{"total":19,"items":[{"citing_arxiv_id":"2606.12915","ref_index":78,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Mass Varying Neutrino Oscillation in Teleparallel Gravity","primary_cat":"hep-ph","submitted_at":"2026-06-11T05:18:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Torsion-coupled scalar in teleparallel gravity induces density-dependent neutrino masses that alter MSW resonance and yield constraints on coupling parameters from Super-Kamiokande, Borexino and SNO data.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.08070","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Earth-Density Stratification and Quantum Gravity Corrections in Long-Baseline Neutrino Oscillation Experiments","primary_cat":"hep-ph","submitted_at":"2026-06-06T09:34:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Unified calculation shows Earth density stratification biases CP phase up to 172 degrees at 12000 km baselines, with Planck-scale corrections partially compensating at 7000 km for certain Majorana phases.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06580","ref_index":6,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Neutrino mass ordering from the next Galactic supernova at DUNE, HK, and JUNO","primary_cat":"hep-ph","submitted_at":"2026-06-04T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Neutronization burst and accretion-phase rise-time observables from a 10 kpc core-collapse supernova enable DUNE, HK and JUNO to discriminate neutrino mass ordering at 3-6 sigma using multiple progenitor simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.00745","ref_index":125,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Comparisons of triple-differential cross sections for quasielastic-like $\\nu_\\mu$-hydrocarbon interactions using $\\langle E_\\nu\\rangle \\sim$ 3~GeV versus $\\sim$ 6~GeV beams in MINERvA","primary_cat":"hep-ex","submitted_at":"2026-05-30T14:25:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"MINERvA compares quasielastic-like cross sections at two neutrino beam energies and finds discrepancies pointing to overestimated final state interactions for protons and pions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.31600","ref_index":79,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gravitational Waves from hybrid defects as probe of Flavor symmetry breaking: Machine-Learning Approach","primary_cat":"astro-ph.CO","submitted_at":"2026-05-29T17:59:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Hybrid string-bounded domain wall networks from sequential U(1)_F and Z2 symmetry breaking generate a GW spectrum with a unique low-frequency slope that future detectors can observe and an MLP surrogate can characterize for fast SNR inference.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.24224","ref_index":5,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"High Statistics Measurements of $\\nu_{\\mu}$ Charged-Current Single $\\pi^{+}$ Production with Zero Pion Kinetic Energy Threshold in MINERvA","primary_cat":"hep-ex","submitted_at":"2026-05-22T21:11:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"High-statistics measurement of νμ CC 1π+ production cross sections on scintillator with zero pion KE threshold shows modern models disagree with data by up to 20% in key regions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.10972","ref_index":23,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Tripartite Entanglement as a Probe of Neutrino Mass Hierarchy, CP Violation, and Non-Standard Interactions","primary_cat":"hep-ph","submitted_at":"2026-05-08T20:18:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"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.","context_count":1,"top_context_role":"baseline","top_context_polarity":"baseline","context_text":"Using the global linear entropy as our entanglement measure, we introduce the hierarchy sensitivity diagnostic ∆Sand study how it responds to each of the above effects. We also propose its neutrino-antineutrino decomposition as a tool to independently isolate the CP-asymmetry signal and the matter-hierarchy signal. All results are benchmarked against the DUNE experiment [23] atL= 1300 km. 2 Theoretical Framework 2.1 Oscillation Probabilities Flavor eigenstates (νe, νµ, ντ) are related to mass eigenstates (ν 1, ν2, ν3) via the PMNS matrix [1, 2]: U=   c12c13 s12c13 s13e−iδCP −s12c23 −c 12s23s13eiδCP c12c23 −s 12s23s13eiδCP s23c13 s12s23 −c 12c23s13eiδCP −c12s23 −s 12c23s13eiδCP c23c13   ,(1) wherec ij = cosθ ij,s ij = sinθ ij."},{"citing_arxiv_id":"2605.06559","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The strange and flavor-singlet axial form factors of the nucleon from lattice QCD","primary_cat":"hep-lat","submitted_at":"2026-05-07T16:53:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"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.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"(u+d−2s), and singlet (u+d+s) components. These channels probe distinct aspects of QCD: the isovector channel is sensitive toWboson exchange, whereas the isoscalar currents are sensitive toZboson scattering, which also receives contributions from the strange quark. In particular, the isovector channel is relevant in the anal- ysis of upcoming neutrino experiments [4, 5], whereas channels involvingZboson exchange and sea-quark con- tributions are needed as input for the precise extrac- tion of the weak charge of the proton in the upcoming P2 experiment [6]. Furthermore, the strange component Gs A(Q2) is crucial for calculating the cross-section within various dark matter models [7]: in this context, it is par-"},{"citing_arxiv_id":"2605.05015","ref_index":56,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Dephasing Effects on the Dynamical Evolution of Quantum Correlations and Coherence in Neutrino Oscillations","primary_cat":"quant-ph","submitted_at":"2026-05-06T15:13:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"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.","context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"(T2K Collaboration),Observation of Electron Neutrino Appearance in a Muon Neutrino Beam, Phys. Rev. Lett.111, 211803 (2013), arXiv:1308.0465 [hep-ex]. [54] F. An et al. (JUNO Collaboration),Neutrino Physics with JUNO, J. Phys. G43, 030401 (2016), arXiv:1507.05613 [physics.ins-det]. [55] A. Abusleme et al. (JUNO Collaboration),The JUNO Experiment: Status and Prospects, Prog. Part. Nucl. Phys.103, 92 (2021), arXiv:2104.02565 [hep-ex]. [56] R. Acciarri et al. (DUNE Collaboration),Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE), arXiv:1512.06148 [physics.ins-det]. [57] B. Abi et al. (DUNE Collaboration),Deep Underground Neutrino Experiment (DUNE), Eur. Phys. J. C80, 978 (2020), arXiv:2006.16043 [hep-ex]. [58] M. M. Guzzo, P. C. de Holanda and R. L."