| dc.citation.conferencePlace |
KO |
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| dc.citation.title |
3rd CHEA Collaboration meeting |
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| dc.contributor.author |
Ryu, Dongsu |
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| dc.contributor.author |
Kim, Jihyun |
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| dc.contributor.author |
Ki, Suk |
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| dc.contributor.author |
Rey, Soo-Chang |
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| dc.contributor.author |
Kang, Hyesung |
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| dc.date.accessioned |
2024-02-01T00:39:56Z |
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| dc.date.available |
2024-02-01T00:39:56Z |
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| dc.date.created |
2019-12-27 |
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| dc.date.issued |
2019-01-16 |
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| 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 |
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| dc.identifier.uri |
https://scholarworks.unist.ac.kr/handle/201301/80234 |
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| dc.publisher |
UNIST CHEA (고에너지 천체물리 연구센터) |
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| dc.title |
Utra-High-Energy Cosmic Rays and Filaments of Galaxies |
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| dc.type |
Conference Paper |
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| dc.date.conferenceDate |
2019-01-16 |
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