Search results for Neutrinos: Phenomenology and Eligio Lisi INFN, Bari, Italy Neutrinos: Phenomenology and Interpretation

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Esteban Roulet CONICET, Bariloche, Argentina PEV NEUTRINOS FROM THE PROPAGATION OFPEV NEUTRINOS FROM THE PROPAGATION OF ULTRA-HIGH ENERGY COSMIC RAYSULTRA-HIGH ENERGY COSMIC…

MuCool Status and Plans Neutrinos from Stored Muons nSTORM n physics with a μ storage ring Outline Historical context Physics motivation The facility Physics potential Project…

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…

ATMOSPHERIC NEUTRINOS Large uncertainties ~20% on absolute normalization but useful well known quantities can be singled out Super-Kamiokande response curves Atmospheric…

1 Using Neutrinos as a Probe of the Strong Interaction Neutrino Anti-neutrino Deep-Inelastic Scattering off of Massive Nuclear Targets e-Nucleus XI Elba – June, 2010 Jorge…

ANTI-NEUTRINOS- DIRAC OR MAJORANA Ettore Fiorini Berkeley October 28 2005 ν=ν− or ν≠ν− Lepton number conservation or violation Has neutrino a finite mass 100 %…

Neutrinos Beyond the νStandard Model Belén Gavela Universidad Autónoma de Madrid and IFT BeyondStandardModel because 1 Experimental evidence for new particle physics:…

Prepared for submission to JHEP Neutrinos as flavor eigenstates: Interactions and oscillations in neutron β decay Cheng-Yang Lee Manipal Centre for Natural Sciences, Centre…

Physics of Massive Neutrinos Concha Gonzalez-Garcia PHYSICS OF MASSIVE NEUTRINOS Concha Gonzalez-Garcia ICREA-University of Barcelona YITP-Stony Brook Nufact07 Summer Institute…

Astrophysical Neutrinos Neutrinos as probes HQL Munich October 16th-20th 2006 L Oberauer TU Munich Energy Spectra of Astrophysical Neutrinos thermal sources Non-thermal sources…

Slide 1 1 Ionization Cooling – neutrinos, colliders and beta-beams David Neuffer July 2009 Slide 2 2Outline  Front End and Cooling – IDS neutrino factory  Study…

Down-Going UHE Neutrinos In The Pierre Auger Observatory + Neutrino Follow-Up Of GW Michael Schimp on behalf of the Pierre Auger Collaboration October 11 2016 UHE EeV ν…

GRBs are one of the leading candidates for the source of the highest energy cosmic rays. Protons accelerated along with the electrons in GRB would interact with the ambient…

The sixth Astrophysical Multimessenger Observatory NetworkAMON Workshop May 22, 2019 Detection of supernova neutrinos at Super-Kamiokande 1 M. Nakahata Kamioka Observatory,…

Physics of Massive Neutrinos Concha Gonzalez-Garcia Plan of Lectures I Standard Neutrino Properties and Mass Terms Beyond Standard II Effects of ν Mass: Neutrino Oscillations…

Fisica del neutrino (con massa) Eligio Lisi INFN, Sezione di Bari Dip. di Fisica & INFN, Milano Bicocca 14 Marzo 2007 1 Schema: • Un po’ di storia • Le oscillazioni…

ar X iv :h ep -p h 01 03 06 5v 2 7 N ov 2 00 1 Oscillating neutrinos and µ → e γ JA Casas1∗and A Ibarra12† 1 Instituto de Estructura de la Materia CSIC Serrano 123…

Neutrino Mass Ordering: Hints and Challenges ß René Magri+e Voice of Space 1931 Eligio Lisi INFN Bari Italy Solvay ν Workshop Brussels 2017 OUTLINE: •  Prologue: 3ν…

Fisica del neutrino: stato e prospettive Eligio Lisi INFN, Sezione di Bari Univ. di Roma “La Sapienza” 29 Aprile 2005 1 Schema: • Un po’ di storia • Le oscillazioni…

MuCool Status and Plans Neutrinos from Stored Muons nSTORM n physics with a μ storage ring And Beyond Outline Introduction Physics motivation Current facility design status…