuals
that should be added to this list. We understand that strong
community participation in NESS02 is important to the prospects for
creating NUSEL.
Some support is available for the local expenses of students and
other young researchers. Please notify the Working Group Leaders
of young people that potentially require such support.
gratta@stanford.edu
Phone: (650) 725-6509
Physics Dept.
Stanford University
Stanford CA 94305-4060
haxton@phys.washington.edu
Phone: (206) 685-2397
INT, Box 351550
University of Washington
Seattle, WA 98195