Advanced Double Pulse Detection Techniques in the Baikal-GVD Neutrino Telescope
- NázevTitle
- Advanced Double Pulse Detection Techniques in the Baikal-GVD Neutrino TelescopeAdvanced Double Pulse Detection Techniques in the Baikal-GVD Neutrino Telescope
- Druh výsledkuResult type
- Kvalifikační práceThesis
- AutořiAuthors
- E. Eckerová, L. Fajt, R. Hodák, R. Dvornický
- Časopis / citaceJournal / citation
- Defense date 2020-06-09. Master Thesis. CTU IEAP. Department of Experimental Physics; Comenius University Bratislava.
- RokYear
- 2020
- JazykLanguage
- eng
- RIVRIV
- RIV/68407700:21670/20:00341584!RIV21-MSM-21670___
- ProjektProject
- Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
AbstraktAbstract
The aim of the Master thesis is the Baikal-GVD (Gigaton Volume Detector) neutrino telescope which is located in the biggest freshwater lake in the world – Lake Baikal. The goal is to detect almost undetectable neutrinos having their origin in the Universe. The Baikal-GVD detector is a three-dimensional array of light sensitive sensors – photomultipliers that register light from secondary charged particles at the bottom of the lake. High energy tau neutrino identification is a direct proof of the astrophysical neutrinos detection. The high energy tau neutrinos cannot be created in the collisions of charged cosmic particles in our atmosphere. A large amount of double pulses created in the detector is a typical signature of the tau neutrino registration. Their possible identification is therefore determined by a development of a precise method which can identify double pulses reliably.
The aim of the Master thesis is the Baikal-GVD (Gigaton Volume Detector) neutrino telescope which is located in the biggest freshwater lake in the world – Lake Baikal. The goal is to detect almost undetectable neutrinos having their origin in the Universe. The Baikal-GVD detector is a three-dimensional array of light sensitive sensors – photomultipliers that register light from secondary charged particles at the bottom of the lake. High energy tau neutrino identification is a direct proof of the astrophysical neutrinos detection. The high energy tau neutrinos cannot be created in the collisions of charged cosmic particles in our atmosphere. A large amount of double pulses created in the detector is a typical signature of the tau neutrino registration. Their possible identification is therefore determined by a development of a precise method which can identify double pulses reliably.