| dc.description.abstract | Neutrino astronomy experiments like KM3NeT allow to survey the Universe leveraging
the properties of neutrinos of being electrically neutral and weakly interacting particles,
making them a suitable messenger. Observing neutrino emission in association
with electromagnetic radiation allows evaluating models for the acceleration of particles
occurring in high energy sources such as Supernovae or Active Galactic Nuclei.
This is the main goal of the ARCA project in KM3NeT. In addition, KM3NeT has
a program for lower energy neutrinos called ORCA, aimed at distinguishing between
the scenarios of “normal hierarchy” and “inverted hierarchy” for neutrino mass eigenstates.
The KM3NeT Collaboration is currently building a network of three Cherenkov telescopes
in the Mediterranean sea, in deep water off the coasts of Capopassero, Italy;
Toulon, France, and Pylos, Greece. The water overburden shields the detectors from
down-going charged particles produced by the interactions of cosmic rays in the atmosphere,
while up-going neutrinos that cross the Earth are the target of the observation.
Cosmic rays are a background to the KM3NeT signal, usually discarded by directional
information. Nevertheless, they provide a reliable reference to calibrate the detector
and work out its effective operating parameters, namely direction and energy of the
incoming particles.
Estimation of tracking capabilities is directly connected to the evaluation of the ability
of the experiment to detect astrophysical point-like sources, i.e. its discovery potential.
Being able to distinguish among the three neutrino flavours, or between neutrinos and
muons, as well as estimating the neutrino direction and energy, are the main goals
of such experiments. Trigger and reconstruction algorithms are designed to separate
the signal from background and to provide an estimation for the above mentioned
quantities, respectively... [edited by author] | it_IT |
