MG13 - Talk detail |
Participant |
Spurio, Maurizio | |||||||
Institution |
Dipartimento di Fisica and INFN- Bologna - Viale Berti Pichat 6/2 - Bologna - Italy - Italy | |||||||
Session |
SF2 |
Accepted |
|
Order |
Time |
|||
Talk |
Oral abstract |
Title |
Neutrino physics and astrophysics with the ANTARES neutrino telescope | |||||
Co-authors | ||||||||
Abstract |
The ANTARES detector is currently the largest operating neutrino telescope in the Northern Hemisphere. The detector array (operating in its full configuration since 2008) consists of 12 detector lines holding a total of 885 Optical Modules. It is located in the Mediterranean Sea, near Toulon (France) at a depth of about 2500m. Its scientific target is the detection of ultra-high energy cosmic neutrinos through measurement of Cherenkov radiation from neutrino-induced charged leptons. Here, an overview of the results of various analyses will be given, in particular for the searches of point-like sources, of an excess of high energy events over the background due to the atmospheric neutrinos and the measurement of the atmospheric neutrino oscillations using a neutrino telescope. |
|||||||
Session |
GW2 |
Accepted |
|
Order |
Time |
|||
Talk |
Oral abstract |
Title |
Neutrino physics and astrophysics with the ANTARES neutrino telescope | |||||
Co-authors | ||||||||
Abstract |
The ANTARES detector is currently the largest operating neutrino telescope in the Northern Hemisphere. The detector array (operating in its full configuration since 2008) consists of 12 detector lines holding a total of 885 Optical Modules. It is located in the Mediterranean Sea, near Toulon (France) at a depth of about 2500m. Its scientific target is the detection of ultra-high energy cosmic neutrinos through measurement of Cherenkov radiation from neutrino-induced charged leptons. Here, an overview of the results of various analyses will be given, in particular for the searches of point-like sources, of an excess of high energy events over the background due to the atmospheric neutrinos and the measurement of the atmospheric neutrino oscillations using a neutrino telescope. |
|||||||