WEKO3
アイテム
{"_buckets": {"deposit": "b21642dd-1383-41c4-87aa-8e9b272720fe"}, "_deposit": {"created_by": 1, "id": "20678", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "20678"}, "status": "published"}, "_oai": {"id": "oai:jaxa.repo.nii.ac.jp:00020678", "sets": ["1793", "1891"]}, "author_link": ["197081", "197083", "197084", "197082"], "item_5_alternative_title_1": {"attribute_name": "その他のタイトル", "attribute_value_mlt": [{"subitem_alternative_title": "超新星核合成および超新星からのプレソーラーグレインのC、N、Al、SiおよびTi同位体比"}]}, "item_5_biblio_info_10": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2003-11", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "116", "bibliographicPageStart": "113", "bibliographic_titles": [{"bibliographic_title": "第36回月・惑星シンポジウム"}, {"bibliographic_title": "Proceedings of the 36th ISAS Lunar and Planetary Symposium", "bibliographic_titleLang": "en"}]}]}, "item_5_description_17": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "It is investigated how many kinds of isotopic ratios of individual presolar grains from supernovae are reproduced by supernova mixing models under appropriate mixing ratios. The abundance distribution of the supernova ejecta is evaluated from the calculation of detailed nucleosynthesis calculation during the evolution and the supernova explosion of a 4 solar mass He star. Two cases of the mixing models with artificial mixing ratios are considered; one consists of the He/N, He/C, O/Ne, and Si/S-layers and the other consists of the He/N, He/C Si/S and Ni layers. The isotopic ratios of C-12/C-13, N-14/N-15, Al-26/Al-27, Si-29/Si-28, Si-30/Si-28, and Ti-44/Ti-48 of eleven SiC X grains and four low density graphite grains are compared with those of the supernova mixing models with appropriate mixing ratios. For one SiC X grain, four kinds of the isotopic ratios are reproduced by the supernova mixing model. For twelve SiC X grains and low density graphite grains, three kinds of the isotopic ratios are reproduced by the supernova mixing model. The number of grains three kinds of the isotopic ratios of which are reproduced by the mixing model depends on the C/O ratio of the mixing model. For most of the grains, three kinds of the isotopic ratios are reproduced when the C/O ratio is 0.5 to 2. However, for only two grains, three kinds of the isotopic ratios are reproduced by the oxygen-rich mixture such as C/O less than 0.1.", "subitem_description_type": "Other"}]}, "item_5_description_32": {"attribute_name": "資料番号", "attribute_value_mlt": [{"subitem_description": "資料番号: AA0046650029", "subitem_description_type": "Other"}]}, "item_5_publisher_8": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "宇宙航空研究開発機構宇宙科学研究本部"}]}, "item_5_publisher_9": {"attribute_name": "出版者(英)", "attribute_value_mlt": [{"subitem_publisher": "Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)"}]}, "item_5_text_20": {"attribute_name": "その他キーワード", "attribute_value_mlt": [{"subitem_text_value": "天体物理学"}, {"subitem_text_value": "核物理学及び高エネルギー物理学"}]}, "item_5_text_35": {"attribute_name": "JAXAカテゴリ", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ: シンポジウム・研究会"}]}, "item_5_text_36": {"attribute_name": "JAXAカテゴリ2", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ2: IS"}]}, "item_5_text_42": {"attribute_name": "シンポジウム区分", "attribute_value_mlt": [{"subitem_text_value": "シンポジウム区分: 023"}]}, "item_5_text_43": {"attribute_name": "DSpaceコレクション番号", "attribute_value_mlt": [{"subitem_text_value": "DSpaceコレクション番号: 7"}]}, "item_5_text_6": {"attribute_name": "著者所属", "attribute_value_mlt": [{"subitem_text_value": "東京大学 大学院理学系研究科"}, {"subitem_text_value": "九州大学 理学部 物理学科"}]}, "item_5_text_7": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "University of Tokyo Graduate School of Science"}, {"subitem_text_language": "en", "subitem_text_value": "Kyushu University Department of Physics, School of Sciences"}]}, "item_access_right": {"attribute_name": "アクセス権", "attribute_value_mlt": [{"subitem_access_right": "metadata only access", "subitem_access_right_uri": "http://purl.org/coar/access_right/c_14cb"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "吉田, 敬"}], "nameIdentifiers": [{"nameIdentifier": "197081", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "橋本, 正章"}], "nameIdentifiers": [{"nameIdentifier": "197082", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Yoshida, Takashi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "197083", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Hashimoto, Masaaki", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "197084", "nameIdentifierScheme": "WEKO"}]}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "超新星", "subitem_subject_scheme": "Other"}, {"subitem_subject": "核合成", "subitem_subject_scheme": "Other"}, {"subitem_subject": "同位体比", "subitem_subject_scheme": "Other"}, {"subitem_subject": "アバンダンス", "subitem_subject_scheme": "Other"}, {"subitem_subject": "進化", "subitem_subject_scheme": "Other"}, {"subitem_subject": "超新星爆発モデル", "subitem_subject_scheme": "Other"}, {"subitem_subject": "プレソーラーグレイン", "subitem_subject_scheme": "Other"}, {"subitem_subject": "炭素", "subitem_subject_scheme": "Other"}, {"subitem_subject": "supernova", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "nucleosynthesis", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "isotope