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Search for CP-violating Neutrino Non-Standard Interactions with the NOvA Experiment
Authors:
NOvA Collaboration,
M. A. Acero,
B. Acharya,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
N. Balashov,
P. Baldi,
B. A. Bambah,
A. Bat,
K. Bays,
R. Bernstein,
T. J. C. Bezerra,
V. Bhatnagar,
D. Bhattarai,
B. Bhuyan,
J. Bian,
A. C. Booth,
R. Bowles,
B. Brahma
, et al. (182 additional authors not shown)
Abstract:
This Letter reports a search for charge-parity (CP) symmetry violating non-standard interactions (NSI) of neutrinos with matter using the NOvA Experiment, and examines their effects on the determination of the standard oscillation parameters. Data from $ν_μ(\barν_μ)\rightarrowν_μ(\barν_μ)$ and $ν_μ(\barν_μ)\rightarrowν_{e}(\barν_{e})$ oscillation channels are used to measure the effect of the NSI…
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This Letter reports a search for charge-parity (CP) symmetry violating non-standard interactions (NSI) of neutrinos with matter using the NOvA Experiment, and examines their effects on the determination of the standard oscillation parameters. Data from $ν_μ(\barν_μ)\rightarrowν_μ(\barν_μ)$ and $ν_μ(\barν_μ)\rightarrowν_{e}(\barν_{e})$ oscillation channels are used to measure the effect of the NSI parameters $\varepsilon_{eμ}$ and $\varepsilon_{eτ}$. With 90% C.L. the magnitudes of the NSI couplings are constrained to be $|\varepsilon_{eμ}| \, \lesssim 0.3$ and $|\varepsilon_{eτ}| \, \lesssim 0.4$. A degeneracy at $|\varepsilon_{eτ}| \, \approx 1.8$ is reported, and we observe that the presence of NSI limits sensitivity to the standard CP phase $δ_{\tiny\text{CP}}$.
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Submitted 11 March, 2024;
originally announced March 2024.
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Expanding neutrino oscillation parameter measurements in NOvA using a Bayesian approach
Authors:
NOvA Collaboration,
M. A. Acero,
B. Acharya,
P. Adamson,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
N. Balashov,
P. Baldi,
B. A. Bambah,
A. Bat,
K. Bays,
R. Bernstein,
T. J. C. Bezerra,
V. Bhatnagar,
D. Bhattarai,
B. Bhuyan,
J. Bian,
A. C. Booth,
R. Bowles,
B. Brahma,
C. Bromberg
, et al. (174 additional authors not shown)
Abstract:
NOvA is a long-baseline neutrino oscillation experiment that measures oscillations in charged-current $ν_μ \rightarrow ν_μ$ (disappearance) and $ν_μ \rightarrow ν_{e}$ (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 [Phys. Rev. D 106, 032004 (20…
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NOvA is a long-baseline neutrino oscillation experiment that measures oscillations in charged-current $ν_μ \rightarrow ν_μ$ (disappearance) and $ν_μ \rightarrow ν_{e}$ (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 [Phys. Rev. D 106, 032004 (2022)] 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 $θ_{13}$ and the Jarlskog invariant. We use these results to quantify the strength of our inferences about CP violation, as well as 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 also shown to be consistent with the reactor measurements, supporting the general applicability and robustness of the PMNS framework for neutrino oscillations.
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Submitted 16 November, 2023; v1 submitted 13 November, 2023;
originally announced November 2023.
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Uniform Distribution Technique for Neutrino Beam Scan Simulation
Authors:
D. A. Wickremasinghe,
S. Ganguly,
K. Yonehara,
R. Zwaska,
P. Snopok,
Y. Yu
Abstract:
In Fermilab's neutrino facilities such as the Neutrinos at the Main Injector (NuMI) and the upcoming Long Baseline Neutrino Facility (LBNF), a proton beam strikes high-power target, producing positively and negatively charged pions and kaons. There is a need for detailed simulations in order to capture all particle interactions and beam propagation from protons on target to short-lived mesons deca…
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In Fermilab's neutrino facilities such as the Neutrinos at the Main Injector (NuMI) and the upcoming Long Baseline Neutrino Facility (LBNF), a proton beam strikes high-power target, producing positively and negatively charged pions and kaons. There is a need for detailed simulations in order to capture all particle interactions and beam propagation from protons on target to short-lived mesons decaying into muons and neutrinos. The generation of individual beam simulations is a resource-intensive and time-consuming process. In this paper, we describe a method through which many simulation samples with high statistics can be generated to study the effects of beam scan across a target for given beam configurations.
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Submitted 23 January, 2024; v1 submitted 14 September, 2023;
originally announced September 2023.
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Exploring the Focusing Mechanism of the NuMI Horn Magnets
Authors:
Katsuya Yonehara,
Sudeshna Ganguly,
Don Athula Wickremasinghe,
Pavel Snopok,
Yiding Yu
Abstract:
Neutrinos at the Main Injector (NuMI) is a project at Fermilab that provides an intense beam of neutrinos used by a number of experiments. NuMI creates a beam of pions that decay into neutrinos, muons, and other particles. Muons are registered by the muon monitors. Magnetic horns are the key elements of the NuMI beam line. This paper uses the muon beam profile observed at the muon monitors to stud…
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Neutrinos at the Main Injector (NuMI) is a project at Fermilab that provides an intense beam of neutrinos used by a number of experiments. NuMI creates a beam of pions that decay into neutrinos, muons, and other particles. Muons are registered by the muon monitors. Magnetic horns are the key elements of the NuMI beam line. This paper uses the muon beam profile observed at the muon monitors to study the NuMI horn focusing mechanism. It is found that the horn magnet generates dipole and quadrupole fields to focus pions. This suggests that the optics of the horn magnet are predominantly linear. Our study shows that the muon beam profile accurately detects the horn current within 0.05%.
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Submitted 15 May, 2023;
originally announced May 2023.
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The Profiled Feldman-Cousins technique for confidence interval construction in the presence of nuisance parameters
Authors:
M. A. Acero,
B. Acharya,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
A. Bat,
K. Bays,
R. Bernstein,
V. Bhatnagar,
D. Bhattarai,
B. Bhuyan,
J. Bian,
A. C. Booth,
R. Bowles
, et al. (196 additional authors not shown)
Abstract:
Measuring observables to constrain models using maximum-likelihood estimation is fundamental to many physics experiments. The Profiled Feldman-Cousins method described here is a potential solution to common challenges faced in constructing accurate confidence intervals: small datasets, bounded parameters, and the need to properly handle nuisance parameters. This method achieves more accurate frequ…
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Measuring observables to constrain models using maximum-likelihood estimation is fundamental to many physics experiments. The Profiled Feldman-Cousins method described here is a potential solution to common challenges faced in constructing accurate confidence intervals: small datasets, bounded parameters, and the need to properly handle nuisance parameters. This method achieves more accurate frequentist coverage than other methods in use, and is generally applicable to the problem of parameter estimation in neutrino oscillations and similar measurements. We describe an implementation of this method in the context of the NOvA experiment.
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Submitted 1 August, 2022; v1 submitted 28 July, 2022;
originally announced July 2022.
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Measurement of the $ν_e-$Nucleus Charged-Current Double-Differential Cross Section at $\left< E_ν \right> = $ 2.4 GeV using NOvA
Authors:
M. A. Acero,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
R. Bernstein,
V. Bhatnagar,
D. Bhattarai,
B. Bhuyan,
J. Bian,
A. C. Booth,
R. Bowles,
B. Brahma,
C. Bromberg
, et al. (190 additional authors not shown)
Abstract:
The inclusive electron neutrino charged-current cross section is measured in the NOvA near detector using $8.02\times10^{20}$ protons-on-target (POT) in the NuMI beam. The sample of GeV electron neutrino interactions is the largest analyzed to date and is limited by $\simeq$ 17\% systematic rather than the $\simeq$ 7.4\% statistical uncertainties. The double-differential cross section in final-sta…
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The inclusive electron neutrino charged-current cross section is measured in the NOvA near detector using $8.02\times10^{20}$ protons-on-target (POT) in the NuMI beam. The sample of GeV electron neutrino interactions is the largest analyzed to date and is limited by $\simeq$ 17\% systematic rather than the $\simeq$ 7.4\% statistical uncertainties. The double-differential cross section in final-state electron energy and angle is presented for the first time, together with the single-differential dependence on $Q^{2}$ (squared four-momentum transfer) and energy, in the range 1 GeV $ \leq E_ν < $6 GeV. Detailed comparisons are made to the predictions of the GENIE, GiBUU, NEUT, and NuWro neutrino event generators. The data do not strongly favor a model over the others consistently across all three cross sections measured, though some models have especially good or poor agreement in the single differential cross section vs. $Q^{2}$.
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Submitted 21 June, 2022;
originally announced June 2022.
