Copyright © by the contributing authors, 2007-2024.Ideas, requests, problems regarding Daya Bay? Send feedback
today.
Neutrino studies have now moved from the discovery era to the precision measurement era. It’s important to measure the mixing angle and mass splitting parameters as precisely as possible, because neutrino behavior could hold the key to understanding the asymmetry between matter and antimatter in the universe. This asymmetry, known as the charge-parity or CP violation, explains why shortly after the Big Bang, when most matter and antimatter annihilated each other, some matter was left over to make up the universe we see today.
The Fluctuating Neutrino
The behavior of neutrinos is unlike any other fundamental particle: they seem to disappear, reappear, and transform themselves as they travel, unimpeded, from sources like the sun and other stars, through space, planets, and even our own bodies.
Neutrinos come in three flavors—electron, muon, and tau. And as a neutrino travels, thanks to quantum mechanical fluctuations, it oscillates between flavors. That is, a particle that starts out as an electron neutrino might at some point turn into a tau neutrino. Then at another point it will present itself more like it did in the beginning. As time goes by, these transformations happen again and again, with the oscillation having a particular amplitude and frequency—similar to sound and light waves.
The amplitude of neutrino oscillations gives scientists information about the rate at which neutrinos transform into different flavors, known as the mixing angle. The frequency of the oscillations gives information about the difference between the masses, a property known as mass splitting.
The Neutrino Net
To study neutrino oscillations, the Daya Bay Collaboration has immersed eight detectors in three large underground pools of water. These detectors sit at different distances from the six China General Nuclear Power Group reactors in Daya Bay. The reactors emit steady streams of electron antineutrinos, which for purposes of the experiment are essentially the same as electron neutrinos. The detectors pick up the transformations that occur as these millions of quadrillions of electron antineutrinos travel farther away from their origin in the reactors.
Based on the data collected over 217 days with six of the Daya Bay detectors and 404 days using all eight of the Daya Bay detectors, the research team has determined the value for a specific mixing angle, called theta13 (pronounced theta-one-three), to a precision two times better than previous results. Similar improvement was made in the precision of measuring the mass splitting. These measurements support the three-neutrino model, which describes physicists’ best thinking about the three types of neutrinos.
The Daya Bay Collaboration continues to take data. At the end of 2017 it will have roughly four times more data to further improve precision for both mixing angle of theta13 and corresponding mass splitting. By then, all three mixing angles (including theta12 and theta23) and mass splittings may be determined to comparable precisions, better than three percent.
The unprecedented precision of the data set allows for many other studies. The team is looking for evidence of a possible “sterile” neutrino, a hypothetical type that may mix with the three known neutrino flavors. If this sterile neutrino shows itself in the data, scientists will need to rethink the three-neutrino model. In addition, the record-breaking data sample is ideal for finding new physics beyond what are known.
2015-09-11
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Copyright © by the contributing authors, 2007-2024. Ideas, requests, problems regarding Daya Bay? Send feedback |