{"created":"2023-06-20T13:23:24.691728+00:00","id":4260,"links":{},"metadata":{"_buckets":{"deposit":"2b091044-3a96-46a2-914e-f4f28166d221"},"_deposit":{"created_by":21,"id":"4260","owners":[21],"pid":{"revision_id":0,"type":"depid","value":"4260"},"status":"published"},"_oai":{"id":"oai:ir.soken.ac.jp:00004260","sets":["1:274"]},"author_link":["2478","734","2481","738","2479","2480"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1972","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"6","bibliographicPageEnd":"1884","bibliographicPageStart":"1870","bibliographicVolumeNumber":"48","bibliographic_titles":[{"bibliographic_title":"Progress of Theoretical Physics"},{"bibliographic_title":"Progress of Theoretical Physics","bibliographic_titleLang":"en"}]}]},"item_10001_creator_3":{"attribute_name":"著者別名","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"池内, 了"}],"nameIdentifiers":[{"nameIdentifier":"738","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"1000090025461","nameIdentifierScheme":"NRID","nameIdentifierURI":" "},{"nameIdentifier":"90025461","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=90025461"}]}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"As a continuation of the preceding paper, the evolution of carbon-oxygen stars of 1.5M⊙ and 2.6M⊙ has been computed from a pre-carbon-burning stage to a pre-supernova stage for the two alternative cases, with and without neutrino loss. \n\nIn the case without neutrinos, it has been found that after the termination of central carbon-burning electrons become degenerate at the center and both neon-burning and siliconburning begin as strong flashes. Finally, both of the stars become dynamically unstable on account of the photo-disintegration of iron. \n\nIn the case with neutrinos, the inversion of temperature gradient occurs in stages after central carbon-burning. This is due to the effect of neutrino loss coupled with the effect of electron degeneracy. Finally, the 1.5M⊙ star and the 2.6M⊙ star become unstable on account of the inverse-beta process of silicon and the photo-disintegration of iron, respectively.","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Oxford University Press "}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"10.1143/PTP.48.1870"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1143/PTP.48.1870","subitem_relation_type_select":"DOI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"©  2014  The Physical Society of Japan "}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0033-068X","subitem_source_identifier_type":"ISSN"}]},"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":"IKEUCHI, Satoru"}],"nameIdentifiers":[{"nameIdentifier":"734","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"NAKAZAWA, Kiyoshi "}],"nameIdentifiers":[{"nameIdentifier":"2478","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"MURAI, Tadayuki"}],"nameIdentifiers":[{"nameIdentifier":"2479","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"HOSHI, Reiun "}],"nameIdentifiers":[{"nameIdentifier":"2480","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"HAYASHI, Chushiro "}],"nameIdentifiers":[{"nameIdentifier":"2481","nameIdentifierScheme":"WEKO"}]}]},"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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Stellar Evolution toward Pre-Supernova Stage. II","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Stellar Evolution toward Pre-Supernova Stage. II"},{"subitem_title":"Stellar Evolution toward Pre-Supernova Stage. II","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"21","path":["274"],"pubdate":{"attribute_name":"公開日","attribute_value":"2014-02-19"},"publish_date":"2014-02-19","publish_status":"0","recid":"4260","relation_version_is_last":true,"title":["Stellar Evolution toward Pre-Supernova Stage. II"],"weko_creator_id":"21","weko_shared_id":21},"updated":"2023-06-20T14:26:17.254854+00:00"}