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Measurement of the Double-Differential Muon-neutrino Charged-Current Inclusive Cross Section in the NOvA Near Detector
Authors:
M. A. Acero,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
B. Behera,
R. Bernstein,
V. Bhatnagar,
D. Bhattarai,
B. Bhuyan,
J. Bian,
J. Blair,
A. C. Booth,
R. Bowles
, et al. (181 additional authors not shown)
Abstract:
We report cross-section measurements of the final-state muon kinematics for \numu charged-current interactions in the NOvA near detector using an accumulated 8.09$\times10^{20}$ protons-on-target (POT) 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…
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We report cross-section measurements of the final-state muon kinematics for \numu charged-current interactions in the NOvA near detector using an accumulated 8.09$\times10^{20}$ protons-on-target (POT) 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, $E_ν$, and square of the four-momentum transfer, $Q^2$. We compare the results to inclusive cross-section predictions from various neutrino event generators via $χ^2$ 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 $Q^2$, indicating a missing suppression of the cross section in current neutrino-nucleus scattering models.
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Submitted 18 July, 2023; v1 submitted 24 September, 2021;
originally announced September 2021.
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An Improved Measurement of Neutrino Oscillation Parameters by the NOvA Experiment
Authors:
M. A. Acero,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
R. Bernstein,
V. Bhatnagar,
D. Bhattarai,
B. Bhuyan,
J. Bian,
J. Blair,
A. C. Booth,
R. Bowles,
C. Bromberg
, et al. (180 additional authors not shown)
Abstract:
We present new $ν_μ\rightarrowν_e$, $ν_μ\rightarrowν_μ$, $\overlineν_μ\rightarrow\overlineν_e$, and $\overlineν_μ\rightarrow\overlineν_μ$ oscillation measurements by the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over the previously reported results. The additional data, combined with previously published neutrino and antineutrino data, are all analyzed using improved tech…
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We present new $ν_μ\rightarrowν_e$, $ν_μ\rightarrowν_μ$, $\overlineν_μ\rightarrow\overlineν_e$, and $\overlineν_μ\rightarrow\overlineν_μ$ oscillation measurements by the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over the previously reported results. The additional data, combined with previously published neutrino and antineutrino data, are all analyzed using improved techniques and simulations. A joint fit to the $ν_e$, $ν_μ$, $\overlineν_e$, and $\overlineν_μ$ candidate samples within the 3-flavor neutrino oscillation framework continues to yield a best-fit point in the normal mass ordering and the upper octant of the $θ_{23}$ mixing angle, with $Δm^{2}_{32} = (2.41\pm0.07)\times 10^{-3}$ eV$^2$ and $\sin^2θ_{23} = 0.57^{+0.03}_{-0.04}$. The data disfavor combinations of oscillation parameters that give rise to a large asymmetry in the rates of $ν_e$ and $\overlineν_e$ appearance. This includes values of the CP-violating phase in the vicinity of $δ_\text{CP} = π/2$ which are excluded by $>3σ$ for the inverted mass ordering, and values around $δ_\text{CP} = 3π/2$ in the normal ordering which are disfavored at 2$σ$ confidence.
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Submitted 8 August, 2022; v1 submitted 18 August, 2021;
originally announced August 2021.
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Extended search for supernova-like neutrinos in NOvA coincident with LIGO/Virgo detections
Authors:
M. A. Acero,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
R. Bernstein,
V. Bhatnagar,
B. Bhuyan,
J. Bian,
J. Blair,
A. C. Booth,
R. Bowles,
C. Bromberg,
N. Buchanan
, et al. (178 additional authors not shown)
Abstract:
A search is performed for supernova-like neutrino interactions coincident with 76 gravitational wave events detected by the LIGO/Virgo Collaboration. For 40 of these events, full readout of the time around the gravitational wave is available from the NOvA Far Detector. For these events, we set limits on the fluence of the sum of all neutrino flavors of $F < 7(4)\times 10^{10}\mathrm{cm}^{-2}$ at 9…
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A search is performed for supernova-like neutrino interactions coincident with 76 gravitational wave events detected by the LIGO/Virgo Collaboration. For 40 of these events, full readout of the time around the gravitational wave is available from the NOvA Far Detector. For these events, we set limits on the fluence of the sum of all neutrino flavors of $F < 7(4)\times 10^{10}\mathrm{cm}^{-2}$ at 90% C.L. assuming energy and time distributions corresponding to the Garching supernova models with masses 9.6(27)$\mathrm{M}_\odot$. Under the hypothesis that any given gravitational wave event was caused by a supernova, this corresponds to a distance of $r > 29(50)$kpc at 90% C.L. Weaker limits are set for other gravitational wave events with partial Far Detector data and/or Near Detector data.
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Submitted 23 August, 2021; v1 submitted 10 June, 2021;
originally announced June 2021.
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Search for active-sterile antineutrino mixing using neutral-current interactions with the NOvA experiment
Authors:
M. A. Acero,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
R. Bernstein,
V. Bhatnagar,
B. Bhuyan,
J. Bian,
J. Blair,
A. C. Booth,
R. Bowles,
C. Bromberg,
N. Buchanan
, et al. (174 additional authors not shown)
Abstract:
This Letter reports results from the first long-baseline search for sterile antineutrinos mixing in an accelerator-based antineutrino-dominated beam. The rate of neutral-current interactions in the two NOvA detectors, at distances of 1 km and 810 km from the beam source, is analyzed using an exposure of $12.51\times10^{20}$ protons-on-target from the NuMI beam at Fermilab running in antineutrino m…
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This Letter reports results from the first long-baseline search for sterile antineutrinos mixing in an accelerator-based antineutrino-dominated beam. The rate of neutral-current interactions in the two NOvA detectors, at distances of 1 km and 810 km from the beam source, is analyzed using an exposure of $12.51\times10^{20}$ protons-on-target from the NuMI beam at Fermilab running in antineutrino mode. A total of $121$ of neutral-current candidates are observed at the Far Detector, compared to a prediction of $122\pm11$(stat.)$\pm15$(syst.) assuming mixing between three active flavors. No evidence for $\barν_μ\rightarrow\barν_{s}$ oscillation is observed. Interpreting this result within a 3+1 model, constraints are placed on the mixing angles $θ_{24} < 25^{\circ}$ and $θ_{34} < 32^{\circ}$ at the 90% C.L. for $0.05$eV$^{2} \leq Δm^{2}_{41} \leq 0.5$eV$^{2}$, the range of mass splittings that produces no significant oscillations at the Near Detector. These are the first 3+1 confidence limits set using long-baseline accelerator antineutrinos.
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Submitted 30 September, 2021; v1 submitted 8 June, 2021;
originally announced June 2021.
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Seasonal Variation of Multiple-Muon Cosmic Ray Air Showers Observed in the NOvA Detector on the Surface
Authors:
M. A. Acero,
P. Adamson,
L. Aliaga,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
R. Bernstein,
V. Bhatnagar,
B. Bhuyan,
J. Bian,
J. Blair,
A. C. Booth,
R. Bowles,
C. Bromberg,
N. Buchanan
, et al. (172 additional authors not shown)
Abstract:
We report the rate of cosmic ray air showers with multiplicities exceeding 15 muon tracks recorded in the NOvA Far Detector between May 2016 and May 2018. The detector is located on the surface under an overburden of 3.6 meters water equivalent. We observe a seasonal dependence in the rate of multiple-muon showers, which varies in magnitude with multiplicity and zenith angle. During this period, t…
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We report the rate of cosmic ray air showers with multiplicities exceeding 15 muon tracks recorded in the NOvA Far Detector between May 2016 and May 2018. The detector is located on the surface under an overburden of 3.6 meters water equivalent. We observe a seasonal dependence in the rate of multiple-muon showers, which varies in magnitude with multiplicity and zenith angle. During this period, the effective atmospheric temperature and surface pressure ranged between 210 K to 230 K and 940mbar to 990mbar, respectively; the shower rates are anti-correlated with the variation in the effective temperature. The variations are about 30% larger for the highest multiplicities than the lowest multiplicities and 20% larger for showers near the horizon than vertical showers.
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Submitted 13 July, 2021; v1 submitted 9 May, 2021;
originally announced May 2021.
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Measurement of the Atmospheric Muon Rate with the MicroBooNE Liquid Argon TPC
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
V. Basque,
M. Bass,
F. Bay,
S. Berkman,
A. Bhanderi,
A. Bhat,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez
, et al. (165 additional authors not shown)
Abstract:
MicroBooNE is a near-surface liquid argon (LAr) time projection chamber (TPC) located at Fermilab. We measure the characterisation of muons originating from cosmic interactions in the atmosphere using both the charge collection and light readout detectors. The data is compared with the CORSIKA cosmic-ray simulation. Good agreement is found between the observation, simulation and previous results.…
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MicroBooNE is a near-surface liquid argon (LAr) time projection chamber (TPC) located at Fermilab. We measure the characterisation of muons originating from cosmic interactions in the atmosphere using both the charge collection and light readout detectors. The data is compared with the CORSIKA cosmic-ray simulation. Good agreement is found between the observation, simulation and previous results. Furthermore, the angular resolution of the reconstructed muons inside the TPC is studied in simulation.
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Submitted 13 April, 2021; v1 submitted 22 December, 2020;
originally announced December 2020.
