{"created":"2023-07-27T05:30:37.698476+00:00","id":130838,"links":{},"metadata":{"_buckets":{"deposit":"eb5f715c-431b-4492-a53b-d0068c05454c"},"_deposit":{"created_by":3,"id":"130838","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"130838"},"status":"published"},"_oai":{"id":"oai:tohoku.repo.nii.ac.jp:00130838","sets":["91:141"]},"author_link":["335513"],"item_2_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2019-04-17","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"8","bibliographicPageStart":"084034","bibliographicVolumeNumber":"99","bibliographic_titles":[{"bibliographic_title":"Physical Review D"}]}]},"item_2_date_62":{"attribute_name":"登録日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2019-04-17","subitem_date_issued_type":"Created"}]},"item_2_date_63":{"attribute_name":"公開日(投稿完了日)","attribute_value_mlt":[{"subitem_date_issued_datetime":"2020-07-28","subitem_date_issued_type":"Created"}]},"item_2_date_65":{"attribute_name":"発行日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2020-07-28","subitem_date_issued_type":"Created"}]},"item_2_description_41":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"subitem_description":"学術論文(Ariticle)","subitem_description_type":"Other"}]},"item_2_publisher_34":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"American Physical Society"}]},"item_2_radio_69":{"attribute_name":"公開範囲","attribute_value_mlt":[{"subitem_radio_item":"学外"}]},"item_2_relation_11":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1103/PhysRevD.99.084034","subitem_relation_type_select":"DOI"}}]},"item_2_relation_14":{"attribute_name":"情報源","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"出版社サイト"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.084034","subitem_relation_type_select":"URI"}}]},"item_2_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"2470-0010","subitem_source_identifier_type":"ISSN"}]},"item_2_version_type_16":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Shijun, Yoshida"}],"nameIdentifiers":[{"nameIdentifier":"335513","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":"2020-07-28"}],"displaytype":"detail","filename":"YOSHIDA-Shijun-2020Tour01-47.pdf","filesize":[{"value":"676.8 kB"}],"format":"application/pdf","license_note":"© 2019 American Physical Society","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"YOSHIDA-Shijun-2020Tour01-47.pdf","url":"https://tohoku.repo.nii.ac.jp/record/130838/files/YOSHIDA-Shijun-2020Tour01-47.pdf"},"version_id":"ef3a2ca9-4012-44b4-841e-494a5073fdf0"}]},"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":"Stably stratified stars containing magnetic fields whose toroidal components are much larger than the poloidal ones in general relativity: A perturbation analysis","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Stably stratified stars containing magnetic fields whose toroidal components are much larger than the poloidal ones in general relativity: A perturbation analysis"}]},"item_type_id":"2","owner":"3","path":["141"],"pubdate":{"attribute_name":"公開日","attribute_value":"2020-07-28"},"publish_date":"2020-07-28","publish_status":"0","recid":"130838","relation_version_is_last":true,"title":["Stably stratified stars containing magnetic fields whose toroidal components are much larger than the poloidal ones in general relativity: A perturbation analysis"],"weko_creator_id":"3","weko_shared_id":3},"updated":"2023-07-27T21:37:03.661624+00:00"}