Conveners
Neutrino Astrophysics
- Artur Ankowski (University of Wroclaw)
Neutrino Astrophysics
- Artur Ankowski (University of Wroclaw)
In the first part of this talk recent results from the joint oscillation analyses using T2K beam neutrinos and atmospheric neutrinos will be discussed, together with the oscillation parameters which are derived from this study.
In the second part of the presentation the studies on the Diffuse Supernova Neutrino Background (DSNB) at the Super-Kamiokande will be covered.
Hyper-Kamiokande is the next generation water Cherenkov neutrino detector,
which construction started in 2020 in Japan, and the experiment is expected to start data taking in 2027. Its fiducial volume, 8 times bigger than Super-Kamiokande, instrumented with new photosensors, combined with the upgraded to 1.3 MW J-PARC neutrino beam produced 295 km away and upgraded a near detector suite, will...
The network of two next-generation underwater Cherenkov neutrino telescopes: ARCA and ORCA is being successively deployed in the Mediterranean Sea by the KM3NeT Collaboration. The focus of ARCA is neutrino astronomy, while ORCA is mainly dedicated to neutrino oscillation studies. Both detectors are already operational in their intermediate states and collect valuable results, including the...
The Giant Radio Array for Neutrino Detection (GRAND) is a next-generation observatory aiming to discover the sources of ultra-high-energy cosmic rays (UHECRs) through the detection of radio signals emitted during the interaction of the UHE particles with the atmosphere. This goal would be achieved by deploying 200,000 radio antennas over 200,000 km2 distributed worldwide, gathering enough UHE...
The success of next-generation neutrino oscillation experiments, such as DUNE and Hyper-Kamiokande, relies heavily on our ability to predict neutrino-nuclei cross sections accurately. In my talk, I will demonstrate how deep learning techniques can enhance the models for neutrino and electron-nuclei scattering cross sections.
The Pacific Ocean Neutrino Experiment (P-ONE) is an initiative to construct a multi-cubic-kilometre neutrino telescope in the depths of the Northeast Pacific Ocean.
P-ONE aims to complement the existing neutrino observatories and probe high-energy astrophysical neutrinos, providing insights into the southern celestial hemisphere, including the Galactic Plane. Capitalising on the established...
Hot white dwarfs lose energy mainly in the form of neutrinos through plasmon decay from the inner part of the star. BSM physics can have visible contributions to the cooling of these compact objects. The aim of this study is to show how hot white dwarf cooling could be altered by a dark photon from the $L_\mu - L_\tau$ model and explore these effects from ultra-light to heavy intermediators....
