P. Adamson’s research while affiliated with Fermi National Accelerator Laboratory (Fermilab) and other places

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Publications (200)


FIG. 1. Flux of ν μ neutrinos at the NOvA Near Detector (solid histogram) shown with the total 1-σ uncertainty (shaded band) [46].
FIG. 14. The estimated 2p2h cross section of Fig. 13 displayed in bins of E avail for six contiguous slices of j⃗ qj.
Measurement of d 2 σ / d | q → | d E avail in charged current ν μ -nucleus interactions at ⟨ E ν ⟩ = 1.86 GeV using the NOvA Near Detector
  • Article
  • Full-text available

March 2025

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23 Reads

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1 Citation

Physical Review D

M. A. Acero

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B. Acharya

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P. Adamson

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[...]

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R. Zwaska

Double- and single-differential cross sections for inclusive charged-current ν μ -nucleus scattering are reported for the kinematic domain 0 to 2 GeV / c in three-momentum transfer and 0 to 2 GeV in available energy, at a mean ν μ energy of 1.86 GeV. The measurements are based on an estimated 995,760 ν μ charged-current (CC) interactions in the scintillator medium of the NOvA Near Detector. The subdomain populated by 2-particle-2-hole (2p2h) reactions is identified by the cross section excess relative to predictions for ν μ -nucleus scattering that are constrained by a data control sample. Models for 2-particle-2-hole processes are rated by χ 2 comparisons of the predicted-versus-measured ν μ CC inclusive cross section over the full phase space and in the restricted subdomain. Shortfalls are observed in neutrino generator predictions obtained using the theory-based València and SuSAv2 2p2h models. Published by the American Physical Society 2025

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Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA

February 2025

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20 Reads

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2 Citations

Physical Review Letters

We report a search for neutrino oscillations to sterile neutrinos under a model with three active and one sterile neutrinos ( 3 + 1 model). This analysis uses the NOvA detectors exposed to the NuMI beam, running in neutrino mode. The data exposure, 13.6 × 10 20 protons on target, doubles that previously analyzed by NOvA, and the analysis is the first to use ν μ charged-current interactions in conjunction with neutral-current interactions. Neutrino samples in the near and far detectors are fitted simultaneously, enabling the search to be carried out over a Δ m 41 2 range extending 2 (3) orders of magnitude above (below) 1 eV 2 . NOvA finds no evidence for active-to-sterile neutrino oscillations under the 3 + 1 model at 90% confidence level. New limits are reported in multiple regions of parameter space, excluding some regions currently allowed by IceCube at 90% confidence level. We additionally set the most stringent limits for anomalous ν τ appearance for Δ m 41 2 ≤ 3 eV 2 . Published by the American Physical Society 2025


Monte Carlo method for constructing confidence intervals with unconstrained and constrained nuisance parameters in the NOvA experiment

February 2025

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29 Reads

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1 Citation

Journal of Instrumentation

Measuring observables to constrain models using maximum-likelihood estimation is fundamental to many physics experiments. Wilks' theorem provides a simple way to construct confidence intervals on model parameters, but it only applies under certain conditions. These conditions, such as nested hypotheses and unbounded parameters, are often violated in neutrino oscillation measurements and other experimental scenarios. Monte Carlo methods can address these issues, albeit at increased computational cost. In the presence of nuisance parameters, however, the best way to implement a Monte Carlo method is ambiguous. This paper documents the method selected by the NOvA experiment, the profile construction. It presents the toy studies that informed the choice of method, details of its implementation, and tests performed to validate it. It also includes some practical considerations which may be of use to others choosing to use the profile construction.


Search for C P -Violating Neutrino Nonstandard Interactions with the NOvA Experiment

November 2024

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48 Reads

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4 Citations

Physical Review Letters

This Letter reports a search for charge-parity ( C P ) symmetry violating nonstandard interactions (NSI) of neutrinos with matter using the NOvA Experiment, and examines their effects on the determination of the standard oscillation parameters. Data from ν μ ( ν ¯ μ ) → ν μ ( ν ¯ μ ) and ν μ ( ν ¯ μ ) → ν e ( ν ¯ e ) oscillation channels are used to measure the effect of the NSI parameters ϵ e μ and ϵ e τ . With 90% CL the magnitudes of the NSI couplings are constrained to be | ϵ e μ | ≲ 0.3 and | ϵ e τ | ≲ 0.4 . A degeneracy at | ϵ e τ | ≈ 1.8 is reported, and we observe that the presence of NSI limits sensitivity to the standard C P phase δ C P . Published by the American Physical Society 2024


