{"_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": ["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"], "permalink_uri": "https://ir.soken.ac.jp/records/4260", "pubdate": {"attribute_name": "公開日", "attribute_value": "2014-02-19"}, "publish_date": "2014-02-19", "publish_status": "0", "recid": "4260", "relation": {}, "relation_version_is_last": true, "title": ["Stellar Evolution toward Pre-Supernova Stage. II"], "weko_shared_id": 21}