Conveners
Neutrino properties
- Shao-Feng Ge (TDLI-SJTU)
Neutrino properties
- Tailin Zhu (TDLI)
Neutrino properties
- Junting Huang (Shanghai Jiao Tong University)
Neutrino properties
- Luca Visinelli (Shanghai Jiao Tong University)
Neutrino oscillation experiments have provided us with our only direct proof of physics beyond the standard model (BSM) in the form of lepton flavour violation in neutrino propagation due to neutrino masses and flavour mixing in the leptonic sector. In this talk I will first review the present status of neutrino masses and mixing in the minimal framework with three massive neutrinos. I will...
In this talk, we present a theoretical overview on our current understanding of neutrino masses and lepton flavor mixing. The typical ideas of Neutrino mass generation are summarized, and the basic properties of massive neutrinos are discussed in connection with future experimental observations.
Tokai-to-Kamioka (T2K) is a long baseline neutrino oscillation experiment in Japan. A (anti-)muon neutrino beam with energy peak ~0.6GeV is produced at Japan Proton Accelerator Research Complex (J-PARC) in Tokai, propagates through 295km and is observed in the far detector Super-Kamiokande (SK). T2K can perform precise measurements in the muon neutrino disappearance channel, i.e. 𝜃!" and |Δ𝑚"!...
Solar neutrinos interacting with nuclei in dark matter detectors through coherent elastic neutrino-nucleus scattering (CEvNS), often referred to as the 'neutrino fog,' presents a significant challenge to direct DM detection efforts. The XENONnT detector, known for its large exposure and low background, offers an exceptional opportunity to investigate this interaction. Utilizing data from...
The cosmic neutrinos detected by the IceCube Collaboration present a compelling opportunity to explore potential new physics beyond the Standard Model and conventional relativity. In this presentation, I will discuss how the association of IceCube neutrinos with gamma-ray bursts can serve as a valuable framework for investigating Lorentz Invariance Violation (LIV) in neutrinos. Furthermore, I...
The Coherent Elastic Neutrino-Nucleus Scattering (CEvNS) was predicted in 1974. Still, it wasn't experimentally confirmed until 2017 due to its shallow energy deposit, making detection challenging due to energy threshold and background levels. Liquid Xenon Time Projection Chambers (LXeTPCs) have shown excellence in dark matter searches and may be an ideal technology for detecting CEvNS. The...
Coherent elastic neutrino-nucleus scattering (CEvNS) is the primary and enhanced interaction process for low-energy neutrinos with matter. To precisely study neutrino physics via this process, we are constructing an array of scintillation crystal detectors with a total mass of 300 kg of CsI(Na), named CICENNS. This detector will be installed at the China Spallation Neutron Source (CSNS) and...
Neutrino oscillation experiments have provided us with our only
direct proof of physics beyond the standard model (BSM) in the form of
lepton flavour violation in neutrino propagation due to neutrino
masses and flavour mixing in the leptonic sector. In this talk I will
first review the present status of neutrino masses and mixing
in the minimal framework with three massive neutrinos.
I...
