{"id":22998,"date":"2025-10-22T11:15:46","date_gmt":"2025-10-22T15:15:46","guid":{"rendered":"https:\/\/www.yorku.ca\/news\/?p=22998"},"modified":"2025-10-23T15:50:43","modified_gmt":"2025-10-23T19:50:43","slug":"rival-neutrino-experiments-nova-and-t2k-publish-first-joint-analysis","status":"publish","type":"post","link":"https:\/\/www.yorku.ca\/news\/2025\/10\/22\/rival-neutrino-experiments-nova-and-t2k-publish-first-joint-analysis\/","title":{"rendered":"'Rival' neutrino experiments NOvA and T2K publish first joint analysis"},"content":{"rendered":"
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The combined results add to physicists\u2019 understanding and they validate the impressive collaborative effort <\/em>
between two competing \u2014 yet complementary \u2014 experiments<\/em>.<\/p>\n\n\n\n

TORONTO, Oct. 22, 2025<\/strong> \u2013 The Tokai to Kamioka<\/a> (T2K) experiment in Japan and the NuMI Off-axis \u03bde<\/sub> Appearance<\/a> (NOvA) experiment in the United States, previously considered rival experiments, conducted a joint analysis and published their first results today in the journal Nature<\/a><\/em>.<\/p>\n\n\n\n

Both are long-baseline neutrino oscillation experiments using accelerators, and by leveraging their different baselines and neutrino energies, they achieved precision measurements of neutrino oscillations.<\/p>\n\n\n\n

Neutrinos are subatomic particles that are neutral and weigh almost nothing, and almost never interact with the matter around them, making them notoriously hard to study. However, they may hold the secret to why the universe is now filled with matter and light. Everything known about particle physics tells scientists that when the universe began there were equal amounts of matter and antimatter, which when they collide, annihilate to form light.<\/p>\n\n\n

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Deborah Harris<\/figcaption><\/figure>\n<\/div>\n\n\n

\u201cIf matter and antimatter behave identically, then the universe now should hold nothing but light.\u00a0 Something must have tipped the balance to favour matter over antimatter, and all the other particles we have studied till now cannot tip this balance. It is possible that neutrinos may be what tipped that balance, so the field is trying as hard as it can to see if neutrinos and antineutrinos behave differently from each other,\u201d says York University Professor Deborah Harris<\/strong><\/a>.<\/p>\n\n\n\n

Harris, a particle physicist in the Department of Physics and Astronomy, Faculty of Science, is an active member of the large research collaboration T2K.  She also collaborates on a next generation neutrino oscillation experiment aiming to measure oscillations with even more precision, called the Deep Underground Neutrino Experiment (DUNE), and is a senior scientist at Fermi National Accelerator Laboratory in the United States. <\/p>\n\n\n\n

The combined efforts of T2K and NOvA succeeded in reducing the uncertainty in the differences between neutrino masses to below two per cent. Although the ordering of the three neutrino masses is still unknown, their results show that depending on this ordering, the magnitude of CP symmetry violation \u2013 a difference in behaviour between particles and antiparticles \u2013 would be strongly constrained.<\/p>\n\n\n\n

This achievement marks an important step toward uncovering CP symmetry violation in neutrinos and the origin of the matter\u2013antimatter asymmetry in the universe. The joint analysis combined 10 years of T2K data collected since 2010 and six years of NOvA data collected since 2014, and it also demonstrates the strength of collaboration between two international experiments that are competitive yet complementary.<\/p>\n\n\n\n

\u201cThis combination does not yet see a definitive difference between neutrinos and antineutrinos but by combining the two experiment\u2019s data we know much more about neutrinos than either experiment can tell us by itself,\u201d says Harris.<\/p>\n\n\n\n

York University researchers have been an important part of T2K since its inception and contributed the critical Optical Transition Radiation Detector in the beamline. These researchers include Professor Sampa Bhadra and postdoctoral Fellows Dr. No\u00eb Roy and Dr. Arturo Fiorentini, and former PhD students Dr. Rowan Zaki and Dr. Mitchell Yu.    <\/p>\n\n\n

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Fig. 1 : T2K in Japan (left) and NOvA in the United States (right) are both long-baseline experiments: they each shoot an intense beam of neutrinos that passes through both a near detector close to the neutrino source and a far detector hundreds of kilometers away. Both experiments compare data recorded in each detector to learn about neutrinos\u2019 behavior and properties.<\/em> Credit: T2K and NOvA collaborations<\/em><\/figcaption><\/figure>\n<\/div>\n\n\n

