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  1. 3781
    por Peruzzo, Letizia
    Publicado 2018
    “…New limits on heavy neutrinos from kaon decays into pions, muons and positrons are presented in this report.…”
    Enlace del recurso
    Enlace del recurso
    Search for heavy neutrinos at the NA48/2 and NA62 experiments at CERN
  2. 3782
    “…Beta - neutrino correlation measurements are key in the research of physics beyond the Standard Model. …”
    Enlace del recurso
    Enlace del recurso
    Scalar current limit from the beta-neutrino correlation: the WISArD experiment
  3. 3783
    por Fiorillo, D F G
    Publicado 2020
    “…We consider a minimal type-I seesaw neutrino mass mechanism model with two heavy neutral leptons (right-handed or sterile neutrinos) with arbitrary masses. …”
    Enlace del recurso
    Enlace del recurso
    Investigating two heavy neutral leptons neutrino seesaw mechanism at SHiP
  4. 3784
    por Lanceri, Livio
    Publicado 1987
    “…Indeed, a unique value of this parameter can explain the couplings measured in many different processes, including leptonic and semileptonic neutrino scattering, asymmetries in electron-nucleon, electron-positron, and muon interactions, parity violating effects in atomic transitions, and the masses of the W and z bosons. $^{2}$…”
    Enlace del recurso
    Enlace del recurso
    A precise determination of the electroweak mixing angle from semileptonic neutrino scattering
  5. 3785
    por Kent, N J M
    Publicado 2001
    Enlace del recurso
    Investigation of the interaction muon-neutrino N --> K0(s) mu+ mu- X
  6. 3786
    Enlace del recurso
    CERN neutrinos to Gran Sasso (CNGS): Status and future proton beam options
  7. 3787
    “…Comparison of the flux measured at large underground neutrino experiments with geologically informed predictions of geoneutrino emission from the crust provide the critical test needed to define the mantle’s radiogenic power. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    Revealing the Earth’s mantle from the tallest mountains using the Jinping Neutrino Experiment
  8. 3788
    “…The demand to process billions of neutrino events with many machine learning algorithm inferences creates a computing challenge. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    GPU-Accelerated Machine Learning Inference as a Service for Computing in Neutrino Experiments
  9. 3789
    “…According to the data of the LVD neutrino telescope for 29 years of operation (1992–2021), an experimental limitation on the frequency of neutrino bursts from gravitational collapses of stars in the Galaxy was obtained: less than 1 event in 12.6 years ([Formula: see text] year[Formula: see text]) at a 90[Formula: see text] confidence level.…”
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    Search for Neutrino Radiation from the Collapse of Stellar Cores Using LVD Detector
  10. 3790
    Publicado 1969
    Enlace del recurso
    Around the Laboratories: Brookhaven: 7 foot model. Batavia: Neutrino plans. Serpukhov: Neutrino plans. Heidelberg: New acceleration scheme. Minnesota: Close down of PLA. Los Alamos: LAMPF construction
  11. 3791
    por Zichichi, Antonino
    Publicado 2012
    “…The LVD time stability allows to establish a time-shift in the OPERA experiment, thus providing the first proof against Superluminal neutrinos, using the horizontal muons of the "Teramo Anomaly". …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Time-Shift in the OPERA set-up: proof against superluminal neutrinos without the need of knowing the CERN-LNGS distance and Reminiscences on the origin of the Gran Sasso Lab, of the 3rd neutrino and of the "Teramo Anomaly"
  12. 3792
    por Schwetz, Thomas
    Publicado 2006
    “…The sensitivity of future neutrino oscillation experiments is determined within a frequentist framework by using a statistical procedure based on Monte Carlo simulations. …”
    Enlace del recurso
    Enlace del recurso
    What is the probability that $\theta_{13}$ and CP violation will be discovered in future neutrino oscillation experiments?
  13. 3793
    por CERN. Geneva
    Publicado 2001
    Enlace del recurso
    Search for the neutral Higgs boson in the neutrino channel at sqrts =192-202 GeV
  14. 3794
    Enlace del recurso
    5th International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region
  15. 3795
    por Hartmann, R
    Publicado 1975
    Enlace del recurso
    Enlace del recurso
    A magnetized focusing iron shield against muons in high-energy neutrino beams
  16. 3796
    Publicado 2007
    Enlace del recurso
    Des faisceaux de neutrinos ont parcouru 732km sous les Alpes
  17. 3797
    por Wachsmuth, H W
    Publicado 1979
    Enlace del recurso
    Neutrino and muon fluxes in the CERN 400 GeV proton beam dump experiments
  18. 3798
    por Schwetz, Thomas
    Publicado 2007
    Enlace del recurso
    What is the probability that $\theta_{13}$ and CP Violation will be discovered in future neutrino oscillation experiments ?
  19. 3799
    por Schwetz, Thomas
    Publicado 2007
    “…Standard active-sterile neutrino oscillations do not provide a satisfactory description of the LSND evidence for neutrino oscillations together with the constraints from MiniBooNE and other null-result short-baseline oscillation experiments. …”
    Enlace del recurso
    Enlace del recurso
    LSND versus MiniBooNE: Sterile neutrinos with energy dependent masses and mixing?
  20. 3800
    Publicado 2007
    “…The reconstruction of the core of a neutrino interaction at OPERA. The neutrino arriving from the left of the image has interacted with the lead of a brick, producing various particles identifiable by their tracks visible in the emulsion.…”
    Enlace del recurso
    First neutrino events seen by the core of the OPERA experiment (CNGS) on 2 October 2007
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