{"created":"2023-06-19T09:12:41.751155+00:00","id":24561,"links":{},"metadata":{"_buckets":{"deposit":"6a41213d-6a2d-433b-b326-92f091c8e9ee"},"_deposit":{"created_by":12,"id":"24561","owners":[12],"pid":{"revision_id":0,"type":"depid","value":"24561"},"status":"published"},"_oai":{"id":"oai:kumadai.repo.nii.ac.jp:00024561","sets":["448:538","585:614:1055"]},"author_link":["155822","155823","155824","155825","155811"],"item_15_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"234","bibliographicPageStart":"227","bibliographicVolumeNumber":"13","bibliographic_titles":[{"bibliographic_title":"Physics Reports of Kumamoto University","bibliographic_titleLang":"en"}]}]},"item_15_description_5":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"We investigate synthesis of heavy elements in a helium star of 32 M_sun.　Numerical calculations of nucleosynthesis have been performed during the stage of hydrostatic stellar evolution. A collapsar model is adopted whose jets are driven by magneto-hydrodynamical effects of differentially rotating core. Nucleosynthesis inside the jets is followed along the trajectories of tracer particles. Both results of hydrostatic and explosive nucleosyntheses are combined to be the yields after supernoca explosion. Comparing with the solar system abundances, we find appreciable overproduction for nuclei of the mass number 60<A<200.","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_15_publisher_36":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"熊本大学","subitem_publisher_language":"ja"}]},"item_15_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0303-4070","subitem_source_identifier_type":"PISSN"}]},"item_15_source_id_9":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00774081","subitem_source_identifier_type":"NCID"}]},"item_15_subject_20":{"attribute_name":"日本十進分類法","attribute_value_mlt":[{"subitem_subject":"443.5","subitem_subject_scheme":"NDC"}]},"item_15_version_type_19":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Ono, Masaomi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155822","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hashimoto, Masa-aki","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155823","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kikuchi, Yukihiro","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155824","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Fujimoto, Shin-ichiro","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155825","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Arai, Kenzo","creatorNameLang":"en"},{"creatorName":"荒井, 賢三","creatorNameLang":"ja"},{"creatorName":"アライ, ケンゾウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"155811","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2020-03-02"}],"displaytype":"detail","filename":"PR0013_227-234.pdf","filesize":[{"value":"1.9 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PR0013_227-234.pdf","url":"https://kumadai.repo.nii.ac.jp/record/24561/files/PR0013_227-234.pdf"},"version_id":"9be759b3-cad5-4cc1-b2f8-42fd4ae62187"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Synthesis of Heavy Elements in a Helium Star of 32 M_sun inside a Jet of Supernova Explosion","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Synthesis of Heavy Elements in a Helium Star of 32 M_sun inside a Jet of Supernova Explosion","subitem_title_language":"en"}]},"item_type_id":"15","owner":"12","path":["538","1055"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2011-02-25"},"publish_date":"2011-02-25","publish_status":"0","recid":"24561","relation_version_is_last":true,"title":["Synthesis of Heavy Elements in a Helium Star of 32 M_sun inside a Jet of Supernova Explosion"],"weko_creator_id":"12","weko_shared_id":-1},"updated":"2023-10-17T06:40:57.980491+00:00"}