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KamLAND Websites with additional images can be
accessed at http://hep.stanford.edu/neutrino/KamLAND/KamLAND.html
The Japanese KamLAND Website can be accessed at: http://www.awa.tohoku.ac.jp/html/KamLAND/.
TUSCALOOSA, Ala. - Results from the first six months of experiments
at KamLAND, an underground neutrino detector in central Japan, show
that anti-neutrinos emanating from nearby nuclear reactors are “disappearing,”
which indicates they have mass and can oscillate, or change, from
one type to another.
The University of Alabama has two faculty members, a post-doctoral
research associate and several graduate students involved in the
international project.
Neutrinos are subatomic particles that interact so rarely with
other matter that one could pass untouched through a wall of lead
stretching from the earth to the moon. They are produced during
nuclear fusion, the reaction that lights the sun and other stars.
Anti-neutrinos are created in fission reactions such as those that
drive nuclear power plants.
It is hoped that this research will one day be able to help unlock
the secrets about the fundamental nature of matter, how the sun
works, the composition and evolution of the Earth, the process of
star collapse and the origin and future of the universe.
In a paper for Physical Review Letters, the 92 physicists from
Japan, the United States and China, who make up the KamLAND collaboration,
report that during 145 days of operation, they recorded 54 electron
anti-neutrino events in the energy range of one to 10 million electron
volts, as opposed to the approximately 86 events predicted by the
Standard Model under the assumption that no oscillations occur.
Anti-neutrinos are the anti-matter counterpart to neutrinos. These
results, obtained using well-understood, man-made anti-neutrino
sources, provide independent confirmation of earlier studies involving
solar neutrinos and show that the Standard Model of Particle Physics,
which has successfully explained fundamental physics since the 1970’s,
is in need of updating.
The results also point the way to the first direct measurements
of the total radioactivity of the earth.
University of Alabama researchers have been involved in the KamLAND
project since the beginning of its construction in 1998.
“This research has put another piece of the puzzle in place,”
said Dr. Jerrry Busenitz, professor of physics at The University
of Alabama. “KamLAND has provided an important confirmation
that neutrinos do in fact oscillate.”
“There have been a wide range of hypotheses on this subject,
and neutrino research is scientifically popular right now,”
said Dr. Andreas Piepke, professor of physics at The University
of Alabama. “The results of our research are strong evidence
that we are well on the way to a full understanding of neutrinos.”
KamLAND stands for Kamioka Liquid scintillator Anti-Neutrino Detector.
Located in a mine cavern beneath the mountains of Japan’s
main island of Honshu, near the city of Toyama, it is the largest
low-energy anti-neutrino detector ever built. The detector consists
of a 13 meter (43 feet) in diameter weather balloon filled with
about a kiloton of liquid scintillator, a chemical soup that emits
flashes of light when an incoming anti-neutrino collides with a
proton.
These light flashes are detected by a surrounding array of 1,879
photomultiplier light sensors, which convert the flashes into electronic
signals that computers can analyze. The photomultipliers are attached
to the inner surface of an 18-meter in diameter stainless steel
sphere and separated from the weather balloon by a buffering bath
of inert oil and water, which helps suppress interference from background
radiation.
The anti-neutrino events that were recorded in the KamLAND detector
for this study stem from electron anti-neutrinos that originated
from the 51 nuclear reactors in Japan plus 18 reactors in South
Korea. Anti-neutrinos, like neutrinos, come in three different types
or “flavors,” electron, muon and tau.
According to the predictions from the Standard Model, neutrinos/anti-neutrinos
are without mass. Contrary to this, over the past years, neutrino
experiments implied that the ghost-like snippets of matter do possess
mass, enabling them to oscillate and change flavor over a distance.
KamLAND’s results are compatible with earlier results and
were obtained using a complementary approach.
Construction of the KamLAND detector began in 1998 and operations
began in January of 2002.
Japan’s Ministry of Education, Science, Sports, and Culture
provided more than $20 million of KamLAND’s construction costs.
The U.S. Department of Energy’s Office of Science provided
nearly $6 million.
The KamLAND experiments will continue for several more years, making
refined measurements of reactor neutrinos that should shed more
light on neutrino mass and flavor mixing. Since anti-neutrinos also
are produced during the decay of radioactive uranium and thorium
in the crust and mantle of the Earth, the KamLAND detector can also
be used to measure our planet’s internal radioactivity.
KamLAND, with a more purified liquid scintillator, will also be
used to study solar neutrinos in a new low energy regime. For now,
the evidence of neutrino oscillations and flavor has been firmly
established.
The KamLAND neutrino experiments are being conducted by an international
collaboration largely comprised of scientists from Japan and the
United States. The U.S. team at KamLAND includes researchers from
The University of Alabama, the University of California Berkeley,
Stanford University, the California Institute of Technology, Drexel
University, the University of Hawaii, Louisiana State University,
the University of New Mexico, the University of Tennessee, Duke
University, the University of North Carolina and North Carolina
State University.
The Japanese team at KamLAND is led by Atsuto Suzuki, a professor
of physics at the Research Center for Neutrino Science at Tohuku
University. Suzuki is the overall head of the international collaboration,
which also includes, in addition to Tohuku University participants,
researchers from the Institute of High Energy Physics in Beijing.
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