The NOvA Neutrino Experiment

The NOvA Neutrino Experiment Follow us on Twitter . Neutrino Oscillation experiment operating between Fermilab in Batavia, IL and Ash River, MN

Please join us in congratulating Linda Cremonesi (Imperial College London, Assoc. Prof of Particle Physics) on becoming ...
04/07/2026

Please join us in congratulating Linda Cremonesi (Imperial College London, Assoc. Prof of Particle Physics) on becoming NOvA's new co-spokesperson. We're excited to welcome Linda into this leadership role and look forward to the insight, energy, and vision she will bring to the collaboration. Congratulations, Linda, and best wishes for the road ahead!

Today we celebrate and thank Tricia Vahle (William & Mary, Prof. of Physics) for 8 years of outstanding stewardship of N...
04/07/2026

Today we celebrate and thank Tricia Vahle (William & Mary, Prof. of Physics) for 8 years of outstanding stewardship of NOvA. Tricia's leadership, dedication, and care for the collaboration have helped shape an important era for the experiment. We are deeply grateful for all she has given to NOvA and the community. Thank you, Tricia!

📸 Prabhjot Singh

Big week for NOvA! We ran a special generator at our Near Detector, flooding it with billions of neutrons. Neutrons are ...
02/11/2026

Big week for NOvA!

We ran a special generator at our Near Detector, flooding it with billions of neutrons. Neutrons are notoriously hard to detect, so this dedicated run will help us better understand how they interact with our detector.

The event display shows the generator position (red ×) and neutron interactions (colored boxes) lighting up the detector. The team shielded our electronics with steel, polyethylene, and water; captured some amazing data!

This work will improve our ability to understand the neutrons produced in neutrino interactions, improving our future analyses.

📸 Taylor Contreras

Using four years of data from the NOvA Near Detector, this paper presents a detailed study of the seasonal variation of ...
01/09/2026

Using four years of data from the NOvA Near Detector, this paper presents a detailed study of the seasonal variation of cosmic-ray–induced multiple-muon events. While single muons show a well-known summer maximum driven by atmospheric temperature effects, multiple-muon events exhibit the opposite behavior, peaking in winter. By combining high-statistics NOvA data with dedicated CORSIKA simulations that include seasonal atmospheric profiles, the study demonstrates that detector size and depth are the key factors governing the observed phase reversal, providing a unified explanation for multiple-muon seasonal behavior across experiments. The result of this study makes it possible for the first time to understand the seasonal variation of observed multiple muon events for a detector of any size and depth.

Read the publication in PRD here: https://journals.aps.org/prd/abstract/10.1103/6djf-6bn5

We have a new article out in PRL describing our most recent three-flavor oscillation analysis with 10 years of NOvA data...
01/08/2026

We have a new article out in PRL describing our most recent three-flavor oscillation analysis with 10 years of NOvA data. This analysis uses double the neutrino-mode dataset of our previous result, an updated simulation, and expands our electron neutrino selection to lower energies

NOvA is now able to determine the atmospheric mass splitting to about 1.5%, marking a major step into a new era of precision neutrino physics. This accuracy enables a novel way to probe which neutrino is the lightest, the "mass ordering", by comparing NOvA’s results with those from reactor-based neutrino experiments. Using this method, NOvA data show an 87% preference for the normal ordering over the inverted ordering.

See the article in PRL here: https://journals.aps.org/prl/abstract/10.1103/x53y-2b86

It's the end of the 2025, which means it is time for us to look back on the year in NOvA's Year In Review!This year we p...
12/31/2025

It's the end of the 2025, which means it is time for us to look back on the year in NOvA's Year In Review!

This year we published four papers, covering new techniques (JINST 20 T02001), cross-section measurements (PRD 111, 052009), sterile neutrino searches (PRL 134, 081804), and a joint analysis of NOvA and T2K data with our friends on T2K (Nature 646, 818–824). You can see these along with all of our other publications on our website: https://novaexperiment.fnal.gov/publications/

We met up for collaboration meetings at University of Wisconsin-Madison in the summer (during national cheese day 🧀 ) and at Fermilab in the fall.

We also had a record-breaking number of successful PhD defenses this year - 13 in total! Congratulations, Doctors! 🎉

We're super excited for next year. See you all in 2026!

We recently combined forces with our friends on the T2K experiment to jointly analyse our data. This initial joint analy...
10/22/2025

We recently combined forces with our friends on the T2K experiment to jointly analyse our data. This initial joint analysis provides some of the most precise neutrino-oscillation measurements in the field. It was published today in Nature.

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’ behavior and properties. The experiments are complementary and provide the power to break degeneracies.

There are three remaining unknowns in the neutrino oscillation puzzle: the mass ordering, whether CP is violated – ie whether neutrinos and antineutrinos behave differently, and the octant of the 23 mixing angle. All of these affect the magnitude and energy dependence of the muon neutrino->electron neutrino appearance oscillation probability, and could affect electron neutrino appearance probability in antineutrinos differently.

NOvA and T2K both measure the appearance probabilities with different baselines and energies. This means the size of the effect of the mass ordering, in particular, is different between the two experiments. This provides one more way to tell the difference between the effects of CP violation and the mass ordering.

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

See the publication here: https://www.nature.com/articles/s41586-025-09599-3

Last week we were spreading nus at the University of Sussex for  . We covered a bunch of topics ---Emerson Bannister (Un...
06/17/2025

Last week we were spreading nus at the University of Sussex for . We covered a bunch of topics ---

Emerson Bannister (University of Sussex) presented on NOvA’s Test Beam programme: https://indico.global/event/14588/contributions/126677/

Thiago Bezerra (University of Sussex) talked about NOvA’s latest three-flavour neutrino oscillation analysis: https://indico.global/event/14588/contributions/126695/

Adam Lister (University of Wisconsin - Madison) gave a talk on NOvA’s searches for Beyond Standard Model physics using neutrino oscillations: https://indico.global/event/14588/contributions/126698/

Alex Booth (Queen Mary University of London) presented on NOvA’s machine learning tools we use for our reconstruction: https://indico.global/event/14588/contributions/126716/

Tyler Horoho (University of Virginia) talked about NOvA’s non-oscillation BSM programme: https://indico.global/event/14588/contributions/126731/

Travis Olson (University of Houston) gave a talk on NOvA’s cross-section measurements: https://indico.global/event/14588/contributions/126730/

We additionally had some great plenary talks from NOvA Spokesperson Patricia Vahle (William & Mary) and Analysis Coordinator Linda Cremonesi (Queen Mary University of London)

📸: Linda Cremonesi, Adam Lister, Josephine Long

Last week we had an awesome time at UW-Madison for our collaboration meeting. We were very lucky to be in the Dairy Stat...
06/09/2025

Last week we had an awesome time at UW-Madison for our collaboration meeting. We were very lucky to be in the Dairy State on National Cheese Day 🧀. Physics + cheese curds, what more could you want?

📸 Sarah Perdue (UW-Madison Physics)

We have a new article out in PRD, a double differential inclusive cross-section measurement using hadronic and leptonic ...
03/28/2025

We have a new article out in PRD, a double differential inclusive cross-section measurement using hadronic and leptonic variables, aimed at isolating the two-particle two-hole (2p2h) process. In 2p2h scattering two nucleons are ejected from the nucleous leaving two "holes" behind.

This paper presents NOvA's first measurement of a cross section in available energy (A proxy for energy transfer), and three-momentum transfer. Energy and momentum transfer are the variables that model builders for the 2p2h process present their work in, and the measurement finds a tension between the measured data and currently available models in GENIE.

See paper here: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.111.052009

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