{"created":"2023-05-15T12:08:42.675871+00:00","id":14009,"links":{},"metadata":{"_buckets":{"deposit":"ec422636-98ec-4d83-99a6-823d29244cef"},"_deposit":{"created_by":3,"id":"14009","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"14009"},"status":"published"},"_oai":{"id":"oai:iwate-u.repo.nii.ac.jp:00014009","sets":["1672:1800"]},"author_link":["58991","58990"],"item_16_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2005-07-20","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"4","bibliographicPageEnd":"D48","bibliographicPageStart":"D47","bibliographicVolumeNumber":"111","bibliographic_titles":[{"bibliographic_title":"素粒子論研究"}]}]},"item_16_date_6":{"attribute_name":"登録日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2010-10-25"}]},"item_16_description_12":{"attribute_name":"Abstract","attribute_value_mlt":[{"subitem_description":"ストレンジネス自由度を考慮すると高密度中性子星物質は核子に加えてハイペロンが対等な構成要素として参画する「バリオン物質」としての舞台を提供する。我々は,この数年間,バリオン間相互作用についての理論的研究の進展やハイパー核から引き出される実験的知見にも注意を払いつつ, G行列計算に基づく有効相互作用アプローチにより現実的なハイペロン混在中性子星モデルの導出にとり組んできた。ここでは,この研究の中で得られた新たな知見に焦点をあわせ,逆に「Y混在中性子星がどのような問題を提起しているか」について述べる。","subitem_description_type":"Other"}]},"item_16_full_name_3":{"attribute_name":"著者別名","attribute_value_mlt":[{"nameIdentifiers":[{"nameIdentifier":"58991","nameIdentifierScheme":"WEKO"}],"names":[{"name":"TAKATSUKA, Tatsuyuki"}]}]},"item_16_publisher_14":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"素粒子論グループ 素粒子研究編集部"}]},"item_16_relation_16":{"attribute_name":"異版である","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"http://ci.nii.ac.jp/naid/110006415755","subitem_relation_type_select":"URI"}}]},"item_16_rights_18":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"素粒子論グループ 素粒子研究編集部"},{"subitem_rights":"本文データは学協会の許諾に基づきCiNiiから複製したものである"}]},"item_16_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0371-1838","subitem_source_identifier_type":"ISSN"}]},"item_16_text_4":{"attribute_name":"著者(機関)","attribute_value_mlt":[{"subitem_text_value":"岩手大学人文社会科学部"}]},"item_16_version_type_27":{"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":"高塚, 龍之"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2016-11-14"}],"displaytype":"detail","filename":"sk-v111n4pD47-48.pdf","filesize":[{"value":"160.2 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"sk-v111n4pD47-48.pdf","url":"https://iwate-u.repo.nii.ac.jp/record/14009/files/sk-v111n4pD47-48.pdf"},"version_id":"1fa24096-14ef-44b1-be24-ec7f90e2892e"}]},"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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"ハイペロン混在中性子星が提起する問題","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"ハイペロン混在中性子星が提起する問題"}]},"item_type_id":"16","owner":"3","path":["1800"],"pubdate":{"attribute_name":"公開日","attribute_value":"2010-10-25"},"publish_date":"2010-10-25","publish_status":"0","recid":"14009","relation_version_is_last":true,"title":["ハイペロン混在中性子星が提起する問題"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-05-16T12:11:20.882702+00:00"}