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Search for Slow Magnetic Monopoles with the NOvA Detector on the Surface
Authors:
NOvA Collaboration,
M. A. Acero,
P. Adamson,
L. Aliaga,
T. Alion,
V. Allakhverdian,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
S. Bending,
R. Bernstein,
V. Bhatnagar,
B. Bhuyan,
J. Bian,
J. Blair
, et al. (174 additional authors not shown)
Abstract:
We report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure of the NOvA experiment's Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, setting an upper limit on the flux of $2\times 10^{-14} \mathrm{cm^{-2}s^{-1}sr^{-1}}$ at 90% C.L. for mon…
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We report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure of the NOvA experiment's Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, setting an upper limit on the flux of $2\times 10^{-14} \mathrm{cm^{-2}s^{-1}sr^{-1}}$ at 90% C.L. for monopole speed $6\times 10^{-4} < β< 5\times 10^{-3}$ and mass greater than $5\times 10^{8}$ GeV. Because of NOvA's small overburden of 3 meters-water equivalent, this constraint covers a previously unexplored low-mass region.
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Submitted 5 January, 2021; v1 submitted 10 September, 2020;
originally announced September 2020.
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Supernova neutrino detection in NOvA
Authors:
NOvA Collaboration,
M. A. Acero,
P. Adamson,
G. Agam,
L. Aliaga,
T. Alion,
V. Allakhverdian,
N. Anfimov,
A. Antoshkin,
E. Arrieta-Diaz,
L. Asquith,
A. Aurisano,
A. Back,
C. Backhouse,
M. Baird,
N. Balashov,
P. Baldi,
B. A. Bambah,
S. Bashar,
K. Bays,
S. Bending,
R. Bernstein,
V. Bhatnagar,
B. Bhuyan,
J. Bian
, et al. (177 additional authors not shown)
Abstract:
The NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the flux of neutrinos which are emitted during a core-collapse supernova through inverse beta decay interactions on carbon at energies of…
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The NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the flux of neutrinos which are emitted during a core-collapse supernova through inverse beta decay interactions on carbon at energies of $\mathcal{O}(10~\text{MeV})$. This signature provides a means to study the dominant mode of energy release for a core-collapse supernova occurring in our galaxy. We describe the data-driven software trigger system developed and employed by the NOvA experiment to identify and record neutrino data from nearby galactic supernovae. This technique has been used by NOvA to self-trigger on potential core-collapse supernovae in our galaxy, with an estimated sensitivity reaching out to 10~kpc distance while achieving a detection efficiency of 23\% to 49\% for supernovae from progenitor stars with masses of 9.6M$_\odot$ to 27M$_\odot$, respectively.
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Submitted 29 July, 2020; v1 submitted 14 May, 2020;
originally announced May 2020.
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Vertex-Finding and Reconstruction of Contained Two-track Neutrino Events in the MicroBooNE Detector
Authors:
MicroBooNE collaboration,
P. Abratenko,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
V. Basque,
L. Bathe-Peters,
S. Berkman,
A. Bhanderi,
A. Bhat,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Castillo Fernandez,
F. Cavanna,
G. Cerati
, et al. (164 additional authors not shown)
Abstract:
We describe algorithms developed to isolate and accurately reconstruct two-track events that are contained within the MicroBooNE detector. This method is optimized to reconstruct two tracks of lengths longer than 5 cm. This code has applications to searches for neutrino oscillations and measurements of cross sections using quasi-elastic-like charged current events. The algorithms we discuss will b…
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We describe algorithms developed to isolate and accurately reconstruct two-track events that are contained within the MicroBooNE detector. This method is optimized to reconstruct two tracks of lengths longer than 5 cm. This code has applications to searches for neutrino oscillations and measurements of cross sections using quasi-elastic-like charged current events. The algorithms we discuss will be applicable to all detectors running in Fermilab's Short Baseline Neutrino program (SBN), and to any future liquid argon time projection chamber (LArTPC) experiment with beam energies ~1 GeV. The algorithms are publicly available on a GITHUB repository. This reconstruction offers a complementary and independent alternative to the Pandora reconstruction package currently in use in LArTPC experiments, and provides similar reconstruction performance for two-track events.
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Submitted 7 December, 2020; v1 submitted 21 February, 2020;
originally announced February 2020.
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Search for heavy neutral leptons decaying into muon-pion pairs in the MicroBooNE detector
Authors:
P. Abratenko,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
V. Basque,
S. Berkman,
A. Bhanderi,
A. Bhat,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Castillo Fernandez,
F. Cavanna,
G. Cerati,
Y. Chen,
E. Church
, et al. (159 additional authors not shown)
Abstract:
We present upper limits on the production of heavy neutral leptons (HNLs) decaying to $μπ$ pairs using data collected with the MicroBooNE liquid-argon time projection chamber (TPC) operating at Fermilab. This search is the first of its kind performed in a liquid-argon TPC. We use data collected in 2017 and 2018 corresponding to an exposure of $2.0 \times 10^{20}$ protons on target from the Fermila…
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We present upper limits on the production of heavy neutral leptons (HNLs) decaying to $μπ$ pairs using data collected with the MicroBooNE liquid-argon time projection chamber (TPC) operating at Fermilab. This search is the first of its kind performed in a liquid-argon TPC. We use data collected in 2017 and 2018 corresponding to an exposure of $2.0 \times 10^{20}$ protons on target from the Fermilab Booster Neutrino Beam, which produces mainly muon neutrinos with an average energy of $\approx 800$ MeV. HNLs with higher mass are expected to have a longer time-of-flight to the liquid-argon TPC than Standard Model neutrinos. The data are therefore recorded with a dedicated trigger configured to detect HNL decays that occur after the neutrino spill reaches the detector. We set upper limits at the $90\%$ confidence level on the element $\lvert U_{\mu4}\rvert^2$ of the extended PMNS mixing matrix in the range $\lvert U_{\mu4}\rvert^2<(6.6$-$0.9)\times 10^{-7}$ for Dirac HNLs and $\lvert U_{\mu4}\rvert^2<(4.7$-$0.7)\times 10^{-7}$ for Majorana HNLs, assuming HNL masses between $260$ and $385$ MeV and $\lvert U_{e 4}\rvert^2 = \lvert U_{τ4}\rvert^2 = 0$.
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Submitted 12 February, 2020; v1 submitted 24 November, 2019;
originally announced November 2019.
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Reconstruction and Measurement of $\mathcal{O}$(100) MeV Energy Electromagnetic Activity from $π^0 \rightarrow γγ$ Decays in the MicroBooNE LArTPC
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
V. Basque,
M. Bass,
F. Bay,
S. Berkman,
A. Bhanderi,
A. Bhat,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez
, et al. (164 additional authors not shown)
Abstract:
We present results on the reconstruction of electromagnetic (EM) activity from photons produced in charged current $ν_μ$ interactions with final state $π^0$s. We employ a fully-automated reconstruction chain capable of identifying EM showers of $\mathcal{O}$(100) MeV energy, relying on a combination of traditional reconstruction techniques together with novel machine-learning approaches. These stu…
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We present results on the reconstruction of electromagnetic (EM) activity from photons produced in charged current $ν_μ$ interactions with final state $π^0$s. We employ a fully-automated reconstruction chain capable of identifying EM showers of $\mathcal{O}$(100) MeV energy, relying on a combination of traditional reconstruction techniques together with novel machine-learning approaches. These studies demonstrate good energy resolution, and good agreement between data and simulation, relying on the reconstructed invariant $π^0$ mass and other photon distributions for validation. The reconstruction techniques developed are applied to a selection of $ν_μ + {\rm Ar} \rightarrow μ+ π^0 + X$ candidate events to demonstrate the potential for calorimetric separation of photons from electrons and reconstruction of $π^0$ kinematics.
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Submitted 4 October, 2019;
originally announced October 2019.
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A Method to Determine the Electric Field of Liquid Argon Time Projection Chambers Using a UV Laser System and its Application in MicroBooNE
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
V. Basque,
M. Bass,
F. Bay,
S. Berkman,
A. Bhanderi,
A. Bhat,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez
, et al. (165 additional authors not shown)
Abstract:
Liquid argon time projection chambers (LArTPCs) are now a standard detector technology for making accelerator neutrino measurements, due to their high material density, precise tracking, and calorimetric capabilities. An electric field (E-field) is required in such detectors to drift ionized electrons to the anode to be collected. The E-field of a TPC is often approximated to be uniform between th…
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Liquid argon time projection chambers (LArTPCs) are now a standard detector technology for making accelerator neutrino measurements, due to their high material density, precise tracking, and calorimetric capabilities. An electric field (E-field) is required in such detectors to drift ionized electrons to the anode to be collected. The E-field of a TPC is often approximated to be uniform between the anode and the cathode planes. However, significant distortions can appear from effects such as mechanical deformations, electrode failures, or the accumulation of space charge generated by cosmic rays. The latter is particularly relevant for detectors placed near the Earth's surface and with large drift distances and long drift time. To determine the E-field in situ, an ultraviolet (UV) laser system is installed in the MicroBooNE experiment at Fermi National Accelerator Laboratory. The purpose of this system is to provide precise measurements of the E-field, and to make it possible to correct for 3D spatial distortions due to E-field non-uniformities. Here we describe the methodology developed for deriving spatial distortions, the drift velocity and the E-field from UV-laser measurements.
