Description
The phenomenon of neutrino oscillation is now well understood from the
solar, atmospheric, reactor and accelerator neutrino experiments. This
oscillation is characterized by a unitary PMNS matrix which is parametrized by three mixing angles and one phase known as the leptonic CP phase. Though there are already significant amount of information about the three mixing angles but the CP phase is still unknown. The long baseline experiments(LBL) have CP sensitivity coming from the appearance channel but atmospheric neutrinos known to have negligible CP sensitivity. In my presentation I will describe the synergy between the LBL experiment NOVA, T2K and the atmospheric neutrino experiment ICAL@INO for obtaining the
first hint of CP violation in the lepton sector.
| WG1: Neutrino Oscillation Physics (Yes/No) | Yes |
|---|---|
| WG2: Neutrino Scattering Physics (Yes/No) | No |
| WG3: Accelerator Physics (Yes/No) | No |
| WG4: Muon Physics (Yes/No) | No |
| Type of presentation | Poster |
Author
Mr
Monojit Ghosh
(Physical Research Laboratory)
Co-authors
Dr
Pomita Ghoshal
(LNM Institute of Information Technology)
Prof.
Srubabati Goswami
(Physical Research Laboratory)
Dr
Sushant Raut
(Physical Research Laboratory)
