Scarcity of anti-matter in universe explained
Scientists have 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, anti-matter.india Updated: Dec 31, 2012 19:19 IST
The particles, called anti-neutrinos, were detected at the underground Daya Bay experiment, located near a nuclear reactor in China, 55 kilometers north of Hong Kong.
For the measurement of anti-neutrinos it made in 2012, the Daya Bay collaboration has been named runner-up for breakthrough of the year from Science magazine.
Anti-particles are almost identical twins of sub-atomic particles (electrons, protons and neutrons) that make up our world. When an electron encounters an anti-electron, for example, both are annihilated in a burst of energy. Failure to see these bursts in the universe tells physicists that anti-matter 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 anti-particles was created, but somehow an imbalance came about,” said Karsten Heeger, a professor of physics at the University of Wisconsin-Madison.
“All the studies that have been done have not found enough difference between particles and anti-particles to explain the dominance of matter over anti-matter,” he noted.
But the neutrino, an extremely abundant but almost massless particle, may have the right properties, and may even be its own anti-particle. And that’s why physicists have put their last hope on the neutrino to explain the absence of anti-matter in the universe,” Heeger said.
Heeger and his group at UW-Madison have been responsible for much of the design and development of the anti-neutrino 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 anti-neutrino detectors.
Reactors, Heeger said, are a fertile source of anti-neutrinos, 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 stated.
“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,” said Heeger, “and that is why it was recognized by Science.”