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Submitted 15 October, 2019; v1 submitted 3 October, 2019;
originally announced October 2019.
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Calibration of the charge and energy loss per unit length of the MicroBooNE liquid argon time projection chamber using muons and protons
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
V. Basque,
M. Bass,
F. Bay,
S. Berkman,
A. Bhanderi,
A. Bhat,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez
, et al. (164 additional authors not shown)
Abstract:
We describe a method used to calibrate the position- and time-dependent response of the MicroBooNE liquid argon time projection chamber anode wires to ionization particle energy loss. The method makes use of crossing cosmic-ray muons to partially correct anode wire signals for multiple effects as a function of time and position, including cross-connected TPC wires, space charge effects, electron a…
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We describe a method used to calibrate the position- and time-dependent response of the MicroBooNE liquid argon time projection chamber anode wires to ionization particle energy loss. The method makes use of crossing cosmic-ray muons to partially correct anode wire signals for multiple effects as a function of time and position, including cross-connected TPC wires, space charge effects, electron attachment to impurities, diffusion, and recombination. The overall energy scale is then determined using fully-contained beam-induced muons originating and stopping in the active region of the detector. Using this method, we obtain an absolute energy scale uncertainty of 2\% in data. We use stopping protons to further refine the relation between the measured charge and the energy loss for highly-ionizing particles. This data-driven detector calibration improves both the measurement of total deposited energy and particle identification based on energy loss per unit length as a function of residual range. As an example, the proton selection efficiency is increased by 2\% after detector calibration.
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Submitted 24 February, 2020; v1 submitted 26 July, 2019;
originally announced July 2019.
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First Measurement of Inclusive Muon Neutrino Charged Current Differential Cross Sections on Argon at $E_ν\sim 0.8$ GeV with the MicroBooNE Detector
Authors:
P. Abratenko,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
M. Auger,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez,
F. Cavanna
, et al. (156 additional authors not shown)
Abstract:
We report the first measurement of the double-differential and total muon neutrino charged current inclusive cross sections on argon at a mean neutrino energy of 0.8 GeV. Data were collected using the MicroBooNE liquid argon time projection chamber located in the Fermilab Booster neutrino beam and correspond to $1.6 \times 10^{20}$ protons on target of exposure. The measured differential cross sec…
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We report the first measurement of the double-differential and total muon neutrino charged current inclusive cross sections on argon at a mean neutrino energy of 0.8 GeV. Data were collected using the MicroBooNE liquid argon time projection chamber located in the Fermilab Booster neutrino beam and correspond to $1.6 \times 10^{20}$ protons on target of exposure. The measured differential cross sections are presented as a function of muon momentum, using multiple Coulomb scattering as a momentum measurement technique, and the muon angle with respect to the beam direction. We compare the measured cross sections to multiple neutrino event generators and find better agreement with those containing more complete treatment of quasielastic scattering processes at low $Q^2$. The total flux integrated cross section is measured to be $0.693 \pm 0.010 \, (\text{stat}) \pm 0.165 \, (\text{syst}) \times 10^{-38} \, \text{cm}^{2}$.
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Submitted 30 September, 2019; v1 submitted 23 May, 2019;
originally announced May 2019.
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Design and construction of the MicroBooNE Cosmic Ray Tagger system
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
M. Auger,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez,
F. Cavanna
, et al. (149 additional authors not shown)
Abstract:
The MicroBooNE detector utilizes a liquid argon time projection chamber (LArTPC) with an 85 t active mass to study neutrino interactions along the Booster Neutrino Beam (BNB) at Fermilab. With a deployment location near ground level, the detector records many cosmic muon tracks in each beam-related detector trigger that can be misidentified as signals of interest. To reduce these cosmogenic backgr…
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The MicroBooNE detector utilizes a liquid argon time projection chamber (LArTPC) with an 85 t active mass to study neutrino interactions along the Booster Neutrino Beam (BNB) at Fermilab. With a deployment location near ground level, the detector records many cosmic muon tracks in each beam-related detector trigger that can be misidentified as signals of interest. To reduce these cosmogenic backgrounds, we have designed and constructed a TPC-external Cosmic Ray Tagger (CRT). This sub-system was developed by the Laboratory for High Energy Physics (LHEP), Albert Einstein center for fundamental physics, University of Bern. The system utilizes plastic scintillation modules to provide precise time and position information for TPC-traversing particles. Successful matching of TPC tracks and CRT data will allow us to reduce cosmogenic background and better characterize the light collection system and LArTPC data using cosmic muons. In this paper we describe the design and installation of the MicroBooNE CRT system and provide an overview of a series of tests done to verify the proper operation of the system and its components during installation, commissioning, and physics data-taking.
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Submitted 15 March, 2019; v1 submitted 9 January, 2019;
originally announced January 2019.
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Rejecting cosmic background for exclusive neutrino interaction studies with Liquid Argon TPCs; a case study with the MicroBooNE detector
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
M. Auger,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez,
F. Cavanna
, et al. (150 additional authors not shown)
Abstract:
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and cross-section measurements in surface detectors. We present methods for CR rejection in measurements of charged-current quasielastic-like (CCQE-like) neutrino interactions, with a muon and a proton in the final state, measured using liquid argon time projection chambers (LArTPCs). Using a sample of…
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Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and cross-section measurements in surface detectors. We present methods for CR rejection in measurements of charged-current quasielastic-like (CCQE-like) neutrino interactions, with a muon and a proton in the final state, measured using liquid argon time projection chambers (LArTPCs). Using a sample of cosmic data collected with the MicroBooNE detector, mixed with simulated neutrino scattering events, a set of event selection criteria is developed that produces an event sample with minimal contribution from CR background. Depending on the selection criteria used a purity between 50% and 80% can be achieved with a signal selection efficiency between 50% and 25%, with higher purity coming at the expense of lower efficiency. While using a specific dataset from the MicroBooNE detector and selection criteria values optimized for CCQE-like events, the concepts presented here are generic and can be adapted for various studies of exclusive νμ interactions in LArTPCs.
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Submitted 2 January, 2019; v1 submitted 9 December, 2018;
originally announced December 2018.
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First Measurement of $ν_μ$ Charged-Current $π^{0}$ Production on Argon with a LArTPC
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
M. Auger,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez,
F. Cavanna
, et al. (150 additional authors not shown)
Abstract:
We report the first measurement of the flux-integrated cross section of $ν_μ$ charged-current single $π^{0}$ production on argon. This measurement is performed with the MicroBooNE detector, an 85 ton active mass liquid argon time projection chamber exposed to the Booster Neutrino Beam at Fermilab. This result on argon is compared to past measurements on lighter nuclei to investigate the scaling as…
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We report the first measurement of the flux-integrated cross section of $ν_μ$ charged-current single $π^{0}$ production on argon. This measurement is performed with the MicroBooNE detector, an 85 ton active mass liquid argon time projection chamber exposed to the Booster Neutrino Beam at Fermilab. This result on argon is compared to past measurements on lighter nuclei to investigate the scaling assumptions used in models of the production and transport of pions in neutrino-nucleus scattering. The techniques used are an important demonstration of the successful reconstruction and analysis of neutrino interactions producing electromagnetic final states using a liquid argon time projection chamber operating at the earth's surface.
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Submitted 6 November, 2018;
originally announced November 2018.
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A Deep Neural Network for Pixel-Level Electromagnetic Particle Identification in the MicroBooNE Liquid Argon Time Projection Chamber
Authors:
MicroBooNE collaboration,
C. Adams,
M. Alrashed,
R. An,
J. Anthony,
J. Asaadi,
A. Ashkenazi,
M. Auger,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
I. Caro Terrazas,
R. Carr,
R. Castillo Fernandez,
F. Cavanna
, et al. (148 additional authors not shown)
Abstract:
We have developed a convolutional neural network (CNN) that can make a pixel-level prediction of objects in image data recorded by a liquid argon time projection chamber (LArTPC) for the first time. We describe the network design, training techniques, and software tools developed to train this network. The goal of this work is to develop a complete deep neural network based data reconstruction cha…
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We have developed a convolutional neural network (CNN) that can make a pixel-level prediction of objects in image data recorded by a liquid argon time projection chamber (LArTPC) for the first time. We describe the network design, training techniques, and software tools developed to train this network. The goal of this work is to develop a complete deep neural network based data reconstruction chain for the MicroBooNE detector. We show the first demonstration of a network's validity on real LArTPC data using MicroBooNE collection plane images. The demonstration is performed for stopping muon and a $ν_μ$ charged current neutral pion data samples.
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Submitted 22 August, 2018;
originally announced August 2018.
