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  1. F300 宇宙地球環境研究所
  2. F300b 紀要
  3. 名古屋大学加速器質量分析計業績報告書
  4. 16

年輪中の放射性炭素測定による過去の超新星爆発同定の可能性(第 17回名古屋大学タンデトロン加速器質量分析計シンポジウム平成16(2004)年度報告)

https://doi.org/10.18999/sumrua.16.65
https://doi.org/10.18999/sumrua.16.65
632dd5c4-0065-4df4-8e7a-9ce79fc556db
名前 / ファイル ライセンス アクション
KJ00005461794.pdf KJ00005461794.pdf (541.2 kB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2010-06-04
タイトル
タイトル 年輪中の放射性炭素測定による過去の超新星爆発同定の可能性(第 17回名古屋大学タンデトロン加速器質量分析計シンポジウム平成16(2004)年度報告)
言語 ja
その他のタイトル
その他のタイトル Possibility of Past Supernova Detection with ^<14>C(Proceedingsof the 17^<th> Symposium on Researches Using the Tandetron AMS System at Nagoya University in 2004)
言語 en
著者 毛受, 弘彰

× 毛受, 弘彰

WEKO 81841

ja 毛受, 弘彰

Search repository
MENJO, Hiroaki

× MENJO, Hiroaki

WEKO 81842

en MENJO, Hiroaki

Search repository
桑名, 宏輔

× 桑名, 宏輔

WEKO 81843

ja 桑名, 宏輔

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KUWANA, Kohsuke

× KUWANA, Kohsuke

WEKO 81844

en KUWANA, Kohsuke

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宮原, ひろ子

× 宮原, ひろ子

WEKO 81845

ja 宮原, ひろ子

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MIYAHARA, Hiroko

× MIYAHARA, Hiroko

WEKO 81846

en MIYAHARA, Hiroko

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増田, 公明

× 増田, 公明

WEKO 81847

ja 増田, 公明

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MASUDA, Kimiaki

× MASUDA, Kimiaki

WEKO 81848

en MASUDA, Kimiaki

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村木, 綏

× 村木, 綏

WEKO 81849

ja 村木, 綏

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MURAKI, Yasushi

× MURAKI, Yasushi

WEKO 81850

en MURAKI, Yasushi

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中村, 俊夫

× 中村, 俊夫

WEKO 81851

ja 中村, 俊夫

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NAKAMURA, Toshio

× NAKAMURA, Toshio

WEKO 81852

en NAKAMURA, Toshio

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アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利
言語 ja
権利情報 名古屋大学年代測定資料研究センター
権利
言語 ja
権利情報 本文データは学協会の許諾に基づきCiNiiから複製したものである
抄録
内容記述 It was suggested by Konstantinov and Kocharov that gamma ray emission from a supernova explosion produces detectable amount of ^<14>C in atmosphere of the earth. According to the idea, Damon et al. measured the ^<14>C content in tree rings from AD 998 to AD 1025 and detected Δ^<14>C increase of about 6‰ in AD 1010, which corresponds to an appearance of SN1006 (the supernova explosion that occurred in AD 1006). If the Δ^<14>C increase is really due to the gamma-ray emission by SN1006, the result must be important for the study of cosmic ray acceleration by supernova explosions. However, it is not clear if the Δ^<14>C increase in AD 1010 is caused by SN1006, because Δ^<14>C variation caused by solar activity is not considered. To test the possibility of solar activity, we extended the duration of measurement of tree ring samples. We have measured tree rings of Yaku cedar from AD 992 to AD 1028 and determined Δ^<14>C with the precision of ±2.8‰ by the accelerator mass spectrometry (AMS). Our result agrees with Damon's within the measurement error. Comparison of the 5 years before AD 1011 with the 5 years after shows an average increase of 4.1±1.7‰, which is similar to that of Damon. However, we can see the cyclic feature in the variation, which is similar to the 11-year cycle variation by solar activity as to a cycle length and the amplitude. Therefore, most part of Δ^<14>C increase in AD 1012 is considered to be the variation caused by solar activity. We plan the measurement intended for SN1054, which is a type II supernova. Kinetic energy of type II supernovae is evaluated to be larger than that of type I supernovae (ex : SN1006). So, SN1054 would be more detectable.
言語 en
内容記述タイプ Abstract
内容記述
内容記述 第17回名古屋大学タンデトロン加速器質量分析計シンポジウム平成16(2004)年度報告 Proceedings of the 17th symposiumon Researches Using the Tandetron AMS System at Nagoya University in 2004\
日時:平成17 (2005)年1月24日(月)、25日(火) 会場:名古屋大学シンポジオン Date:January 24th and 25th, 2005 Place:Nagoya University Symposion Hall
言語 ja
内容記述タイプ Other
出版者
言語 ja
出版者 名古屋大学年代測定資料研究センター
言語
言語 jpn
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ departmental bulletin paper
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
ID登録
ID登録 10.18999/sumrua.16.65
ID登録タイプ JaLC
関連情報
関連タイプ isVersionOf
識別子タイプ URI
関連識別子 http://ci.nii.ac.jp/naid/110007150932/
書誌情報 ja : 名古屋大学加速器質量分析計業績報告書

巻 16, p. 65-72, 発行日 2005-03
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