Ponente
Enrique Huesca Santiago
(Deutsches Elektronen-Synchrotron (DESY))
Descripción
The Radio Neutrino Observatory in Greenland (RNO-G) will be, upon completion, the largest cosmic neutrino telescope that uses the in-ice radio detection mechanism. RNO-G is also the first radio detector of its kind, with each station having a combination of antennas deployed at different depths, the so-called shallow and deep components. With this approach, it is expected that RNO-G will be able to uniquely identify the radio signals from Ultra-High-Energy (UHE) neutrinos in ice, separating them from a large background of man-made radio emission or similar radio emission from cosmic-ray air showers.
This presentation will provide an overview of the RNO-G experiment, from the science case to the latest results from the collaboration.
Autor primario
Enrique Huesca Santiago
(Deutsches Elektronen-Synchrotron (DESY))