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Significant Excess of ElectronLike Events in the MiniBooNE Short-Baseline Neutrino Experiment
Authors:
MiniBooNE Collaboration,
A. A. Aguilar-Arevalo,
B. C. Brown,
L. Bugel,
G. Cheng,
J. M. Conrad,
R. L. Cooper,
R. Dharmapalan,
A. Diaz,
Z. Djurcic,
D. A. Finley,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
E. -C. Huang,
W. Huelsnitz,
C. Ignarra,
R. A. Johnson,
G. Karagiorgi,
T. Katori,
T. Kobilarcik,
W. C. Louis,
C. Mariani,
W. Marsh
, et al. (23 additional authors not shown)
Abstract:
The MiniBooNE experiment at Fermilab reports results from an analysis of $ν_e$ appearance data from $12.84 \times 10^{20}$ protons on target in neutrino mode, an increase of approximately a factor of two over previously reported results. A $ν_e$ charged-current quasielastic event excess of $381.2 \pm 85.2$ events ($4.5 σ$) is observed in the energy range $200<E_ν^{QE}<1250$~MeV. Combining these da…
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The MiniBooNE experiment at Fermilab reports results from an analysis of $ν_e$ appearance data from $12.84 \times 10^{20}$ protons on target in neutrino mode, an increase of approximately a factor of two over previously reported results. A $ν_e$ charged-current quasielastic event excess of $381.2 \pm 85.2$ events ($4.5 σ$) is observed in the energy range $200<E_ν^{QE}<1250$~MeV. Combining these data with the $\bar ν_e$ appearance data from $11.27 \times 10^{20}$ protons on target in antineutrino mode, a total $ν_e$ plus $\bar ν_e$ charged-current quasielastic event excess of $460.5 \pm 99.0$ events ($4.7 σ$) is observed. If interpreted in a two-neutrino oscillation model, $ν_μ \rightarrow ν_e$, the best oscillation fit to the excess has a probability of $21.1\%$, while the background-only fit has a $χ^2$ probability of $6 \times 10^{-7}$ relative to the best fit. The MiniBooNE data are consistent in energy and magnitude with the excess of events reported by the Liquid Scintillator Neutrino Detector (LSND), and the significance of the combined LSND and MiniBooNE excesses is $6.0 σ$. A two-neutrino oscillation interpretation of the data would require at least four neutrino types and indicate physics beyond the three neutrino paradigm.Although the data are fit with a two-neutrino oscillation model, other models may provide better fits to the data.
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Submitted 26 October, 2018; v1 submitted 30 May, 2018;
originally announced May 2018.
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Comparison of νμ-Ar multiplicity distributions observed by MicroBooNE to GENIE model predictions
Authors:
C. Adams,
R. An,
J. Anthony,
J. Asaadi,
M. Auger,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
R. Castillo Fernandez,
F. Cavanna,
G. Cerati,
H. Chen,
Y. Chen,
E. Church,
D. Cianci
, et al. (140 additional authors not shown)
Abstract:
We measure a large set of observables in inclusive charged current muon neutrino scattering on argon with the MicroBooNE liquid argon time projection chamber operating at Fermilab. We evaluate three neutrino interaction models based on the widely used GENIE event generator using these observables. The measurement uses a data set consisting of neutrino interactions with a final state muon candidate…
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We measure a large set of observables in inclusive charged current muon neutrino scattering on argon with the MicroBooNE liquid argon time projection chamber operating at Fermilab. We evaluate three neutrino interaction models based on the widely used GENIE event generator using these observables. The measurement uses a data set consisting of neutrino interactions with a final state muon candidate fully contained within the MicroBooNE detector. These data were collected in 2016 with the Fermilab Booster Neutrino Beam, which has an average neutrino energy of 800 MeV, using an exposure corresponding to 5E19 protons-on-target. The analysis employs fully automatic event selection and charged particle track reconstruction and uses a data-driven technique to separate neutrino interactions from cosmic ray background events. We find that GENIE models consistently describe the shapes of a large number of kinematic distributions for fixed observed multiplicity.
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Submitted 26 March, 2019; v1 submitted 17 May, 2018;
originally announced May 2018.
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Ionization Electron Signal Processing in Single Phase LArTPCs II. Data/Simulation Comparison and Performance in MicroBooNE
Authors:
MicroBooNE collaboration,
C. Adams,
R. An,
J. Anthony,
J. Asaadi,
M. Auger,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
R. Carr,
I. Caro Terrazas,
R. Castillo Fernandez,
F. Cavanna,
G. Cerati,
H. Chen
, et al. (146 additional authors not shown)
Abstract:
The single-phase liquid argon time projection chamber (LArTPC) provides a large amount of detailed information in the form of fine-grained drifted ionization charge from particle traces. To fully utilize this information, the deposited charge must be accurately extracted from the raw digitized waveforms via a robust signal processing chain. Enabled by the ultra-low noise levels associated with cry…
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The single-phase liquid argon time projection chamber (LArTPC) provides a large amount of detailed information in the form of fine-grained drifted ionization charge from particle traces. To fully utilize this information, the deposited charge must be accurately extracted from the raw digitized waveforms via a robust signal processing chain. Enabled by the ultra-low noise levels associated with cryogenic electronics in the MicroBooNE detector, the precise extraction of ionization charge from the induction wire planes in a single-phase LArTPC is qualitatively demonstrated on MicroBooNE data with event display images, and quantitatively demonstrated via waveform-level and track-level metrics. Improved performance of induction plane calorimetry is demonstrated through the agreement of extracted ionization charge measurements across different wire planes for various event topologies. In addition to the comprehensive waveform-level comparison of data and simulation, a calibration of the cryogenic electronics response is presented and solutions to various MicroBooNE-specific TPC issues are discussed. This work presents an important improvement in LArTPC signal processing, the foundation of reconstruction and therefore physics analyses in MicroBooNE.
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Submitted 11 June, 2018; v1 submitted 7 April, 2018;
originally announced April 2018.
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Ionization Electron Signal Processing in Single Phase LArTPCs I. Algorithm Description and Quantitative Evaluation with MicroBooNE Simulation
Authors:
MicroBooNE collaboration,
C. Adams,
R. An,
J. Anthony,
J. Asaadi,
M. Auger,
L. Bagby,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
A. Bhat,
K. Bhattacharya,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
R. Castillo Fernandez,
F. Cavanna,
G. Cerati,
H. Chen,
Y. Chen
, et al. (144 additional authors not shown)
Abstract:
We describe the concept and procedure of drifted-charge extraction developed in the MicroBooNE experiment, a single-phase liquid argon time projection chamber (LArTPC). This technique converts the raw digitized TPC waveform to the number of ionization electrons passing through a wire plane at a given time. A robust recovery of the number of ionization electrons from both induction and collection a…
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We describe the concept and procedure of drifted-charge extraction developed in the MicroBooNE experiment, a single-phase liquid argon time projection chamber (LArTPC). This technique converts the raw digitized TPC waveform to the number of ionization electrons passing through a wire plane at a given time. A robust recovery of the number of ionization electrons from both induction and collection anode wire planes will augment the 3D reconstruction, and is particularly important for tomographic reconstruction algorithms. A number of building blocks of the overall procedure are described. The performance of the signal processing is quantitatively evaluated by comparing extracted charge with the true charge through a detailed TPC detector simulation taking into account position-dependent induced current inside a single wire region and across multiple wires. Some areas for further improvement of the performance of the charge extraction procedure are also discussed.
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Submitted 9 April, 2018; v1 submitted 23 February, 2018;
originally announced February 2018.
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First Measurement of Monoenergetic Muon Neutrino Charged Current Interactions
Authors:
A. A. Aguilar-Arevalo,
B. C. Brown,
L. Bugel,
G. Cheng,
E. D. Church,
J. M. Conrad,
R. L. Cooper,
R. Dharmapalan,
Z. Djurcic,
D. A. Finley,
R. S. Fitzpatrick,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
W. Huelsnitz,
C. Ignarra,
R. Imlay,
R. A. Johnson,
J. R. Jordan,
G. Karagiorgi,
T. Katori,
T. Kobilarcik,
W. C. Louis,
K. Mahn
, et al. (24 additional authors not shown)
Abstract:
We report the first measurement of monoenergetic muon neutrino charged current interactions. MiniBooNE has isolated 236 MeV muon neutrino events originating from charged kaon decay at rest ($K^+ \rightarrow μ^+ ν_μ$) at the NuMI beamline absorber. These signal $ν_μ$-carbon events are distinguished from primarily pion decay in flight $ν_μ$ and $\overlineν_μ$ backgrounds produced at the target stati…
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We report the first measurement of monoenergetic muon neutrino charged current interactions. MiniBooNE has isolated 236 MeV muon neutrino events originating from charged kaon decay at rest ($K^+ \rightarrow μ^+ ν_μ$) at the NuMI beamline absorber. These signal $ν_μ$-carbon events are distinguished from primarily pion decay in flight $ν_μ$ and $\overlineν_μ$ backgrounds produced at the target station and decay pipe using their arrival time and reconstructed muon energy. The significance of the signal observation is at the 3.9$σ$ level. The muon kinetic energy, neutrino-nucleus energy transfer ($ω=E_ν-E_μ$), and total cross section for these events is extracted. This result is the first known-energy, weak-interaction-only probe of the nucleus to yield a measurement of $ω$ using neutrinos, a quantity thus far only accessible through electron scattering.
