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Titlebook: Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates; Observation with the Sei Kato Book 2024 The Editor(s) (if app

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發(fā)表于 2025-3-21 19:19:17 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates
副標題Observation with the
編輯Sei Kato
視頻videohttp://file.papertrans.cn/381/380607/380607.mp4
概述Is nominated as an outstanding Ph.D. thesis by the University of Tokyo, Japan.Provides pioneering studies of the rapidly expanding sub-PeV gamma-ray astronomy.Includes multi-messenger studies suggesti
叢書名稱Springer Theses
圖書封面Titlebook: Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates; Observation with the Sei Kato Book 2024 The Editor(s) (if app
描述This book presents two candidates for astrophysical accelerators of cosmic rays with petaelectron-volt (PeV) energies in our Galaxy, the so-called PeVatrons, through the observation of sub-PeV gamma rays performed by the Tibet air shower array. The two gamma-ray sources are TASG J1844-038—a newly detected source in this presented work—and HESS J1849-000. Reconstructing their gamma-ray energy spectra up to the sub-PeV range and also analyzing the archive data published by a radio survey, the book discusses?in depth the emission mechanisms of the observed gamma rays and suggests that these two gamma-ray sources are candidates for PeVatrons. The results give insights into the population of PeVatron in the Galaxy, which is important to consider their contribution to the PeV cosmic rays observed at the Earth..
出版日期Book 2024
關(guān)鍵詞Gamma Ray Astronomy; Air Shower Array; Cosmic Ray Sources; High Energy Astrophysics; PeVatrons
版次1
doihttps://doi.org/10.1007/978-981-97-1643-2
isbn_softcover978-981-97-1645-6
isbn_ebook978-981-97-1643-2Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
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發(fā)表于 2025-3-21 23:03:56 | 只看該作者
Tibet Air Shower Array and the Muon Detector Array,ray covers a geometrical area of . and captures extensive air showers initiated by primary particles to estimate their incoming directions and energies. The MD array with a geometrical area of . installed underground counts the number of muons contained in air showers and discriminates CR- and gamma
板凳
發(fā)表于 2025-3-22 02:25:46 | 只看該作者
Data Analysis,?to . from the conventional range up?to . in previous studies. The extension improves the photon statistics by . for the sources studied in this work. From a Monte Carlo analysis, the angular and energy resolutions of the experiment for sub-PeV gamma rays are estimated to be . and ., respectively. T
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發(fā)表于 2025-3-22 07:37:19 | 只看該作者
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發(fā)表于 2025-3-22 16:36:55 | 只看該作者
978-981-97-1645-6The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
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發(fā)表于 2025-3-23 03:50:42 | 只看該作者
Vertragskosten und Technologie,Search for PeVatrons: Galactic astrophysical accelerators of PeV cosmic rays through the observation of sub-PeV gamma rays (.) is important to understand the origin of the knee of the cosmic-ray energy spectrum observed on the Earth.
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發(fā)表于 2025-3-23 07:27:33 | 只看該作者
Conclusions and Future Prospects,Search for PeVatrons: Galactic astrophysical accelerators of PeV cosmic rays through the observation of sub-PeV gamma rays (.) is important to understand the origin of the knee of the cosmic-ray energy spectrum observed on the Earth.
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