Context<\/h2>\n\n\n\n

When the universe began, physicists expect there should have been equal amounts of matter and antimatter. But if that were so, the matter and antimatter should have perfectly canceled each other out, resulting in total annihilation.<\/p>\n\n\n\n

And yet, here we are. Somehow, matter won out over antimatter \u2014 but we still don\u2019t know how or why.<\/p>\n\n\n\n

Physicists suspect the answer may lie in the mysterious behaviour of abundant yet elusive particles called neutrinos. Specifically, learning more about a phenomenon called neutrino oscillation \u2014 in which neutrinos change types, or flavours, as they travel \u2014 could bring us closer to an answer.<\/p>\n\n\n\n

The international collaborations representing two neutrino experiments, T2K in Japan and NOvA in the United States<\/a>, recently combined forces to produce their first joint results, published today in the journal Nature. This initial joint analysis provides some of the most precise neutrino-oscillation measurements in the field.<\/p>\n\n\n\n

\u201cThese results are an outcome of a cooperation and mutual understanding of two unique collaborations, both involving many experts in neutrino physics, detection technologies and analysis techniques, working in very different environments, using different methods and tools,\u201d says T2K collaborator Tom\u00e1\u0161 Nosek.<\/p>\n\n\n\n

Different experiments, common goals<\/h2>\n\n\n\n

Despite their ubiquity, neutrinos are very difficult to detect and study. Even though they were first seen in the 1950s, the ghostly particles remain deeply enigmatic. Filling in gaps in our knowledge about neutrinos and their properties may reveal fundamental truths about the universe.<\/p>\n\n\n\n

T2K and NOvA are both long-baseline experiments: they each shoot an intense beam of neutrinos that passes through both a near detector close to the neutrino source and a far detector hundreds of miles away. Both experiments compare data recorded in each detector to learn about neutrinos\u2019 behaviour and properties.<\/p>\n\n\n

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The NOvA Neutrino Experiment far detector at Ash River, Minnesota
Credit: Reidar Hahn, Fermilab<\/figcaption><\/figure>\n<\/div>\n\n\n

NOvA, the NuMI Off-axis \u03bde<\/sub> Appearance experiment, sends a beam of neutrinos 810 kilometers from its source at the U.S. Department of Energy\u2019s Fermi National Accelerator Laboratory near Chicago, Ill., to a 14,000-ton liquid-scintillator detector in Ash River, Minnesota.<\/p>\n\n\n\n

The T2K experiment\u2019s neutrino beam travels 295 kilometers from Tokai to Kamioka \u2014 hence the name T2K. Tokai is home to the Japan Proton Accelerator Research Complex (J-PARC) and Kamioka hosts the Super-Kamiokande neutrino detector, an enormous tank of ultrapure water located a kilometer underground.<\/p>\n\n\n\n

Since the experiments have similar science goals but different baselines and different neutrino energies, physicists can learn more by combining their data.<\/p>\n\n\n\n

\u201cBy making a joint analysis you can get a more precise measurement than each experiment can produce alone,\u201d says NOvA collaborator Liudmila Kolupaeva. \u201cAs a rule, experiments in high-energy physics have different designs even if they have the same science goal. Joint analyses allow us to use complementary features of these designs.\u201d<\/p>\n\n\n\n

As long-baseline experiments, NOvA and T2K are ideal for studying neutrino oscillations, a phenomenon that can provide insight into open questions like charge-parity violation and the neutrino mass ordering. Two experiments with different baselines and energies have a better chance of disentangling the two effects than one experiment alone.<\/p>\n\n\n

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\"The
The members of the T2K collaboration. Credit: The T2K Collaboration<\/figcaption><\/figure>\n<\/div>\n\n\n

Interrogating neutrino oscillations<\/h2>\n\n\n\n

The mystery of neutrino mass ordering is the question of which neutrino is the lightest. But it isn\u2019t as simple as placing particles on a scale. Neutrinos have miniscule masses that are made up of combinations of mass states. There are three neutrino mass states, but, confusingly, they don\u2019t map to the three neutrino flavours. In fact, each flavour is made of a mix of the three mass states, and each mass state has a different probability of acting like each flavour of neutrino.<\/p>\n\n\n\n