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Submitted 7 May, 2018; v1 submitted 11 January, 2018;
originally announced January 2018.
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The Pandora multi-algorithm approach to automated pattern recognition of cosmic-ray muon and neutrino events in the MicroBooNE detector
Authors:
MicroBooNE collaboration,
R. Acciarri,
C. Adams,
R. An,
J. Anthony,
J. Asaadi,
M. Auger,
L. Bagby,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
B. Carls,
R. Castillo Fernandez,
F. Cavanna,
H. Chen,
E. Church,
D. Cianci
, et al. (123 additional authors not shown)
Abstract:
The development and operation of Liquid-Argon Time-Projection Chambers for neutrino physics has created a need for new approaches to pattern recognition in order to fully exploit the imaging capabilities offered by this technology. Whereas the human brain can excel at identifying features in the recorded events, it is a significant challenge to develop an automated, algorithmic solution. The Pando…
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The development and operation of Liquid-Argon Time-Projection Chambers for neutrino physics has created a need for new approaches to pattern recognition in order to fully exploit the imaging capabilities offered by this technology. Whereas the human brain can excel at identifying features in the recorded events, it is a significant challenge to develop an automated, algorithmic solution. The Pandora Software Development Kit provides functionality to aid the design and implementation of pattern-recognition algorithms. It promotes the use of a multi-algorithm approach to pattern recognition, in which individual algorithms each address a specific task in a particular topology. Many tens of algorithms then carefully build up a picture of the event and, together, provide a robust automated pattern-recognition solution. This paper describes details of the chain of over one hundred Pandora algorithms and tools used to reconstruct cosmic-ray muon and neutrino events in the MicroBooNE detector. Metrics that assess the current pattern-recognition performance are presented for simulated MicroBooNE events, using a selection of final-state event topologies.
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Submitted 10 August, 2017;
originally announced August 2017.
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Measurement of cosmic-ray reconstruction efficiencies in the MicroBooNE LArTPC using a small external cosmic-ray counter
Authors:
MicroBooNE collaboration,
R. Acciarri,
C. Adams,
R. An,
J. Anthony,
J. Asaadi,
M. Auger,
L. Bagby,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
M. Bishai,
A. Blake,
T. Bolton,
L. Camilleri,
D. Caratelli,
B. Carls,
R. Castillo Fernandez,
F. Cavanna,
H. Chen,
E. Church,
D. Cianci
, et al. (126 additional authors not shown)
Abstract:
The MicroBooNE detector is a liquid argon time projection chamber at Fermilab designed to study short-baseline neutrino oscillations and neutrino-argon interaction cross-section. Due to its location near the surface, a good understanding of cosmic muons as a source of backgrounds is of fundamental importance for the experiment. We present a method of using an external 0.5 m (L) x 0.5 m (W) muon co…
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The MicroBooNE detector is a liquid argon time projection chamber at Fermilab designed to study short-baseline neutrino oscillations and neutrino-argon interaction cross-section. Due to its location near the surface, a good understanding of cosmic muons as a source of backgrounds is of fundamental importance for the experiment. We present a method of using an external 0.5 m (L) x 0.5 m (W) muon counter stack, installed above the main detector, to determine the cosmic-ray reconstruction efficiency in MicroBooNE. Data are acquired with this external muon counter stack placed in three different positions, corresponding to cosmic rays intersecting different parts of the detector. The data reconstruction efficiency of tracks in the detector is found to be $ε_{\mathrm{data}}=(97.1\pm0.1~(\mathrm{stat}) \pm 1.4~(\mathrm{sys}))\%$, in good agreement with the Monte Carlo reconstruction efficiency $ε_{\mathrm{MC}} = (97.4\pm0.1)\%$. This analysis represents a small-scale demonstration of the method that can be used with future data coming from a recently installed cosmic-ray tagger system, which will be able to tag $\approx80\%$ of the cosmic rays passing through the MicroBooNE detector.
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Submitted 31 July, 2017;
originally announced July 2017.
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Noise Characterization and Filtering in the MicroBooNE Liquid Argon TPC
Authors:
MicroBooNE collaboration,
R. Acciarri,
C. Adams,
R. An,
J. Anthony,
J. Asaadi,
M. Auger,
L. Bagby,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
M. Bishai,
A. Blake,
T. Bolton,
B. Bullard,
L. Camilleri,
D. Caratelli,
B. Carls,
R. Castillo Fernandez,
F. Cavanna,
H. Chen,
E. Church
, et al. (130 additional authors not shown)
Abstract:
The low-noise operation of readout electronics in a liquid argon time projection chamber (LArTPC) is critical to properly extract the distribution of ionization charge deposited on the wire planes of the TPC, especially for the induction planes. This paper describes the characteristics and mitigation of the observed noise in the MicroBooNE detector. The MicroBooNE's single-phase LArTPC comprises t…
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The low-noise operation of readout electronics in a liquid argon time projection chamber (LArTPC) is critical to properly extract the distribution of ionization charge deposited on the wire planes of the TPC, especially for the induction planes. This paper describes the characteristics and mitigation of the observed noise in the MicroBooNE detector. The MicroBooNE's single-phase LArTPC comprises two induction planes and one collection sense wire plane with a total of 8256 wires. Current induced on each TPC wire is amplified and shaped by custom low-power, low-noise ASICs immersed in the liquid argon. The digitization of the signal waveform occurs outside the cryostat. Using data from the first year of MicroBooNE operations, several excess noise sources in the TPC were identified and mitigated. The residual equivalent noise charge (ENC) after noise filtering varies with wire length and is found to be below 400 electrons for the longest wires (4.7 m). The response is consistent with the cold electronics design expectations and is found to be stable with time and uniform over the functioning channels. This noise level is significantly lower than previous experiments utilizing warm front-end electronics.
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Submitted 20 May, 2017;
originally announced May 2017.
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Michel Electron Reconstruction Using Cosmic-Ray Data from the MicroBooNE LArTPC
Authors:
MicroBooNE collaboration,
R. Acciarri,
C. Adams,
R. An,
J. Anthony,
J. Asaadi,
M. Auger,
L. Bagby,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
M. Bishai,
A. Blake,
T. Bolton,
L. Bugel,
L. Camilleri,
D. Caratelli,
B. Carls,
R. Castillo Fernandez,
F. Cavanna,
H. Chen,
E. Church
, et al. (121 additional authors not shown)
Abstract:
The MicroBooNE liquid argon time projection chamber (LArTPC) has been taking data at Fermilab since 2015 collecting, in addition to neutrino beam, cosmic-ray muons. Results are presented on the reconstruction of Michel electrons produced by the decay at rest of cosmic-ray muons. Michel electrons are abundantly produced in the TPC, and given their well known energy spectrum can be used to study Mic…
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The MicroBooNE liquid argon time projection chamber (LArTPC) has been taking data at Fermilab since 2015 collecting, in addition to neutrino beam, cosmic-ray muons. Results are presented on the reconstruction of Michel electrons produced by the decay at rest of cosmic-ray muons. Michel electrons are abundantly produced in the TPC, and given their well known energy spectrum can be used to study MicroBooNE's detector response to low-energy electrons (electrons with energies up to ~50 MeV). We describe the fully-automated algorithm developed to reconstruct Michel electrons, with which a sample of ~14,000 Michel electron candidates is obtained. Most of this article is dedicated to studying the impact of radiative photons produced by Michel electrons on the accuracy and resolution of their energy measurement. In this energy range, ionization and bremsstrahlung photon production contribute similarly to electron energy loss in argon, leading to a complex electron topology in the TPC. By profiling the performance of the reconstruction algorithm on simulation we show that the ability to identify and include energy deposited by radiative photons leads to a significant improvement in the energy measurement of low-energy electrons. The fractional energy resolution we measure improves from over 30% to ~20% when we attempt to include radiative photons in the reconstruction. These studies are relevant to a large number of analyses which aim to study neutrinos by measuring electrons produced by $ν_e$ interactions over a broad energy range.
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Submitted 30 August, 2017; v1 submitted 10 April, 2017;
originally announced April 2017.
