Conveners
Neutrinos
- Antonio Insolia (CT)
Neutrinos
- Antonio Insolia (CT)
Prof.
Daniele Fargion
(ROMA1)
21/06/2018, 12:20
Highest energy neutrino in ICECUBE (hundred TeV or PeVs) suggested since five years the birth of a Neutrino Astronomy.
However the possible pollution by atmospheric neutrino signals, in particular prompt charmed ones, might offuscate the ability to discover the main astrophysical UHE neutrino sources. Indeed up to now no AGN or GRB or galactic sharp signal have detected.
A possible...
Mr
Marco Grassi
(APC - IN2P3 - CNRS)
21/06/2018, 12:40
JUNO is a Liquid Scintillator Detector (LSD) currently under construction in the south of China (Jiangmen city, Guangdong province). JUNO aims to detect reactor antineutrinos at a baseline of 53 km, with the goal of determining the neutrino mass ordering and performing a sub-percent measurement of three of the neutrino oscillation parameters. Its physics programme also includes the detection...
Prof.
Justin Vandenbroucke
(University of Wisconsin)
21/06/2018, 16:00
The IceCube Neutrino Observatory has discovered and measured a diffuse astrophysical neutrino flux spanning energies from several TeV to several PeV. The origins of the neutrinos are still unknown despite intense investigation using a variety of multi-messenger approaches. Spectral, temporal, and spatial studies of the astrophysical neutrinos have disfavored individual source classes...
Vladimir Kulikovskiy
(GE)
21/06/2018, 16:30
The ANTARES deep sea neutrino telescope, anchored on the seabed of the Mediterranean Sea, has been continuously taking data for more than ten years. Thanks to its excellent angular resolution in both the muon channel induced by muon neutrinos and the cascade channel induced by interactions of neutrinos of all flavours ANTARES has very large sensitivity for neutrino source searches in the...
Giorgio Maria Riccobene
(LNS)
21/06/2018, 17:00
The multimessenger astronomy era has begun: combined measurement of
gravitational waves, gammas and high-energy cosmic rays and neutrinos
provide unprecedented tools to understand the birth and evolution of
cosmic sources. Hundred kilometres South West off Capo Passero, Sicily
the KM3NeT Collaboration is building the ARCA neutrino detector, formed
by 230 vertical units equipped with 130...
Mr
Michael Schimp
(Bergische Universität Wuppertal)
21/06/2018, 17:50
The surface detector (SD) of the Pierre Auger Observatory is
sensitive to neutrinos at energies in the 100 PeV to 100 EeV range.
This sensitivity, together with its large acceptance, makes it a complementary detector to other
neutrino telescopes, which have their peak sensitivities at lower energies.
The neutrino-induced air showers that the SD of the Pierre Auger
Observatory is sensitive...
