Conveners
WG1: Neutrino oscillation physics: Reactors
- Miao He (IHEP)
WG1: Neutrino oscillation physics: LBN current and Future
- Francesca Di Lodovico (Queen Mary University of London)
WG1: Neutrino oscillation physics: LBN current and Future
- Francesca Di Lodovico (Queen Mary University of London)
WG1: Neutrino oscillation physics: ATM
- Jianming Bian (UC Irvine)
Dr
Cecile Jollet
(IPHC Strasbourg)
9/25/17, 2:00 PM
J. Pedro Ochoa
(Pontifical Catholic University of Chile)
9/25/17, 2:48 PM
Barbara Clerbaux
(Université Libre de Bruxelles (ULB))
9/25/17, 3:12 PM
J. Pedro Ochoa
(Pontifical Catholic University of Chile)
9/25/17, 3:36 PM
Dr
Linda Cremonesi
(University College London)
9/27/17, 11:30 AM
Patrick Dunne
(Imperial College London)
9/27/17, 12:00 PM
Alain Blondel
(University of Geneva)
9/28/17, 2:00 PM
Christoph Bronner
(ICRR Kamioka)
9/28/17, 2:48 PM
Mattias Blennow
(Royal Institute of Technology)
9/28/17, 3:12 PM
Stephen Parke
(Fermilab)
9/28/17, 3:36 PM
Dr
Flor de Maria Blaszczyk
(Boston University)
9/29/17, 2:00 PM
Working Group 1: Neutrino Oscillations
talk
The latest results of Super Kamiokande's atmospheric neutrino analyses are presented. The first part focuses on the three-flavor neutrino oscillation analysis with and without external constraints, optimized for sensitivity to the neutrino mass hierarchy, including data from all four run periods of the experiment. Confidence intervals for the oscillation parameters deltaM_23^2, sin^2_23,...
PHILIPP DAVID ELLER
9/29/17, 2:50 PM
Working Group 1: Neutrino Oscillations
talk
The DeepCore low energy extension of the IceCube Neutrino Observatory allows us to study atmospheric neutrino oscillations. With the ability to distinguish between track- and shower-like events, we can statistically look for the disappearance of muon neutrions and simultaneously the appearance of tau neutrinos. This talk will present IceCube's analysis of the tau neutrino appearance rate using...
Dr
Marco Circella
(INFN Bari)
9/29/17, 3:03 PM
Working Group 1: Neutrino Oscillations
talk
ORCA (Oscillations Research with Cosmics in the Abyss) is the low-energy branch of KM3NeT, the next generation underwater Cherenkov neutrino detector in the Mediterranean. Its primary goal is to resolve the long-standing unsolved question of whether the neutrino mass ordering is normal or inverted by measuring matter oscillation effects with atmospheric neutrinos. The ORCA design foresees a...
