{"created":"2023-05-15T15:03:37.166940+00:00","id":86173,"links":{},"metadata":{"_buckets":{"deposit":"992330ca-efea-4419-b4af-95e839dca6c1"},"_deposit":{"created_by":1,"id":"86173","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"86173"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00086173","sets":["11"]},"author_link":["1047700","1047699","1047701"],"item_10004_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2022-05","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1","bibliographicVolumeNumber":"8","bibliographic_titles":[{"bibliographic_title":"フォトニクスニュース"}]}]},"item_10004_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"現在，同位相面が渦状の形状を持ち内部軌道角運動量を運ぶ「光渦」が基礎科学，工学の広い分野において重要な研究課題の 1 つになっている。本記事では、宇宙に存在するような極めて強い磁場中の電子のシンクロトロン放射によって、渦状の波動関数を持ち内部角運動量を運ぶ「光子渦」の生成について説明する。さらに、光渦と光子渦の違いについても議論する。","subitem_description_type":"Abstract"}]},"item_10004_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"(公社）応用物理学会フォトニクス分科会"}]},"item_10004_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://annex.jsap.or.jp/photonics/publication/latest","subitem_relation_type_select":"URI"}}]},"item_10004_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"2189-6496","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":"早川, 岳人"}],"nameIdentifiers":[{"nameIdentifier":"1047699","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"丸山, 智幸"}],"nameIdentifiers":[{"nameIdentifier":"1047700","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Takehito, Hayakawa","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"1047701","nameIdentifierScheme":"WEKO"}]}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"宇宙における光子渦の生成","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"宇宙における光子渦の生成"}]},"item_type_id":"10004","owner":"1","path":["11"],"pubdate":{"attribute_name":"公開日","attribute_value":"2022-05-19"},"publish_date":"2022-05-19","publish_status":"0","recid":"86173","relation_version_is_last":true,"title":["宇宙における光子渦の生成"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T17:12:22.842444+00:00"}