Figure 1. Event yield per number of tracks divided by neutrino interaction types in the muon-neutrino CC sample.
Figure 5. Efficiency distributions for each cos θµ slice. The values decrease as the muon kinetic energy increases. Conversely, the efficiency increases as more forward-going muons are selected. This pattern results from the containment requirement.
Measurement of the double-differential cross section of muon-neutrino charged-current interactions with low hadronic energy in the NOvA Near Detector

October 2024

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40 Reads

The NOvA collaboration reports cross-section measurements for νμ\nu_{\mu} charged-current interactions with low hadronic energy (maximum kinetic energy of 250 MeV for protons and 175 MeV for pions) in the NOvA Near Detector. The results are presented as a double-differential cross section as a function of the direct observables of the final-state muon kinematics. Results are also presented as a single-differential cross section as a function of the derived square of the four-momentum transfer, Q2Q^{2}, and as a function of the derived neutrino energy. The data correspond to an accumulated 8.09×1020\times10^{20} protons-on-target (POT) in the neutrino mode of the NuMI beam, with a narrow band of neutrino energies peaked at 1.8 GeV. The analysis provides a sample of neutrino-nucleus interactions with an enhanced fraction of quasi-elastic and two-particle-two-hole (2p2h) interactions. This enhancement allows quantitative comparisons with various nuclear models. We find strong disagreement between data and theory-based models in various regions of the muon kinematic phase space, especially in the forward muon direction.


Measurement of d2sigma/d|q|dEavail in charged current neutrino-nucleus interactions at = 1.86 GeV using the NOvA Near Detector

October 2024

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50 Reads

Double- and single-differential cross sections for inclusive charged-current neutrino-nucleus scattering are reported for the kinematic domain 0 to 2 GeV/c in three-momentum transfer and 0 to 2 GeV in available energy, at a mean muon-neutrino energy of 1.86 GeV. The measurements are based on an estimated 995,760 muon-neutrino CC interactions in the scintillator medium of the NOvA Near Detector. The subdomain populated by 2-particle-2-hole reactions is identified by the cross-section excess relative to predictions for neutrino-nucleus scattering that are constrained by a data control sample. Models for 2-particle-2- hole processes are rated by chi-square comparisons of the predicted-versus-measured muon-neutrino CC inclusive cross section over the full phase space and in the restricted subdomain. Shortfalls are observed in neutrino generator predictions obtained using the theory-based Val`encia and SuSAv2 2p2h models.


Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA

September 2024

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50 Reads

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1 Citation

We report a search for neutrino oscillations to sterile neutrinos under a model with three active and one sterile neutrinos (3+1 model). This analysis uses the NOvA detectors exposed to the NuMI beam, running in neutrino mode. The data exposure, 13.6e20 protons on target, doubles that previously analyzed by NOvA, and the analysis is the first to use νμ\nu_{\mu} charged-current interactions in conjunction with neutral-current interactions. Neutrino samples in the Near and Far detectors are fitted simultaneously, enabling the search to be carried out over a Δm412\Delta m^2_{41} range extending 2 (3) orders of magnitude above (below) 1 eV2^2. NOvA finds no evidence for active-to-sterile neutrino oscillations under the 3+1 model at 90% confidence level. New limits are reported in multiple regions of parameter space, excluding some regions currently allowed by IceCube at 90% confidence level. We additionally set the most stringent limits for anomalous ντ\nu_{\tau} appearance for Δm4123\Delta m^{2}_{41} \le 3 eV2^2.


Expanding neutrino oscillation parameter measurements in NOvA using a Bayesian approach

July 2024

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103 Reads

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14 Citations

Physical Review D

NOvA is a long-baseline neutrino oscillation experiment that measures oscillations in charged-current ν μ → ν μ (disappearance) and ν μ → ν e (appearance) channels, and their antineutrino counterparts, using neutrinos of energies around 2 GeV over a distance of 810 km. In this work we reanalyze the dataset first examined in our previous paper [] using an alternative statistical approach based on Bayesian Markov chain Monte Carlo. We measure oscillation parameters consistent with the previous results. We also extend our inferences to include the first NOvA measurements of the reactor mixing angle θ 13 , where we find 0.071 ≤ sin 2 2 θ 13 ≤ 0.107 , and the Jarlskog invariant, where we observe no significant preference for the C P -conserving value J = 0 over values favoring C P violation. We use these results to examine the effects of constraints from short-baseline measurements of θ 13 using antineutrinos from nuclear reactors when making NOvA measurements of θ 23 . Our long-baseline measurement of θ 13 is shown to be consistent with the reactor measurements, supporting the general applicability and robustness of the Pontecorvo-Maki-Nakagawa-Sakata framework for neutrino oscillations. Published by the American Physical Society 2024


