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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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Neutrino Astronomy with Korean Neutrino Observatory

Author(s)
Kwak, Kyujin
Issued Date
2018-10-10
URI
https://scholarworks.unist.ac.kr/handle/201301/80820
Fulltext
http://www.kas.org/html/sub4_01_view.html?gubun=1&idx=60
Citation
2018년 가을 제99차 한국천문학회 학술대회
Abstract
Neutrino astronomy is now possible as the technology to detect neutrinos has been advancing. Current and planned neutrino-detecting facilities can be operated as a conventional telescope because they can measure the direction toward the celestial sources as well as their physical properties like energy. Together with gravitational wave, neutrino astronomy opens a new field of astronomy, often called, multi-messenger astronomy, which also involves “traditional” electro-magnetic-wave-detection-based astronomy. Expecting that Korean Neutrino Observatory (KNO) will be one of the best neutrino observatories when it is constructed, a group of Korean astronomers and astrophysicists formed a working group and began to investigate possible astronomical neutrino sources that could be detected by KNO and other neutrino observatories. This talk presents the recent activities of the working group and introduces the list of possible neutrino sources.
Publisher
한국천문학회

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