Descripción
Chairs: Silvia Capelli (1), Ninetta Saviano (2)
The KArlsruhe TRItium Neutrino experiment (KATRIN) is searching for the signature of the neutrino mass in the endpoint region of the tritium beta-decay spectrum. KATRIN combines a high-intensity gaseous molecular tritium source with a high-resolution spectroscopy using electrostatic filter with magnetic adiabatic collimation to reach the target neutrino-mass sensitivity of 0.2 eV/$c^2$,...
Project 8 is a direct neutrino mass experiment that has developed a new technique, Cyclotron Radiation Emission Spectroscopy (CRES), to make a differential measurement of the tritium $\beta^{-}$ spectrum. Project 8 aims to use the advantages of CRES to surmount the systematic and statistical limitations of current-generation direct neutrino mass measurement methods, proceeding in a phased...
The Electron Capture in $^{163}$Ho experiment, ECHo, is a running experiment for the determination of the neutrino mass scale via the analysis of the end point region of the $^{163}$Ho electron capture spectrum. In the first phase, ECHo-1k, about 60 MMCs pixels enclosing $^{163}$Ho ions for an activity of about 1Bq per pixel have been operated for several months. The goal of this first phase...
The assessment of the absolute neutrino mass scale is still a crucial challenge in today’s particle physics and cosmology. Beta or electron capture decay spectra end-point measurements are currently the only experimental methods which can provide a model-independent measurement of the absolute neutrino mass scale.
While KATRIN is successfully pushing the mass sensitivity below 1 eV, there is...
Do neutrinos have sizable self-interactions? This fundamental question, whose answer directly affects future precise astrophysical and cosmological observations, is difficult to directly test in the laboratory. For the last years, neutrino telescopes have been identified as unique tools to explore neutrino self-interactions. The actual discovery of astrophysical neutrinos and the advent of...
Among the information provided by high energy neutrinos, a promising possibility is to analyze the effects of a Violation of Equivalence Principle (VEP) on neutrino oscillations. We analyze the IceCube data on atmospheric neutrino fluxes under the assumption of a VEP and obtain updated constraints on the parameter space with the benchmark choice that neutrinos with different masses couple with...
In the environment with dense neutrino gases such as in core-collapse supernovae (CCSNe), the neutrino self-interactions are potentially dominant, and collective flavor conversions occur near the core. In particular, the crossings in the neutrino angular distribution can induce fast flavor conversion. The coherent scatterings off heavy nuclei in the preshock region of CCSNe can create tiny...
