{"created":"2023-06-20T15:54:40.665756+00:00","id":181,"links":{},"metadata":{"_buckets":{"deposit":"619c16b9-485e-47b8-96d6-83b9fbf0962c"},"_deposit":{"created_by":8,"id":"181","owners":[8],"pid":{"revision_id":0,"type":"depid","value":"181"},"status":"published"},"_oai":{"id":"oai:ryotokuji-u.repo.nii.ac.jp:00000181","sets":["6:13"]},"author_link":["260"],"control_number":"181","item_10002_alternative_title_1":{"attribute_name":"その他（別言語等）のタイトル","attribute_value_mlt":[{"subitem_alternative_title":"Quark Stars in a QCD-like Effective Theory","subitem_alternative_title_language":"en"}]},"item_10002_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2013","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"7","bibliographicPageEnd":"58","bibliographicPageStart":"41","bibliographic_titles":[{"bibliographic_title":"了德寺大学研究紀要"},{"bibliographic_title":"The Bulletin of Ryotokuji University","bibliographic_titleLang":"en"}]}]},"item_10002_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The spatial structure of quark Cooper pairs in two-flavor quark matter is investigated numerically\nwithin the framework of a modified QCD-like effective model, in which the lattice-QCD-based\ngluon propagator is used. The propagator is considered to include the nonperturbative effects\nin the quenched QCD. We consider β-equilibrated quark matter with electric charge neutrality\ncondition. We find that the coherence length ε ～ 1:1 fm at low to moderate quark chemical\npotential (0:2 < μ < 0:7 GeV). Cooper pair is considered to be bosonic at μ < 0:4 GeV, because\n»=d < 1 in the region(d: interquark distance). Therefore, in the universe, the quark-Bose-Einstein\ncondensation may exist inside some of compact stars.\nFurthermore, we investigate quark stars in our model. We find that, for example, at B^(1/4) =150MeV,\nthe maximum mass is 1:92Msun and its radius is 10:61km (Msun : solar mass, B : bag constant).","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_10002_identifier_registration":{"attribute_name":"ID登録","attribute_value_mlt":[{"subitem_identifier_reg_text":"10.18933/00000152","subitem_identifier_reg_type":"JaLC"}]},"item_10002_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"了德寺大学"}]},"item_10002_relation_12":{"attribute_name":"論文ID（NAID）","attribute_value_mlt":[{"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"40019664149","subitem_relation_type_select":"NAID"}}]},"item_10002_source_id_11":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA12217741","subitem_source_identifier_type":"NCID"}]},"item_10002_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1881-9796","subitem_source_identifier_type":"PISSN"}]},"item_10002_version_type_20":{"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":"木内, 一佳志","creatorNameLang":"ja"},{"creatorName":"キウチ, ヒヨシ","creatorNameLang":"ja-Kana"},{"creatorName":"KIUCHI, Hiyoshi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"260","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":"2016-05-24"}],"displaytype":"detail","filename":"2013_01_8.pdf","filesize":[{"value":"854.5 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"量子色力学類似有効理論に於けるクォーク星","url":"https://ryotokuji-u.repo.nii.ac.jp/record/181/files/2013_01_8.pdf"},"version_id":"763a75a5-9e8e-4ffc-9765-811d870352c7"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"量子色力学類似有効モデル","subitem_subject_scheme":"Other"},{"subitem_subject":"コンパクト星拘束条件","subitem_subject_scheme":"Other"},{"subitem_subject":"ボース・アインシュタイン凝縮","subitem_subject_scheme":"Other"},{"subitem_subject":"クォーク星","subitem_subject_scheme":"Other"},{"subitem_subject":"QCD-like model","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"compact star constraints","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Bose-Einstein condensation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"quark star","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"量子色力学類似有効理論に於けるクォーク星","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"量子色力学類似有効理論に於けるクォーク星","subitem_title_language":"ja"},{"subitem_title":"Quark Stars in a QCD-like Effective Theory","subitem_title_language":"en"}]},"item_type_id":"10002","owner":"8","path":["13"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2016-05-24"},"publish_date":"2016-05-24","publish_status":"0","recid":"181","relation_version_is_last":true,"title":["量子色力学類似有効理論に於けるクォーク星"],"weko_creator_id":"8","weko_shared_id":-1},"updated":"2023-10-06T09:07:30.094538+00:00"}