Advanced Double Pulse Detection Techniques in the Baikal-GVD Neutrino Telescope
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F20%3A00341584" target="_blank" >RIV/68407700:21670/20:00341584 - isvavai.cz</a>
Výsledek na webu
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DOI - Digital Object Identifier
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Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Advanced Double Pulse Detection Techniques in the Baikal-GVD Neutrino Telescope
Popis výsledku v původním jazyce
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.
Název v anglickém jazyce
Advanced Double Pulse Detection Techniques in the Baikal-GVD Neutrino Telescope
Popis výsledku anglicky
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.
Klasifikace
Druh
O - Ostatní výsledky
CEP obor
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OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
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Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2020
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů