Study of the Correlation of Utra-High Energy Cosmic Rays with Active Galactic Nuclei
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 천병구 | - |
dc.date.accessioned | 2021-08-03T20:51:53Z | - |
dc.date.available | 2021-08-03T20:51:53Z | - |
dc.date.created | 2021-06-30 | - |
dc.date.issued | 2009-10-22 | - |
dc.identifier.uri | https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/60509 | - |
dc.description.abstract | We have studied the correlation between ultra-high energy cosmic rays (UHECRs) from the arrival directions of the UHECRs and Active Galactic Nuclei (AGN) sources to investigate the origin of the UHECRs detected at the AUGER experiment (PAO). According to the first result of the PAO, the arrival direction of the UHECRs above 6 x 10^{19} eV is correlated with the AGN lying within about 75 Mpc or other objects with a similar spatial distribution. However our hypothesis study shows there is no clear correlation of the their spatial distributions if the deflection effect is not strong in cosmological space. Our future plan is to test AGN hypothesis more precisly with experimental data set accumulated by both the PAO and the Telescope Array (TA) experiment in next few years. | - |
dc.publisher | 한국물리학회 | - |
dc.title | Study of the Correlation of Utra-High Energy Cosmic Rays with Active Galactic Nuclei | - |
dc.type | Conference | - |
dc.contributor.affiliatedAuthor | 천병구 | - |
dc.identifier.bibliographicCitation | 2009년 가을 한국물리학회 학술논문발표회 | - |
dc.relation.isPartOf | 2009년 가을 한국물리학회 학술논문발표회 | - |
dc.citation.title | 2009년 가을 한국물리학회 학술논문발표회 | - |
dc.citation.conferencePlace | 창원컨벤션센터 | - |
dc.type.rims | CONF | - |
dc.description.journalClass | 2 | - |
Items in ScholarWorks are protected by copyright, with all rights reserved, unless otherwise indicated.
222, Wangsimni-ro, Seongdong-gu, Seoul, 04763, Korea+82-2-2220-1365
COPYRIGHT © 2021 HANYANG UNIVERSITY.
Certain data included herein are derived from the © Web of Science of Clarivate Analytics. All rights reserved.
You may not copy or re-distribute this material in whole or in part without the prior written consent of Clarivate Analytics.