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Determination of muon momentum in the MicroBooNE LArTPC using an improved model of multiple Coulomb scattering
Authors:
MicroBooNE collaboration,
P. Abratenko,
R. Acciarri,
C. Adams,
R. An,
J. Asaadi,
M. Auger,
L. Bagby,
S. Balasubramanian,
B. Baller,
C. Barnes,
G. Barr,
M. Bass,
F. Bay,
M. Bishai,
A. Blake,
T. Bolton,
L. Bugel,
L. Camilleri,
D. Caratelli,
B. Carls,
R. Castillo Fernandez,
F. Cavanna,
H. Chen,
E. Church
, et al. (123 additional authors not shown)
Abstract:
We discuss a technique for measuring a charged particle's momentum by means of multiple Coulomb scattering (MCS) in the MicroBooNE liquid argon time projection chamber (LArTPC). This method does not require the full particle ionization track to be contained inside of the detector volume as other track momentum reconstruction methods do (range-based momentum reconstruction and calorimetric momentum…
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We discuss a technique for measuring a charged particle's momentum by means of multiple Coulomb scattering (MCS) in the MicroBooNE liquid argon time projection chamber (LArTPC). This method does not require the full particle ionization track to be contained inside of the detector volume as other track momentum reconstruction methods do (range-based momentum reconstruction and calorimetric momentum reconstruction). We motivate use of this technique, describe a tuning of the underlying phenomenological formula, quantify its performance on fully contained beam-neutrino-induced muon tracks both in simulation and in data, and quantify its performance on exiting muon tracks in simulation. Using simulation, we have shown that the standard Highland formula should be re-tuned specifically for scattering in liquid argon, which significantly improves the bias and resolution of the momentum measurement. With the tuned formula, we find agreement between data and simulation for contained tracks, with a small bias in the momentum reconstruction and with resolutions that vary as a function of track length, improving from about 10% for the shortest (one meter long) tracks to 5% for longer (several meter) tracks. For simulated exiting muons with at least one meter of track contained, we find a similarly small bias, and a resolution which is less than 15% for muons with momentum below 2 GeV/c. Above 2 GeV/c, results are given as a first estimate of the MCS momentum measurement capabilities of MicroBooNE for high momentum exiting tracks.
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Submitted 5 October, 2017; v1 submitted 17 March, 2017;
originally announced March 2017.
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Design and Construction of the MicroBooNE Detector
Authors:
MicroBooNE Collaboration,
R. Acciarri,
C. Adams,
R. An,
A. Aparicio,
S. Aponte,
J. Asaadi,
M. Auger,
N. Ayoub,
L. Bagby,
B. Baller,
R. Barger,
G. Barr,
M. Bass,
F. Bay,
K. Biery,
M. Bishai,
A. Blake,
V. Bocean,
D. Boehnlein,
V. D. Bogert,
T. Bolton,
L. Bugel,
C. Callahan,
L. Camilleri
, et al. (215 additional authors not shown)
Abstract:
This paper describes the design and construction of the MicroBooNE liquid argon time projection chamber and associated systems. MicroBooNE is the first phase of the Short Baseline Neutrino program, located at Fermilab, and will utilize the capabilities of liquid argon detectors to examine a rich assortment of physics topics. In this document details of design specifications, assembly procedures, a…
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This paper describes the design and construction of the MicroBooNE liquid argon time projection chamber and associated systems. MicroBooNE is the first phase of the Short Baseline Neutrino program, located at Fermilab, and will utilize the capabilities of liquid argon detectors to examine a rich assortment of physics topics. In this document details of design specifications, assembly procedures, and acceptance tests are reported.
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Submitted 17 January, 2017; v1 submitted 17 December, 2016;
originally announced December 2016.
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Convolutional Neural Networks Applied to Neutrino Events in a Liquid Argon Time Projection Chamber
Authors:
MicroBooNE collaboration,
R. Acciarri,
C. Adams,
R. An,
J. Asaadi,
M. Auger,
L. Bagby,
B. Baller,
G. Barr,
M. Bass,
F. Bay,
M. Bishai,
A. Blake,
T. Bolton,
L. Bugel,
L. Camilleri,
D. Caratelli,
B. Carls,
R. Castillo Fernandez,
F. Cavanna,
H. Chen,
E. Church,
D. Cianci,
G. H. Collin,
J. M. Conrad
, et al. (114 additional authors not shown)
Abstract:
We present several studies of convolutional neural networks applied to data coming from the MicroBooNE detector, a liquid argon time projection chamber (LArTPC). The algorithms studied include the classification of single particle images, the localization of single particle and neutrino interactions in an image, and the detection of a simulated neutrino event overlaid with cosmic ray backgrounds t…
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We present several studies of convolutional neural networks applied to data coming from the MicroBooNE detector, a liquid argon time projection chamber (LArTPC). The algorithms studied include the classification of single particle images, the localization of single particle and neutrino interactions in an image, and the detection of a simulated neutrino event overlaid with cosmic ray backgrounds taken from real detector data. These studies demonstrate the potential of convolutional neural networks for particle identification or event detection on simulated neutrino interactions. We also address technical issues that arise when applying this technique to data from a large LArTPC at or near ground level.
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Submitted 16 November, 2016;
originally announced November 2016.
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Using L/E Oscillation Probability Distributions
Authors:
A. A. Aguilar-Arevalo,
B. C. Brown,
L. Bugel,
G. Cheng,
E. D. Church,
J. M. Conrad,
R. Dharmapalan,
Z. Djurcic,
D. A. Finley,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
W. Huelsnitz,
C. Ignarra,
R. Imlay,
R. A. Johnson,
G. Karagiorgi,
T. Katori,
T. Kobilarcik,
W. C. Louis,
C. Mariani,
W. Marsh,
G. B. Mills,
J. Mirabal
, et al. (19 additional authors not shown)
Abstract:
This paper explores the use of $L/E$ oscillation probability distributions to compare experimental measurements and to evaluate oscillation models. In this case, $L$ is the distance of neutrino travel and $E$ is a measure of the interacting neutrino's energy. While comparisons using allowed and excluded regions for oscillation model parameters are likely the only rigorous method for these comparis…
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This paper explores the use of $L/E$ oscillation probability distributions to compare experimental measurements and to evaluate oscillation models. In this case, $L$ is the distance of neutrino travel and $E$ is a measure of the interacting neutrino's energy. While comparisons using allowed and excluded regions for oscillation model parameters are likely the only rigorous method for these comparisons, the $L/E$ distributions are shown to give qualitative information on the agreement of an experiment's data with a simple two-neutrino oscillation model. In more detail, this paper also outlines how the $L/E$ distributions can be best calculated and used for model comparisons. Specifically, the paper presents the $L/E$ data points for the final MiniBooNE data samples and, in the Appendix, explains and corrects the mistaken analysis published by the ICARUS collaboration.
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Submitted 11 July, 2014;
originally announced July 2014.
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Measurement of the Antineutrino Neutral-Current Elastic Differential Cross Section
Authors:
A. A. Aguilar-Arevalo,
B. C. Brown,
L. Bugel,
G. Cheng,
E. D. Church,
J. M. Conrad,
R. Dharmapalan,
Z. Djurcic,
D. A. Finley,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
W. Huelsnitz,
C. Ignarra,
R. Imlay,
R. A. Johnson,
G. Karagiorgi,
T. Katori,
T. Kobilarcik,
W. C. Louis,
C. Mariani,
W. Marsh,
G. B. Mills,
J. Mirabal
, et al. (20 additional authors not shown)
Abstract:
We report the measurement of the flux-averaged antineutrino neutral current elastic scattering cross section ($dσ_{\bar νN \rightarrow \bar νN}/dQ^{2}$) on CH$_{2}$ by the MiniBooNE experiment using the largest sample of antineutrino neutral current elastic candidate events ever collected. The ratio of the antineutrino to neutrino neutral current elastic scattering cross sections and a ratio of an…
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We report the measurement of the flux-averaged antineutrino neutral current elastic scattering cross section ($dσ_{\bar νN \rightarrow \bar νN}/dQ^{2}$) on CH$_{2}$ by the MiniBooNE experiment using the largest sample of antineutrino neutral current elastic candidate events ever collected. The ratio of the antineutrino to neutrino neutral current elastic scattering cross sections and a ratio of antineutrino neutral current elastic to antineutrino charged current quasi elastic cross section is also presented.
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Submitted 27 September, 2013;
originally announced September 2013.
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Improved Search for $\bar ν_μ\rightarrow \bar ν_e$ Oscillations in the MiniBooNE Experiment
Authors:
The MiniBooNE Collaboration,
A. A. Aguilar-Arevalo,
B. C. Brown,
L. Bugel,
G. Cheng,
E. D. Church,
J. M. Conrad,
R. Dharmapalan,
Z. Djurcic,
D. A. Finley,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
W. Huelsnitz,
C. Ignarra,
R. Imlay,
R. A. Johnson,
G. Karagiorgi,
T. Katori,
T. Kobilarcik,
W. C. Louis,
C. Mariani,
W. Marsh,
G. B. Mills
, et al. (20 additional authors not shown)
Abstract:
The MiniBooNE experiment at Fermilab reports results from an analysis of $\bar ν_e$ appearance data from $11.27 \times 10^{20}$ protons on target in antineutrino mode, an increase of approximately a factor of two over the previously reported results. An event excess of $78.4 \pm 28.5$ events ($2.8 σ$) is observed in the energy range $200<E_ν^{QE}<1250$ MeV. If interpreted in a two-neutrino oscilla…
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The MiniBooNE experiment at Fermilab reports results from an analysis of $\bar ν_e$ appearance data from $11.27 \times 10^{20}$ protons on target in antineutrino mode, an increase of approximately a factor of two over the previously reported results. An event excess of $78.4 \pm 28.5$ events ($2.8 σ$) is observed in the energy range $200<E_ν^{QE}<1250$ MeV. If interpreted in a two-neutrino oscillation model, $\barν_μ\rightarrow\barν_e$, the best oscillation fit to the excess has a probability of 66% while the background-only fit has a $χ^2$-probability of 0.5% relative to the best fit. The data are consistent with antineutrino oscillations in the $0.01 < Δm^2 < 1.0$ eV$^2$ range and have some overlap with the evidence for antineutrino oscillations from the Liquid Scintillator Neutrino Detector (LSND). All of the major backgrounds are constrained by in-situ event measurements so non-oscillation explanations would need to invoke new anomalous background processes. The neutrino mode running also shows an excess at low energy of $162.0 \pm 47.8$ events ($3.4 σ$) but the energy distribution of the excess is marginally compatible with a simple two neutrino oscillation formalism. Expanded models with several sterile neutrinos can reduce the incompatibility by allowing for CP violating effects between neutrino and antineutrino oscillations.
