Conveners
Neutrino Physics: Solar/Atm/SN
- Hiroyuki Sekiya (University of Tokyo)
Neutrino Physics: Reactor
- Seon-Hee Seo (Seoul National University)
Neutrino Physics: VSBL reactor exp + Sterile
- Seon-Hee Seo (Seoul National University)
Neutrino Physics: Sterile
- Seon-Hee Seo (Seoul National University)
Neutrino Physics: Neutrino models + collider tests
- Andre De Gouvea (Northwestern University)
Neutrino Physics: DBD I
- Francesc Monrabal (University of Texas at Arlington)
Neutrino Physics: DBD II
- HongJoo Kim (Kyungpook National University)
Neutrino Physics: interaction, x-section
- William Detmold (Massachusetts Institute of Technology)
Neutrino Physics: interaction, x-section+astrophysics/cosmology
- Yvonne Wong (The University of New South Wales)
Neutrino Physics: LBL+R&D
- Sowjanya Gollapinni (Wayne State University (US))
Neutrino Physics: R&D + pheno@future facilities
- Werner Rodejohann
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This talk reports the first measurement using the NOvA detectors of
$\nu_{\mu}$ disappearance in a $\nu_{\mu}$ beam. Oscillation parameters
$\Delta m_{32}^{2}$ and $\sin^{2}\theta_{23}$ are measured as function
of the count and energy spectrum of $\nu_{\mu}$ interactions at a
Near and Far Detector, separated by a distance of $810\text{ km}$.
High-statistics Near Detector energy spectra are...
NOvA is a long-baseline accelerator-based neutrino oscillation experiment that is optimized for NuE measurements. It uses the upgraded NuMI beam from Fermilab and measures electron-neutrino appearance and muon-neutrino disappearance at its Far Detector in Ash River, Minnesota. The NuE appearance analysis at NOvA aims to resolve the neutrino mass hierarchy problem and to constrain the...
Merging the following abstracts:
The T2K long-baseline neutrino oscillation experiment has been running in anti-neutrino mode since 2014 and recently released anti-neutrino oscillation results. These results have been updated with further data and now include the full three-flavour anti-neutrino oscillation analysis. We will present these new results and compare them with the neutrino...