There are two possible mass orderings, called normal or inverted. Under the normal ordering, two of the mass states are relatively light and one is heavy, while the inverted ordering has two heavier mass states and one light.<\/p>\n\n\n\n

In the normal ordering, there is an enhanced probability that muon neutrinos will oscillate to electron neutrinos but a lower probability that muon antineutrinos will oscillate to electron antineutrinos. In the inverted ordering, the opposite happens. However, an asymmetry in the neutrinos\u2019 and antineutrinos\u2019 oscillations could also be explained if neutrinos violate CP symmetry \u2014 in other words, if neutrinos don\u2019t behave the same as their antimatter counterparts.<\/p>\n\n\n

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The members of the NOvA collaboration gathered at Fermilab. Credit: Fermilab Communications Office<\/figcaption><\/figure>\n<\/div>\n\n\n

The combined results of NOvA and T2K do not favour either mass ordering. If the neutrino mass ordering is found to be normal, NOvA\u2019s and T2K\u2019s results are less clear on CP symmetry, requiring additional data to clarify. However, if future results show the neutrino mass ordering is inverted, the results published today provide evidence that neutrinos violate CP symmetry, potentially explaining why the universe is dominated by matter instead of antimatter.<\/p>\n\n\n\n

\u201cNeutrino physics is a strange field. It is very challenging to isolate effects,\u201d says Kendall Mahn, co-spokesperson for T2K. \u201cCombining analyses allows us to isolate one of these effects, and that\u2019s progress.\u201d<\/p>\n\n\n\n

The combined analysis does provide one of the most precise values of the difference in mass between neutrino mass states, a quantity called \u0394m2<\/sup>32<\/sub>. With an uncertainty below two per cent, the new value will enable physicists to make precision comparisons with other neutrino experiments to test whether the neutrino oscillation theory is complete.<\/p>\n\n\n\n

What\u2019s next<\/h2>\n\n\n\n

These first joint results do not definitively solve any mysteries of neutrinos, but they do add to physicists\u2019 knowledge about the particles. Plus, they validate the impressive collaborative effort between two competing \u2014 yet complementary \u2014 experiments.<\/p>\n\n\n\n

The NOvA collaboration consists of more than 250 scientists and engineers from 49 institutions in eight countries. The T2K collaboration has more than 560 members from 75 institutions in 15 countries. The two collaborations began active work on this joint analysis in 2019. It combines six years of data from NOvA, which began collecting data in 2014, and a decade of data from T2K, which started up in 2010.\u00a0 Both experiments continue to take data, and efforts are already underway to update the joint analysis with the new data.<\/p>\n\n\n\n

\u201cThe joint analysis work has benefited both collaborations,\u201d says Patricia Vahle, co-spokesperson for NOvA. \u201cWe have a much better mutual understanding of the strengths and challenges of the different experimental setups and analysis techniques.\u201d<\/p>\n\n\n\n

NOvA and T2K are the only currently operating long-baseline neutrino experiments. Their initial combined results lay a foundation for forthcoming neutrino experiments that will answer the questions around neutrinos unambiguously.<\/p>\n\n\n\n

The Fermilab led Deep Underground Neutrino Experiment is under construction in Illinois and South Dakota in the U.S. With its longer baseline of 1,300 kilometers, DUNE will be more sensitive to neutrino mass ordering and could give physicists a conclusive answer shortly after it turns on in the early years of the next decade.<\/p>\n\n\n\n

In Japan, Hyper-Kamiokande, the successor to Super-Kamiokande, is currently under construction in an underground mine in Kamioka, Hida City, Gifu Prefecture, with experiments scheduled to begin in 2028. Hyper-Kamiokande will conduct highly sensitive searches for CP symmetry violation through high-statistics measurements made possible by a detector about eight times larger and an intense neutrino beam.<\/p>\n\n\n\n

Many physicists hope these next-generation neutrino experiments can come together \u2014 as NOvA and T2K have already done \u2014 to make progress on their shared scientific goals to learn more about neutrinos and their unusual properties.<\/p>\n\n\n\n

\u201cAs shown in this very analysis, there are no truly \u2018rivaling\u2019 experiments because they all share a common goal of scientific study of a phenomenon,\u201d says Nosek. \u201cCollaborating is naturally important for the transfer of knowledge, know-how and experience, and for sharing resources, ideas and tools. The T2K-NOvA collaboration is not merely a sum of T2K and NOvA collaborations. It is much, much more.\u201d<\/p>\n\n\n