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1. Neutrino Oscillation 1. Neutrino Oscillation 1 2 3 θ13 θ12 θ23 θ12 θ13 θ23 Gaol of RENO experiment = θ13 1. Neutrino Oscillation νe νe νe νe νe Distance Probability…
Microsoft PowerPoint - Kearns-NUSS2007-Neutrino-Detectors-I-print.pptNeutrino Detectors I Inverse Beta Decay Tracking Detectors Two ν Experiment NuTeV, MINOS,
Motivation ν masses from ν oscillation are a clear signature of physics beyond SM access to very high new physics scale (M NP ) Oscillation parametrized with neutrino
PowerPoint Jun. 7, 2021 2 || = CKM Hierarchy! || = PMNS Approximate μ-τ symmetry? Fundamental problem: neutrino absolute masses? Quarks vs. Leptons: A big puzzle of
Long-range programme in neutrino physics: superbeam, β beam, neutrino factory Complementary programme in μ physics: rare μ decays, μ properties, μ colliders? Next-generation…
Have neutrinos to do with Dark Energy ? Why neutrinos may play a role Mass scales : Dark Energy density : ρ ~ ( 2×10 -3 eV )- 4. Neutrino mass : eV or below. Cosmological…
Ionization Cooling – neutrinos, colliders and beta-beams David Neuffer July 2009 Outline Front End and Cooling – IDS neutrino factory Study 2A – ISS baseline example…
PHY418 Particle Astrophysics PHY418 Particle Astrophysics High Energy Neutrinos 1 Neutrino astrophysics 2 Relevant to high energy particle astrophysics essentially undetectable…
Neutrinos at the SNS (Spallation Neutron Source) * Yu.Efremenko 0. A little bit of Modern Neutrino History Why Low Energy Neutrinos are Good 2. Some Proposed Neutrino Experiments…
Have neutrinos to do with Dark Energy ? Why neutrinos may play a role Mass scales : Dark Energy density : ρ ~ ( 2×10 -3 eV )- 4. Neutrino mass : eV or below. Cosmological…
Supernova neutrinos - Collective and matter effects at large detectorsAmol Dighe Changing paradigm of SN neutrino oscillations Neutrino-electron forward scattering: MSW effects
CHOOZ DETECTOR Directores del trabajo: Indice 3. EL EXPERIMENTO DOUBLE CHOOZ 4 4. CARACTERIZACION DEL RUIDO DE LA ELECTRONICA 7 5. CALCULO DE LA GANANCIA 8 6. CONCLUSIONES
Confirming as a solution for with neutrinosRegular Article - Theoretical Physics Confirming U(1)Lμ−Lτ as a solution for (g − 2)μ with neutrinos D. W.
Phenomenology with Massive Neutrinos Concha Gonzalez-Garcia PHENOMENOLOGY WITH MASSIVE NEUTRINOS Concha Gonzalez-Garcia YITP Stony Brook ICREA U. Barcelona UB, June 1tth,…
reconstructed vT candidate event Caren Hagner, Universität Hamburg DESY Seminar, 12.10.2010 VARIABLE Value kink (mrad) 41 ± 2 decay length (mm) 1335 ± 35 P (daughter)…
Neutrino lumps connection between dark energy and neutrino properties present equation of state given by neutrino mass ! present dark energy density computable in terms of…
Ionization cross sections of neutrino electronagnetic interactions with electrons Chih-Pan Wu Dept of Physics National Taiwan University P 1 Reference: Phys Lett B 731 159…
An Investigation of Matter Enhanced Neutrino Oscillation with the Sudbury Neutrino Observatory Miles Walter Eldon Smith A dissertation submitted in partial fulfillment of…
Neutrino Factory, ± Decay Rings C Johnstone, FNAL, F Meot, CEA, & G H Rees, RAL Vertical Plane Layout for 2 Isosceles Triangle Rings ν ν -----------------------…
Physics Goal Value of measuring sin22θ13 to 0.01 using reactor antineutrino has been well documented: Clean, Fast, and Cheap! Daya Bay Experiment will measure sin22θ13…