},{"citing_arxiv_id":"2604.20792","ref_index":83,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Irreducible Gravitational Wave Background as a Particle Detector","primary_cat":"hep-ph","submitted_at":"2026-04-22T17:17:40+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"K. Verma (2026), 2604.00866. [78] J. L. Feng, I. Galon, F. Kling, and S. Trojanowski, Phys. Rev. D97, 055034 (2018), 1710.09387. [79] A. Ariga et al. (FASER), Phys. Rev. D99, 095011 (2019), 1811.12522. [80] A. Ariga et al. (FASER) (2018), 1812.09139. [81] A. Ariga et al. (FASER) (2019), 1901.04468. [82] R. Acciarri et al. (DUNE) (2015), 1512.06148. [83] J. M. Berryman, A. de Gouvea, P. J. Fox, B. J. Kayser, K. J. Kelly, and J. L. Raaf, JHEP02, 174 (2020), 1912.07622. [84] B. Batell, J. A. Evans, S. Gori, and M. Rai, JHEP05, 049 (2021), 2008.08108. [85] D. Curtin et al., Rept. Prog. Phys.82, 116201 (2019), 1806.07396. [86] G. Bernardi et al., Phys. Lett. B166, 479 (1986). [87] D. Gorbunov, I. Krasnov, and S."},{"citing_arxiv_id":"2604.07091","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"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","primary_cat":"hep-ex","submitted_at":"2026-04-08T13:44:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"MINERvA measures antineutrino cross sections on multiple nuclei versus transverse momentum and finds significant model discrepancies indicating missing nuclear effects.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.06535","ref_index":2,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Solar Neutrino Flux Fluctuations Caused by Solar Gravity Modes","primary_cat":"astro-ph.SR","submitted_at":"2026-04-08T00:12:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"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.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2601.21256","ref_index":6,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Earth-Density Effects in Long Baseline Neutrino Experiments","primary_cat":"hep-ph","submitted_at":"2026-01-29T04:31:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"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.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2601.21155","ref_index":62,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Nucleon axial-vector form factor and radius from radiatively-corrected antineutrino scattering data","primary_cat":"hep-ph","submitted_at":"2026-01-29T01:30:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Radiative corrections applied to MINERvA antineutrino data yield updated values for the nucleon axial-vector form factor G_A and axial radius.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"the fit without the radiative corrections, when the nucleon vector form factors are fixed to thez-expansion parameterization from Ref. [39]. 5.2 DUNE, Hyper-K, MINERvA, and BEBC pseudodata In this Section, we study the effects of radiative corrections on the nucleon axial-vector form factor and radius that are extracted from simulated pseudodata. These pseudodata samples were created assuming muon neutrino fluxes from the DUNE [62, 63] and Hyper-K [64] technical design reports, and for the fluxes from the MINERvA [9, 65] and BEBC [8, 66] experiments. Neglecting uncertainties on the incoming flux, we generate ten random flux-integrated differential cross sections for four choices of the incoming muon neutrino flux at DUNE, Hyper-K, MINERvA, and BEBC experiments, to act as \"near detectors\" in oscillation experiments."},{"citing_arxiv_id":"2511.11938","ref_index":47,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Improving Neutrino Oscillation Measurements through Event Classification","primary_cat":"hep-ph","submitted_at":"2025-11-14T23:26:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"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.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.11149","ref_index":3,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The High W Challenge: Robust Neutrino Energy Estimators for LArTPCs","primary_cat":"physics.data-an","submitted_at":"2025-11-14T10:27:25+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.03964","ref_index":9,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The role of final-state interaction modeling in neutrino energy reconstruction and oscillation measurements","primary_cat":"hep-ex","submitted_at":"2025-11-06T01:33:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"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.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2508.10983","ref_index":49,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Shedding light on dark matter spikes through refractive neutrino masses","primary_cat":"hep-ph","submitted_at":"2025-08-14T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"UNKNOWN","novelty_score":6.0,"formal_verification":"none","one_line_summary":"DUNE can set competitive bounds on refractive neutrino masses via supernova time-of-flight, with sensitivity significantly enhanced by galactic dark matter density spikes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1907.01185","ref_index":22,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Neutrino oscillations at dual baselines","primary_cat":"hep-ph","submitted_at":"2019-07-02T06:12:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"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.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}