{"created":"2023-05-15T12:08:42.111039+00:00","id":13996,"links":{},"metadata":{"_buckets":{"deposit":"aebf0efe-46a7-476a-9c84-903172a93db7"},"_deposit":{"created_by":3,"id":"13996","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"13996"},"status":"published"},"_oai":{"id":"oai:iwate-u.repo.nii.ac.jp:00013996","sets":["1672:1800"]},"author_link":["58958","58959"],"item_16_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1983-03-20","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"6","bibliographicPageEnd":"F7","bibliographicPageStart":"F2","bibliographicVolumeNumber":"66","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":"通常の中性子星物質では主成分の中性子に混って陽子が数％存在することが知られている。陽子の混在度はこの物質のマクロな性質：超流動性，冷却度合，あるいはパルサーのグリッチ現象，等とからんで大切な量となる。ところで近年汎く検討されてきたπ凝縮は通常の各密度では否定的だが，中性子星内部に存在する高密度核物質では十分に可能性がある．中性子星物質でπ凝縮が起こっている場合，陽子混在度はどうなるだろうか。ここではπ^0凝縮の場合を採りあげこの問題を検討する。結論から云えば，π^0凝縮が起こっていると陽子は通常の場合に比べて，より多く（約2倍）混在できるということである。","subitem_description_type":"Other"}]},"item_16_full_name_3":{"attribute_name":"著者別名","attribute_value_mlt":[{"nameIdentifiers":[{"nameIdentifier":"58959","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/110006469606/","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":"03711838","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":[{"nameIdentifier":"58958","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":"2016-11-14"}],"displaytype":"detail","filename":"sk-v66n6pF2-F7.pdf","filesize":[{"value":"282.2 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"sk-v66n6pF2-F7.pdf","url":"https://iwate-u.repo.nii.ac.jp/record/13996/files/sk-v66n6pF2-F7.pdf"},"version_id":"06752175-bae0-4117-85d3-4ce5c14bfbac"}]},"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":"π^0凝縮下の中性子星物質に於ける陽子混在度","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"π^0凝縮下の中性子星物質に於ける陽子混在度"}]},"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":"13996","relation_version_is_last":true,"title":["π^0凝縮下の中性子星物質に於ける陽子混在度"],"weko_creator_id":"3","weko_shared_id":3},"updated":"2023-05-16T10:55:44.698028+00:00"}