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류동수

Ryu, Dongsu
Astrophysics Lab.
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dc.citation.conferencePlace KO -
dc.citation.title 3rd CHEA Collaboration meeting -
dc.contributor.author Ryu, Dongsu -
dc.contributor.author Kim, Jihyun -
dc.contributor.author Ki, Suk -
dc.contributor.author Rey, Soo-Chang -
dc.contributor.author Kang, Hyesung -
dc.date.accessioned 2024-02-01T00:39:56Z -
dc.date.available 2024-02-01T00:39:56Z -
dc.date.created 2019-12-27 -
dc.date.issued 2019-01-16 -
dc.description.abstract Ultra-high-energy cosmic rays (UHECRs) are particles of extreme energies, coming from outside of our Galaxy. The Telescope Array (TA) experiment recently identified a high concentration in the arrival directions of UHECR events, called hotspot, but the nature and origin of the hotspot is still unknown. Recently in a paper paper, we reported the presence of filaments of galaxies,
connected to the Virgo Cluster, on the sky around the hotspot. Based on it, we suggested a model for the origin of TA hotspot events; they are produced at sources in the Virgo Cluster, and escape to and propagate along filaments, before they are scattered toward us. In this talk, I present this work.
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dc.identifier.bibliographicCitation 3rd CHEA Collaboration meeting -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/80234 -
dc.publisher UNIST CHEA (고에너지 천체물리 연구센터) -
dc.title Utra-High-Energy Cosmic Rays and Filaments of Galaxies -
dc.type Conference Paper -
dc.date.conferenceDate 2019-01-16 -

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