


Underground science includes studies at the frontiers of particle physics, nuclear physics,
astronomy, geology, and biology, as well as applied areas such as materials science and
nuclear proliferation. In the past decade, fundamental progress has been made in underground
experiments in such diverse and exciting fields as nucleon decay, atmospheric neutrino
oscillations, the solar neutrino measurements, searches for dark matter, the measurement of
nuclear fusion cross sections at stellar temperatures, and the discovery of novel
microorganisms that live deep in the earth. In order to participate in these discoveries, U.S.
scientists have had to either take their equipment to other countries or, in a few cases, to make
use of non-optimal facilities in the U.S.
The questions addressed by underground experiments are among the most fundamental and
exciting problems in modern science. Underground experiments will continue to be at the
forefront of fundamental science in the coming decade. Many of the science projects are
described in some detail in the accompanying document `Underground Science.’
The next generation of underground experiments is more challenging technically than previous
studies and will therefore require both significant resources and good planning and
management to succeed. Creating a National Underground Science Laboratory (NUSL) will
establish the conditions that will enable the science, which must be done with large,
sophisticated equipment, to succeed in a cost effective way. A well run NUSL will have a
coherent research program whose priorities are constantly reviewed in order to produce the
best science results.
There are advantages in centralizing most of the experiments in one underground laboratory:
The committee believes that the arguments in favor of a National Underground Science
Laboratory are compelling and urgent.
In order to be world-class, the NUSL must be deep. A depth of approximately 6000-7000
meters of water equivalent (m.w.e) is desirable for many classes of experiments and is
required for certain experiments such as the next generation of solar neutrino and double
beta-decay experiments. Above this level, interference from the cosmic ray related
backgrounds constitute the limiting factor for high sensitivity experiments. The next generation
solar neutrino detectors, dark matter searches, and double beta-decay studies require as low a
cosmic ray produced muon flux as possible. The simplest and most reliable way to achieve
lower cosmic-ray induced backgrounds is to do experiments at greater depths.
The Committee has received many Letters of Interest by scientists throughout the world who
would like to perform pioneering experiments in different subjects using such a deep
underground laboratory. Currently, he deepest available general underground scientific
laboratory is located at a depth of 3800 m.w.e. in the Gran Sasso National Laboratory in Italy.
We believe that the United States will be in a position to lead the world in pioneering
scientific investigations by establishing a National Underground Science Laboratory with a
depth extending to 7000 m.w.e.