ratio", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "abundance", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "evolution", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "supernova explosion model", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "presolar grain", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "carbon", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}]}, "item_language": {"attribute_name": "言語", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "資源タイプ", "attribute_value_mlt": [{"resourcetype": "conference paper", "resourceuri": "http://purl.org/coar/resource_type/c_5794"}]}, "item_title": "Supernova nucleosynthesis and C, N, Al, Si, and Ti isotopic ratios of presolar grains from supernovae", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Supernova nucleosynthesis and C, N, Al, Si, and Ti isotopic ratios of presolar grains from supernovae", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "1", "path": ["1793", "1891"], "permalink_uri": "https://jaxa.repo.nii.ac.jp/records/20678", "pubdate": {"attribute_name": "公開日", "attribute_value": "2015-03-26"}, "publish_date": "2015-03-26", "publish_status": "0", "recid": "20678", "relation": {}, "relation_version_is_last": true, "title": ["Supernova nucleosynthesis and C, N, Al, Si, and Ti isotopic ratios of presolar grains from supernovae"], "weko_shared_id": -1}
Supernova nucleosynthesis and C, N, Al, Si, and Ti isotopic ratios of presolar grains from supernovae
https://jaxa.repo.nii.ac.jp/records/20678
https://jaxa.repo.nii.ac.jp/records/20678d0c49842-37ec-4956-8c87-c59e73a15216
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Supernova nucleosynthesis and C, N, Al, Si, and Ti isotopic ratios of presolar grains from supernovae | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 超新星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 核合成 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 同位体比 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | アバンダンス | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 進化 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 超新星爆発モデル | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | プレソーラーグレイン | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 炭素 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | supernova | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | nucleosynthesis | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | isotope ratio | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | abundance | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | evolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | supernova explosion model | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | presolar grain | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | carbon | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
その他のタイトル | ||||||
その他のタイトル | 超新星核合成および超新星からのプレソーラーグレインのC、N、Al、SiおよびTi同位体比 | |||||
著者 |
吉田, 敬
× 吉田, 敬× 橋本, 正章× Yoshida, Takashi× Hashimoto, Masaaki |
|||||
著者所属 | ||||||
東京大学 大学院理学系研究科 | ||||||
著者所属 | ||||||
九州大学 理学部 物理学科 | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
Kyushu University Department of Physics, School of Sciences | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS) | |||||
書誌情報 |
第36回月・惑星シンポジウム en : Proceedings of the 36th ISAS Lunar and Planetary Symposium p. 113-116, 発行日 2003-11 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | It is investigated how many kinds of isotopic ratios of individual presolar grains from supernovae are reproduced by supernova mixing models under appropriate mixing ratios. The abundance distribution of the supernova ejecta is evaluated from the calculation of detailed nucleosynthesis calculation during the evolution and the supernova explosion of a 4 solar mass He star. Two cases of the mixing models with artificial mixing ratios are considered; one consists of the He/N, He/C, O/Ne, and Si/S-layers and the other consists of the He/N, He/C Si/S and Ni layers. The isotopic ratios of C-12/C-13, N-14/N-15, Al-26/Al-27, Si-29/Si-28, Si-30/Si-28, and Ti-44/Ti-48 of eleven SiC X grains and four low density graphite grains are compared with those of the supernova mixing models with appropriate mixing ratios. For one SiC X grain, four kinds of the isotopic ratios are reproduced by the supernova mixing model. For twelve SiC X grains and low density graphite grains, three kinds of the isotopic ratios are reproduced by the supernova mixing model. The number of grains three kinds of the isotopic ratios of which are reproduced by the mixing model depends on the C/O ratio of the mixing model. For most of the grains, three kinds of the isotopic ratios are reproduced when the C/O ratio is 0.5 to 2. However, for only two grains, three kinds of the isotopic ratios are reproduced by the oxygen-rich mixture such as C/O less than 0.1. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0046650029 |