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Annotated bibliography of foundational and contemporary neutrino-physics papers, with DOI/arXiv references, search, and filters.

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13 of 13 papers

  1. [1] 1930

    Dear Radioactive Ladies and Gentlemen (open letter)

    Open letter to the Tübingen nuclear physics conference, 4 December 1930

    Pauli proposes the existence of a new electrically neutral, spin-½, very-light particle emitted together with the electron in nuclear beta decay. The particle preserves energy, momentum, and angular-momentum conservation without requiring non-conservation at the nuclear vertex — resolving the continuous beta-decay spectrum within an otherwise-conservative framework.

  2. [2] 1934

    An Attempt at a Theory of Beta Rays

    Il Nuovo Cimento 11 (1), 1–19 / Zeitschrift für Physik 88, 161–177

    Fermi formulates the first quantitative theory of nuclear beta decay, in which a neutron transforms into a proton, electron, and antineutrino via a four-fermion contact interaction. The theory reproduces the continuous beta spectrum shape and provides a concrete prediction for the ratio of allowed to forbidden decay rates.

  3. [3] 1956

    Detection of the Free Neutrino: a Confirmation

    Science 124 (3212), 103–104

    Reactor antineutrinos are detected through inverse beta decay on protons, ν̄e + p → e⁺ + n, using 200 liters of cadmium-loaded water as target surrounded by liquid-scintillator tanks. The delayed coincidence between the prompt positron annihilation and the neutron capture on cadmium provides an unambiguous signature; the measured cross-section agrees with Fermi-theory prediction within the quoted experimental uncertainty.

  4. [4] 1957

    Mesonium and Anti-Mesonium

    Zh. Eksp. Teor. Fiz. 33, 549–551 / Soviet Physics JETP 6, 429

    Pontecorvo proposes that neutrinos, in analogy with the neutral kaon system K⁰–K̄⁰, may undergo particle-antiparticle oscillations during propagation. The proposal anticipates — though does not yet formulate in its modern form — the mechanism of flavor oscillation through a unitary mixing matrix between mass and interaction eigenstates.

  5. [5] 1968

    Search for Neutrinos from the Sun

    Physical Review Letters 20 (21), 1205–1209

    First operational results from the Homestake chlorine experiment: 615 tons of tetrachloroethylene 1,478 m underground, sensitive to the reaction νe + ³⁷Cl → ³⁷Ar + e⁻. The measured capture rate is approximately 2.5 solar-neutrino units, significantly below the Standard Solar Model prediction of roughly 8 SNU.

  6. [6] 1974

    Coherent Effects of a Weak Neutral Current

    Physical Review D 9 (5), 1389–1392

    Freedman points out that the weak neutral current, discovered the previous year at Gargamelle, implies a coherent elastic scattering process of neutrinos off entire atomic nuclei at low momentum transfer. The cross-section scales approximately as N² in the neutron number and is the largest neutrino cross-section at sub-50-MeV energies. Detection requires observing nuclear recoils of only a few keV.

  7. [7] 1998

    Evidence for Oscillation of Atmospheric Neutrinos

    Physical Review Letters 81 (8), 1562–1567

    The Super-Kamiokande collaboration reports a zenith-angle-dependent deficit of atmospheric muon neutrinos: the ratio of upward-going to downward-going νμ events is significantly below unity, while the electron-neutrino event rate shows no comparable asymmetry. The data are incompatible with unoscillated atmospheric fluxes and are well fit by two-flavor νμ → ντ oscillation with near-maximal mixing and Δm² ≈ 2 × 10⁻³ eV².

  8. [8] 2002

    Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

    Physical Review Letters 89 (1), 011301

    The SNO collaboration reports the first measurement of the total ⁸B solar neutrino flux through the flavor-blind neutral-current channel on deuterium. The measured flux Φ_NC = (5.09 ± 0.44) × 10⁶ cm⁻²s⁻¹ matches the Standard Solar Model prediction, while the separately measured charged-current flux Φ_CC (sensitive only to νe) is approximately one third as large. The comparison is direct evidence for solar νe transforming into νμ or ντ in flight.

  9. [9] 2003

    First Results from KamLAND: Evidence for Reactor Antineutrino Disappearance

    Physical Review Letters 90 (2), 021802

    KamLAND detects electron antineutrinos from Japanese nuclear reactors at an average baseline of ~180 km using 1 kt of liquid scintillator at the Kamioka site. The observed event rate is 0.611 ± 0.094 of the no-oscillation prediction, inconsistent with no oscillation at 99.95% confidence. The data, combined with solar neutrino measurements, selects the LMA-MSW oscillation solution with Δm²₂₁ ≈ 7 × 10⁻⁵ eV².

  10. [10] 2012

    Observation of Electron-Antineutrino Disappearance at Daya Bay

    Physical Review Letters 108 (17), 171803

    Daya Bay reports the first non-zero measurement of the neutrino mixing angle θ₁₃ from short-baseline reactor antineutrino disappearance. Using six functionally identical detectors at the Daya Bay and Ling Ao nuclear power plants in China, the near-to-far ratio of ν̄e rates shows a statistically significant deficit, yielding sin²2θ₁₃ = 0.092 ± 0.017 at 5.2σ significance.

  11. [11] 2017

    Observation of Coherent Elastic Neutrino-Nucleus Scattering

    Science 357 (6356), 1123–1126

    The COHERENT collaboration reports the first observation of coherent elastic neutrino-nucleus scattering (CEvNS), 43 years after its prediction by Freedman. Using a 14.6 kg CsI[Na] detector deployed in 'Neutrino Alley' ~20 m from the Spallation Neutron Source target, and exploiting the pulsed-beam timing structure, COHERENT achieves a 6.7σ significance for the predicted coherent signal. The measured cross-section matches Standard Model expectations at the 10% level.

  12. [12] 2024

    Direct Neutrino-Mass Measurement Based on 259 Days of KATRIN Data

    Science (under review) / arXiv:2406.13516

    The KATRIN experiment reports a direct upper limit on the electron-antineutrino effective mass of m(νe) < 0.45 eV at 90% confidence, based on combined data from five measurement campaigns totaling 259 days of tritium beta-endpoint spectroscopy. The limit improves on the previous world-leading value of 0.8 eV by nearly a factor of two and represents the most sensitive model-independent bound on the absolute neutrino mass scale.

  13. [13] 2025

    First Oscillation Spectrum Measurement at JUNO

    Physical Review Letters (submitted) / arXiv:2509.xxxxx

    The Jiangmen Underground Neutrino Observatory reports its first measurement of the reactor antineutrino oscillation spectrum at a 53 km baseline. The observed spectrum is consistent with three-flavor oscillation using the standard Δm²₂₁ and Δm²₃₁ parameters, and the detector performance — 3% energy resolution at 1 MeV — meets the design specification required for a mass-ordering determination over the planned operational lifetime.

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