FIG. 1. An example simulated ND event. The overhead view (top) of the particle tracks in the detector and (bottom) the side view of the same tracks. In each view, a small white box shows the vertex region, with a magnified version shown in a large white box. Individual detector cells with recorded energy depositions are shown as colored rectangles, with the size and color of the rectangle related to the amplitude of the detected signal. The beam enters the detector from the left. The μ − is seen as the long, forward-directed track. In the side view (bottom), two photons from a π 0 decay are visible. In the overhead view (top), one of the decay photons is unseen as its highly transverse trajectory stayed within a single yz detector plane.
FIG. 4. Comparison of the data and simulation of the convolutional neural-network-based CVNν μ particle ID. Backgrounds are indicated as shaded subsets of the total. The unshaded portion of the histogram represents ν μ CC events. Note that the CCπ 0 signal is a subset of the unshaded portion of the histogram.
FIG. 8. A comparison of the Ashery et al. [41] and DUET [40] measurements of the π þ → π 0 CX cross section and the spread in cross section of the NOvA simulation consistent with these results. A 68.3% confidence interval for the range of scale factors applied to the nominal simulation was calculated as 1.061 AE 0.146 from a fit to the DUET data.
Measurement of ν μ charged-current inclusive π 0 production in the NOvA near detector

June 2023

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166 Reads

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7 Citations

Physical Review D

Cross sections for the interaction νμA→μ−π0X with neutrino energies between 1 and 5 GeV are measured using a sample of 165,000 selected events collected in the NOvA experiment’s near detector, a hydrocarbon-based detector exposed to the Neutrinos from the Main Injector beam at the Fermi National Accelerator Laboratory. Results are presented as a flux-averaged total cross section and as differential cross sections in the momenta and angles of the outgoing muon and π0, the total four-momentum transfer, and the invariant mass of the hadronic system. Comparisons are made with predictions from a reference version of the genie neutrino interaction generator. The measured total cross section of (3.57±0.44)×10−39 cm2 is 7.5% higher than the genie prediction, but is consistent within experimental errors.


Measurement of the double-differential muon-neutrino charged-current inclusive cross section in the NOvA near detector

March 2023

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96 Reads

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17 Citations

Physical Review D

We report cross-section measurements of the final-state muon kinematics for νμ charged-current interactions in the NOvA near detector using an accumulated 8.09×1020 protons on target in the NuMI beam. We present the results as a double-differential cross section in the observed outgoing muon energy and angle, as well as single-differential cross sections in the derived neutrino energy, Eν, and square of the four-momentum transfer, Q2. We compare the results to inclusive cross-section predictions from various neutrino event generators via χ2 calculations using a covariance matrix that accounts for bin-to-bin correlations of systematic uncertainties. These comparisons show a clear discrepancy between the data and each of the tested predictions at forward muon angle and low Q2, indicating a missing suppression of the cross section in current neutrino-nucleus scattering models.


Citations (75)


... Neutrino interaction models consistently show discrepancies when compared to NOvA data [43][44][45][46], mirroring challenges seen in other experiments. Historically, the experiment has relied on GENIE as the default event generator [47], tuned through targeted modifications informed by theoretical advancements, external data constraints, and ND observations, in order to refine the modeling of the different neutrino-nucleus reaction mechanisms. ...

Reference:

Neutrino Scattering: Connections Across Theory and Experiment
Measurement of d 2 σ / d | q → | d E avail in charged current ν μ -nucleus interactions at ⟨ E ν ⟩ = 1.86 GeV using the NOvA Near Detector

Physical Review D

... In the Standard Model, there are in general two types of axial-vector FFs of a hadron in the weak sector: the weak-charged ones via the weak-charged current interactions mediated by the W ± bosons, and the weakneutral ones via the weak-neutral current interactions mediated by the Z 0 bosons. These axial-vector FFs also serve as important quantities for constraining the systematic uncertainties of high-precision measurements in (anti)neutrino oscillation experiments [23][24][25][26][27][28][29][30][31]. On the theory side, tremendous progress has been reported in the last few years from the first-principle lattice QCD side ; theoretical evaluations of the nucleon axial-vector FFs and their contributions to the associated cross sections based on chiral perturbation theory and various models/approaches are still rapidly developing . ...

Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA

Physical Review Letters

... The 2D contours in the (γ 2 , E b ) space are obtained following the profiled Feldman-Cousins approach [22], treating ϕ and γ 1 as nuisance parameters. The 1D intervals on γ 2 and E b are computed with a similar procedure, treating also E b or Each row corresponds to one specific fit. ...

Monte Carlo method for constructing confidence intervals with unconstrained and constrained nuisance parameters in the NOvA experiment
  • Citing Article
  • February 2025

Journal of Instrumentation

... In reference [32], the authors discuss constraining SNSI at DUNE, further pointing out that the absolute neutrino mass can also be constrained in the presence of SNSI. Reference [70] explores distinguishing different new physics scenarios, including sterile neutrinos and vector and scalar NSI at NOνA (NuMI Off-axis ν e Appearance) [84,85], T2K (Tokai to Kamioka) [86], and DUNE. SNSI using ν(ν)-disappearance in oscillation data across various experiments is analyzed in [33]. ...

First measurement of electron neutrino appearance in NOvA
  • Citing Preprint
  • January 2016

... Interestingly they see a closed contour at 95% CL in sin 2 2θ 24 − ∆m 2 41 plane, centered at sin 2 2θ 24 = 0.16 and ∆m 2 41 = 3.5 eV 2 , which may drop hints about possible structure. This feature certainly motivated us to pursue this investigation, although it is in tension with the results from the other experiments, such as MINOS+ [49]. In this paper we aim at providing a hopefully comprehensive, bird-eye view of such resonance in the (3 + 1) model. ...

Search for sterile neutrinos in MINOS and MINOS+ using a two-detector fit

... Figure 14 presents a summary of the reported allowed regions at 90% CL of the NSI couplings, where the off-diagonal elements have been assumed real-valued with δ αβ = 0 or π for comparison. The results of IC-DeepCore 2021 [46], MINOS 2013 [47] and NOvA 2024 [48] were re-scaled to match the NSI down-quark coupling convention used in this study (see eq. (1.3)). ...

Search for C P -Violating Neutrino Nonstandard Interactions with the NOvA Experiment

Physical Review Letters

... FFs also serve as important quantities for constraining the systematic uncertainties of highprecision measurements in (anti)neutrino oscillation experiments [23][24][25][26][27][28][29][30][31]. On the theory side, tremendous progress has been reported in the last few years from the first-principle lattice QCD side ; theoretical evaluations of the nucleon axial-vector FFs and their contributions to the associated cross sections based on chiral perturbation theory and various models/approaches are still rapidly developing . ...

Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA

... Providing those answers, with the determination of the neutrino mass ordering by clarifying the sign of ∆m 2 31 and the precise measurement of the δ CP -phase to investigate the presence of CP violation in the leptonic sector, would open a way to explore new physics. While the quark mixing matrix has been extensively tested with robust precision, the unitarity of the PMNS matrix, assumed in many oscillation analyses [4,5], still has to be experimentally proven. Under the PMNS matrix unitarity hypothesis, solar [6,7], reactor [8][9][10][11], and atmospheric [1,12,13] neutrino experiments mostly exploited the ν e ,ν e , and ν µ ,ν µ disappearance channels, whereas the high-statistics in ν e andν e appearance channels have been investigated in long-baseline accelerator experiments [4,5]. ...

Expanding neutrino oscillation parameter measurements in NOvA using a Bayesian approach

Physical Review D

... Therefore, θ Adt , being a hadronic variable in the Adler frame, is influenced by both IS and FSI. Additionally, the necessity of reconstructing the neutrino energy renders θ Adt sensitive to neutrino flux uncertainties, which are among the largest systematic uncertainties in neutrino measurements [24][25][26][27][28]. ...

Measurement of ν μ charged-current inclusive π 0 production in the NOvA near detector

Physical Review D

... In this work, we will continue these previous analyses by testing the full SuSAv2 model with CC-inclusive MicroBooNE [56,57] and NOvA [6,58] data on different targets. The contributions considered for the different nuclear reaction channels in Sec. ...

Measurement of the double-differential muon-neutrino charged-current inclusive cross section in the NOvA near detector

Physical Review D