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Submitted 12 March, 2013; v1 submitted 11 March, 2013;
originally announced March 2013.
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First Measurement of the Muon Anti-Neutrino Double-Differential Charged Current Quasi-Elastic Cross Section
Authors:
A. A. Aguilar-Arevalo,
B. C. Brown,
L. Bugel,
G. Cheng,
E. D. Church,
J. M. Conrad,
R. Dharmapalan,
Z. Djurcic,
D. A. Finley,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
W. Huelsnitz,
C. Ignarra,
R. Imlay,
R. A. Johnson,
G. Karagiorgi,
T. Katori,
T. Kobilarcik,
W. C. Louis,
C. Mariani,
W. Marsh,
G. B. Mills,
J. Mirabal
, et al. (20 additional authors not shown)
Abstract:
The largest sample ever recorded of $\numub$ charged-current quasi-elastic (CCQE, $\numub + p \to \mup + n$) candidate events is used to produce the minimally model-dependent, flux-integrated double-differential cross section $\frac{d^{2}σ}{dT_μd\uz}$ for $\numub$ incident on mineral oil. This measurement exploits the unprecedented statistics of the MiniBooNE anti-neutrino mode sample and provides…
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The largest sample ever recorded of $\numub$ charged-current quasi-elastic (CCQE, $\numub + p \to \mup + n$) candidate events is used to produce the minimally model-dependent, flux-integrated double-differential cross section $\frac{d^{2}σ}{dT_μd\uz}$ for $\numub$ incident on mineral oil. This measurement exploits the unprecedented statistics of the MiniBooNE anti-neutrino mode sample and provides the most complete information of this process to date. Also given to facilitate historical comparisons are the flux-unfolded total cross section $σ(E_ν)$ and single-differential cross section $\frac{dσ}{d\qsq}$ on both mineral oil and on carbon by subtracting the $\numub$ CCQE events on hydrogen. The observed cross section is somewhat higher than the predicted cross section from a model assuming independently-acting nucleons in carbon with canonical form factor values. The shape of the data are also discrepant with this model. These results have implications for intra-nuclear processes and can help constrain signal and background processes for future neutrino oscillation measurements.
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Submitted 4 August, 2013; v1 submitted 29 January, 2013;
originally announced January 2013.
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Low Mass WIMP Searches with a Neutrino Experiment: A Proposal for Further MiniBooNE Running
Authors:
A. A. Aguilar-Arevalo,
B. Batell,
R. Cooper,
P. deNiverville,
R. Dharmapalan,
Z. Djurcic,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
S. Habib,
W. Huelsnitz,
C. Jiang,
R. A. Johnson,
W. Ketchum,
T. Kobilarcik,
W. C. Louis,
W. Marsh,
D. McKeen,
G. B. Mills,
J. Mirabal,
C. D. Moore,
P. Nienaber,
Z. Pavlovic,
D. Perevalov
, et al. (8 additional authors not shown)
Abstract:
A proposal submitted to the FNAL PAC is described to search for light sub-GeV WIMP dark matter at MiniBooNE. The possibility to steer the beam past the target and into an absorber leads to a significant reduction in neutrino background, allowing for a sensitive search for elastic scattering of WIMPs off nucleons or electrons in the detector. Dark matter models involving a vector mediator can be pr…
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A proposal submitted to the FNAL PAC is described to search for light sub-GeV WIMP dark matter at MiniBooNE. The possibility to steer the beam past the target and into an absorber leads to a significant reduction in neutrino background, allowing for a sensitive search for elastic scattering of WIMPs off nucleons or electrons in the detector. Dark matter models involving a vector mediator can be probed in a parameter region consistent with the required thermal relic density, and which overlaps the region in which these models can resolve the muon g-2 discrepancy. Estimates of signal significance are presented for various operational modes and parameter points. The experimental approach outlined for applying MiniBooNE to a light WIMP search may also be applicable to other neutrino facilities.
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Submitted 9 November, 2012;
originally announced November 2012.
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Dual baseline search for muon antineutrino disappearance at 0.1 eV^2 < Δm^2 < 100 eV^2
Authors:
MiniBooNE Collaboration,
SciBooNE Collaboration,
G. Cheng,
W. Huelsnitz,
A. A. Aguilar-Arevalo,
J. L. Alcaraz-Aunion,
S. J. Brice,
B. C. Brown,
L. Bugel,
J. Catala-Perez,
E. D. Church,
J. M. Conrad,
R. Dharmapalan,
Z. Djurcic,
U. Dore,
D. A. Finley,
R. Ford,
A. J. Franke,
F. G. Garcia,
G. T. Garvey,
C. Giganti,
J. J. Gomez-Cadenas,
J. Grange,
P. Guzowski,
A. Hanson
, et al. (66 additional authors not shown)
Abstract:
The MiniBooNE and SciBooNE collaborations report the results of a joint search for short baseline disappearance of \bar{ν_μ} at Fermilab's Booster Neutrino Beamline. The MiniBooNE Cherenkov detector and the SciBooNE tracking detector observe antineutrinos from the same beam, therefore the combined analysis of their datasets serves to partially constrain some of the flux and cross section uncertain…
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The MiniBooNE and SciBooNE collaborations report the results of a joint search for short baseline disappearance of \bar{ν_μ} at Fermilab's Booster Neutrino Beamline. The MiniBooNE Cherenkov detector and the SciBooNE tracking detector observe antineutrinos from the same beam, therefore the combined analysis of their datasets serves to partially constrain some of the flux and cross section uncertainties. Uncertainties in the ν_μ background were constrained by neutrino flux and cross section measurements performed in both detectors. A likelihood ratio method was used to set a 90% confidence level upper limit on \bar{ν_μ} disappearance that dramatically improves upon prior limits in the Δm^2=0.1-100 eV^2 region.
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Submitted 5 November, 2012; v1 submitted 1 August, 2012;
originally announced August 2012.
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A Combined $ν_μ\to ν_e$ and $\barν_μ\to \barν_e$ Oscillation Analysis of the MiniBooNE Excesses
Authors:
MiniBooNE Collaboration,
A. A. Aguilar-Arevalo,
B. C. Brown,
L. Bugel,
G. Cheng,
E. D. Church,
J. M. Conrad,
R. Dharmapalan,
Z. Djurcic,
D. A. Finley,
R. Ford,
F. G. Garcia,
G. T. Garvey,
J. Grange,
W. Huelsnitz,
C. Ignarra,
R. Imlay,
R. A. Johnson,
G. Karagiorgi,
T. Katori,
T. Kobilarcik,
W. C. Louis,
C. Mariani,
W. Marsh,
G. B. Mills
, et al. (20 additional authors not shown)
Abstract:
The MiniBooNE experiment at Fermilab reports results from an analysis of the combined $ν_e$ and $\bar ν_e$ appearance data from $6.46 \times 10^{20}$ protons on target in neutrino mode and $11.27 \times 10^{20}$ protons on target in antineutrino mode. A total excess of $240.3 \pm 34.5 \pm 52.6$ events ($3.8 σ$) is observed from combining the two data sets in the energy range $200<E_ν^{QE}<1250$ Me…
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The MiniBooNE experiment at Fermilab reports results from an analysis of the combined $ν_e$ and $\bar ν_e$ appearance data from $6.46 \times 10^{20}$ protons on target in neutrino mode and $11.27 \times 10^{20}$ protons on target in antineutrino mode. A total excess of $240.3 \pm 34.5 \pm 52.6$ events ($3.8 σ$) is observed from combining the two data sets in the energy range $200<E_ν^{QE}<1250$ MeV. In a combined fit for CP-conserving $ν_μ\rightarrow ν_e$ and $\barν_μ\rightarrow\barν_e$ oscillations via a two-neutrino model, the background-only fit has a $χ^2$-probability of 0.03% relative to the best oscillation fit. The data are consistent with neutrino oscillations in the $0.01 < Δm^2 < 1.0$ eV$^2$ range and with the evidence for antineutrino oscillations from the Liquid Scintillator Neutrino Detector (LSND).
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Submitted 27 August, 2012; v1 submitted 19 July, 2012;
originally announced July 2012.