Scientists help explain scarcity of antimatter
A collaboration, with major participation by physicists at the University of Wisconsin-Madison, has made a precise measurement of elusive, nearly massless particles, and obtained a crucial hint as to why the universe is dominated by matter, not by its close relative, antimatter.
The particles, called antineutrinos, were detected at the underground Daya Bay experiment, located near a nuclear reactor in China, 55 km north of Hong Kong.
For the measurement of antineutrinos it made in 2012, the Daya Bay collaboration has been named runner-up for breakthrough of the year from Science.
Antiparticles are almost identical twins of subatomic particles (electrons, protons, and neutrons) that make up our world. When an electron encounters an antielectron, for example, both are annihilated in a burst of energy. Failure to see these bursts in the universe tells physicists that antimatter is vanishingly rare, and that matter rules the roost in today's universe.
"At the beginning of time, in the Big Bang, a soup of particles and antiparticles was created, but somehow an imbalance came about," says Karsten Heeger, a professor of physics at UW-Madison. "All the studies that have been done have not found enough difference between particles and antiparticles to explain the dominance of matter over antimatter."
But the neutrino, an extremely abundant but almost massless particle, may have the right properties, and may even be its own anti-particle, Heeger says. "And that's why physicists have put their last hope on the neutrino to explain the absence of antimatter in the universe."
Heeger and his group at UW-Madison have been responsible for much of the design and development of the antineutrino detectors at Daya Bay. Jeff Cherwinka, from the university's Physical Sciences Laboratory in Stoughton, Wis. is chief engineer of the experiment and has overseen much of the detector assembly and installation. The construction of the experiment was completed this fall and data-taking started in October using the full set of antineutrino detectors.
Reactors, Heeger says, are a fertile source of antineutrinos, and measuring how they change during their short flights from the reactor to the detector, gives a basis for calculating a quantity called the "mixing angle," the probability of transformation from one flavor into another.
The measurement of the Daya Bay experiment, released in March 2012, even before the last set of detectors was installed, showed a surprisingly large angle, Heeger says. "People thought the angle might be really tiny, so we built an experiment that was 10 times as sensitive as we ended up needing.
"The neutrino community has been waiting for a long time for this parameter, which will be used for planning experiments for next decade and beyond," says Heeger, "and that is why it was recognized by Science."
Source: University of Wisconsin-Madison