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RELIC NEUTRINOS: NEUTRINO PROPERTIES FROM COSMOLOGY Sergio Pastor (IFIC) ν RELIC NEUTRINOS: OUTLINE Massive neutrinos Standard neutrinos Extra radiation and Neutrino asymmetries…
Study of neutrino oscillations with ANTARES J. Brunner Method : Use event ratios MC events with oscillations Split into Non-oscillation event rate Oscillation correction…
Neutrino interaction measurements in K2K SciBar RCCN Neutrino Workshop December 10, 2004, Kashiwa M.Hasegawa (Kyoto-Univ.) For the K2K SciBar Group Table of Contents Introduction…
Future Reactor and Solar Neutrino Facilities S. Biller, Oxford University near Reactor Experiments (13) Distance Probability νe 1.0 Eν ≤ 8 MeV Well understood,…
Opportunities for neutrino experiments at ISOLDE Tânia Melo Mendonça IFIMUP, Porto University and CERN High Power Targetry Brainstorming Day Outline Beta beams within the…
Hunting for Cosmological Neutrino Background (CvB) Gianpiero Mangano INFN, Sezione di Napoli, Italy NO-VE 2008 G. Mangano NO-VE 2008 CvB standard features Neutrinos decoupled…
Cosmological Aspects of Neutrino Physics (I) Sergio Pastor (IFIC) 61st SUSSP St Andrews, August 2006 ν Cosmological Aspects of Neutrino Physics 1st lecture Introduction:…
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)…
PowerPoint Presentation Inflationary Freedom and Cosmological Neutrino Constraints Roland de Putter JPL/Caltech CosKASI 4/16/2014 The absolute mass scale Σmν is a crucial…
Diapositive 1 New results from neutrino oscillation experiments Michel Gonin – Ecole Polytechnique – France 1987 : SUPER NOVA SN1987A Super-Kamiokande The experiments…
ORNL_talkMEDIUM-MASS NUCLEI Joanna E. Sobczyk in collaboration with S. Bacca B. Acharya G. Hagen • Neutrino-nucleus scattering in MeV-GeV region • LIT-CC
Cosmological Aspects of Neutrino Physics (II) Sergio Pastor (IFIC) 61st SUSSP St Andrews, August 2006 ν Cosmological Aspects of Neutrino Physics 2nd lecture Degenerate relic…
Multi-messenger Astronomy Neutrino 20041 2 • A vast subject and a very active field • Multi-messengers: photons (radio, IR, visible, X- and γ-rays) protons
Constraining Neutrino Mass Hierarchy and θ13 with Supernova Neutrino Data Stan Yen SNOLAB EAC August 2009 Importance of Understanding ν flavour transitions in Supernovae…
Neutrino Oscillations Gary Cheng Physics 135c 6/1/07 Introduction: Theory Neutrinos have mass eigenstates ν1, ν2, ν3 that are superpositions of the flavor eigenstates…
Solar Neutrino Results from Phase III of the Sudbury Neutrino Observatory Alan Poon Berkeley Lab Solar Neutrinos Bahcall et al Solar Neutrino Problem ~Y2K • Deficits were…
Solar Neutrino Results from Phase III of the Sudbury Neutrino Observatory Alan Poon Berkeley Lab Solar Neutrinos Bahcall et al Solar Neutrino Problem ~Y2K • Deficits were…
Slide 1Jeanne Wilson IoP HEPP 2013, Liverpool 8/4/2013 Non-Accelerator Neutrino Physics* *Excluding neutrino mass measurements Some ^ Slide 2 Content Probing neutrino properties…
1. Neutrino mass and the LHCMiha Nemevšek ICTP, Triestewith Maiezza, Melfo, Nesti, Senjanović, Tello, Vissani and Zhang Balkan Workshop 2011, Donji Milanovac 2. LHC a neutrino…
Slide 1 1 Deep Sea Neutrino Telescope Detection Principle Slide 2 2 Basic Properties of Neutrino Spin: ½ (fermion) Type: lepton Flavors: muonic, electronic, tau Masses:…