MINERvA measures antineutrino cross sections on multiple nuclei versus transverse momentum and finds significant model discrepancies indicating missing nuclear effects.
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representative citing papers
DUNE can set competitive bounds on refractive neutrino masses via supernova time-of-flight, with sensitivity significantly enhanced by galactic dark matter density spikes.
Tripartite entanglement entropy distinguishes neutrino mass hierarchy and CP phases, amplified twofold by MSW matter effects, with a linear CP-independent relation to the NSI parameter ε_ee and stable optimal L/E ≈ 655 km/GeV.
Lattice QCD yields the singlet axial form factor G_A^{u+d+s}(Q^2) and strange G_A^s(Q^2) with full error budget after chiral, continuum, and infinite-volume extrapolations.
Solar g-modes cause undetectable time-varying neutrino flux fluctuations but a non-negligible net mean flux increase proportional to mode amplitude squared that may vary over the 11-year solar activity cycle.
Radiative corrections applied to MINERvA antineutrino data yield updated values for the nucleon axial-vector form factor G_A and axial radius.
Supervised ML classification of neutrino events by interaction channel prior to energy reconstruction improves accuracy and sensitivity by 10-20% in simulated DUNE analyses while remaining robust to generator mismodeling.
Realistic variations in final-state interaction modeling can distort reconstructed neutrino energy spectra in DUNE-like experiments by amounts comparable to or exceeding those from changes in Δm²₃₂ or δ_CP, creating a potential degeneracy.
A new correlation-exploiting parameter is introduced for dual-baseline neutrino oscillation experiments to aid determination of mass hierarchy and CP phase, analyzed in the T2HKK context.
In neutrino oscillations treated as open quantum systems, coherence outlasts steering and negativity under amplitude damping, phase flip, and phase damping, showing memory-induced revivals in non-Markovian regimes.
Realistic Earth density profiles introduce energy-dependent structures in neutrino oscillation probabilities that path-averaged models miss, potentially biasing CP phase inference in long-baseline experiments.
citing papers explorer
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Measurement of Inclusive Charged-Current $\bar{\nu}_{\mu}$ Scattering on C, CH, Fe, and Pb at $\langle E_{\bar{\nu}}\rangle \sim$ 6 GeV with MINERvA
MINERvA measures antineutrino cross sections on multiple nuclei versus transverse momentum and finds significant model discrepancies indicating missing nuclear effects.
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Shedding light on dark matter spikes through refractive neutrino masses
DUNE can set competitive bounds on refractive neutrino masses via supernova time-of-flight, with sensitivity significantly enhanced by galactic dark matter density spikes.
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Tripartite Entanglement as a Probe of Neutrino Mass Hierarchy, CP Violation, and Non-Standard Interactions
Tripartite entanglement entropy distinguishes neutrino mass hierarchy and CP phases, amplified twofold by MSW matter effects, with a linear CP-independent relation to the NSI parameter ε_ee and stable optimal L/E ≈ 655 km/GeV.
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The strange and flavor-singlet axial form factors of the nucleon from lattice QCD
Lattice QCD yields the singlet axial form factor G_A^{u+d+s}(Q^2) and strange G_A^s(Q^2) with full error budget after chiral, continuum, and infinite-volume extrapolations.
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Solar Neutrino Flux Fluctuations Caused by Solar Gravity Modes
Solar g-modes cause undetectable time-varying neutrino flux fluctuations but a non-negligible net mean flux increase proportional to mode amplitude squared that may vary over the 11-year solar activity cycle.
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Nucleon axial-vector form factor and radius from radiatively-corrected antineutrino scattering data
Radiative corrections applied to MINERvA antineutrino data yield updated values for the nucleon axial-vector form factor G_A and axial radius.
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Improving Neutrino Oscillation Measurements through Event Classification
Supervised ML classification of neutrino events by interaction channel prior to energy reconstruction improves accuracy and sensitivity by 10-20% in simulated DUNE analyses while remaining robust to generator mismodeling.
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The role of final-state interaction modeling in neutrino energy reconstruction and oscillation measurements
Realistic variations in final-state interaction modeling can distort reconstructed neutrino energy spectra in DUNE-like experiments by amounts comparable to or exceeding those from changes in Δm²₃₂ or δ_CP, creating a potential degeneracy.
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Neutrino oscillations at dual baselines
A new correlation-exploiting parameter is introduced for dual-baseline neutrino oscillation experiments to aid determination of mass hierarchy and CP phase, analyzed in the T2HKK context.
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Dephasing Effects on the Dynamical Evolution of Quantum Correlations and Coherence in Neutrino Oscillations
In neutrino oscillations treated as open quantum systems, coherence outlasts steering and negativity under amplitude damping, phase flip, and phase damping, showing memory-induced revivals in non-Markovian regimes.
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Earth-Density Effects in Long Baseline Neutrino Experiments
Realistic Earth density profiles introduce energy-dependent structures in neutrino oscillation probabilities that path-averaged models miss, potentially biasing CP phase inference in long-baseline experiments.
- Irreducible Gravitational Wave Background as a Particle Detector
- The High W Challenge: Robust Neutrino Energy Estimators for LArTPCs