The 260 members of the NOvA Neutrino Experiment recently reported their initial findings in two papers. The team is trying get a clearer picture of the role neutrinos, mysterious subatomic particles, played in the evolution of the cosmos.
The first paper, in Physical Review Letters, describes the first appearance of electron neutrinos in the NOvA experiment. A second paper, in Physical Review D, describes the disappearance of muon neutrinos in the experiment.
Taken together, the papers offer insights into fundamental neutrino properties such as mass, the way neutrinos oscillate from one type to another, and whether neutrinos are a key to the dominance of matter in the universe.
In a presentation describing the results, physicist Mayly Sanchez clicked to a slide showing the telltale track of an electron neutrino racing through the 14,000-ton Far Detector of the experiment.
Since that detector started full operations in November 2014, two analyses of data from the long-distance experiment have made the first experimental observations of muon neutrinos changing to electron neutrinos.
One analysis found 11 such transitions. Sanchez wrote on her slide, “All 11 of them are absolutely gorgeous.”
How the Experiment Works
NOνA scientists use a 300-ton particle detector at U.S. Department of Energy’s Fermilab near Chicago (the Near Detector) and a 14,000-ton detector in northern Minnesota (the Far Detector) to study neutrino oscillations. The Near Detector sits in a cavern 350 feet underground and measures the composition of the neutrino beam as it leaves the Fermilab site. As they travel straight through the earth, the neutrinos oscillate. The Far Detector records what types of neutrino arrive in Minnesota.
See a time-lapse video of the detector construction below. You can view live data from the experiment here.
Sanchez, an Iowa State University associate professor of physics and astronomy who is also an Intensity Frontier Fellow at Fermilab, is one of the leaders of the NOvA experiment. She serves on the experiment’s executive committee and co-leads the analysis of electron neutrino appearance in the Far Detector.
The paper about electron neutrino appearance reports two, independent analyses of detector data: One found six cases of the muon neutrinos sent to the Far Detector oscillating into electron neutrinos. The other found 11 oscillations. If there were no oscillations, researchers predicted there would be one electron neutrino observed in the Far Detector.
Sanchez says the flickering electron neutrino tracks she helped analyze prove the experiment can do what it was designed to do—spotting and measuring neutrinos after they make the 500-mile, 3-millisecond journey from Fermilab to the Far Detector in northern Minnesota.
The detector is huge: 344,000 plastic cells within a structure 200 feet long, 50 feet high, and 50 feet wide, making it the world’s largest freestanding plastic structure.
“The big news here is we observed electron neutrino appearance,” Sanchez says.
If the calibrations and parameters had been just a little off, “we might not have seen anything,” she says. “When you design an experiment like this, you hope that nature is kind to you and allows you to do a measurement.”
In this case, physicists are detecting and measuring mysterious and lightweight neutrinos. They’re subatomic particles that are among the most abundant in the universe but almost never interact with matter. They’re created in nature by the sun, by collapsing stars, and by cosmic rays interacting with the atmosphere. They’re also created by nuclear reactors and particle accelerators.
There are three types of neutrinos: electron, muon, and tau. As they travel at almost the speed of light, they oscillate from one type to another. Takaaki Kajita of Japan and Arthur B. McDonald of Canada won the 2015 Nobel Prize in Physics for their contributions to the independent, experimental discoveries of neutrino oscillation.
3 Goals of NOvA
The NOvA experiment has three main physics goals: make the first observations of muon neutrinos changing to electron neutrinos, determine the tiny masses of the three neutrino types, and look for clues that help explain how matter came to dominate antimatter in the universe.
At the beginning of the universe, physicists believe there were equal amounts of matter and antimatter. That’s actually a problem because matter and antimatter annihilate each other when they touch.
But the universe still exists. So something happened to throw off that balance and create a universe full of matter. Could it be that neutrinos decayed asymmetrically and tipped the scales toward matter?
The NOvA experiment, as it takes more and more neutrino data, could provide some answers.
Sanchez likes the data she’s seen: “These are absolutely stunning electron neutrino events. We’ve looked at them and they’re textbook perfect—all 11 of them so far.”
This article was originally published by Iowa State University. Republished via Futurity.org under Creative Commons License 4.0.
