{"created":"2023-05-15T15:25:30.448057+00:00","id":13168,"links":{},"metadata":{"_buckets":{"deposit":"66b396bc-a556-40e0-862a-7d8d3876b007"},"_deposit":{"created_by":3,"id":"13168","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"13168"},"status":"published"},"_oai":{"id":"oai:sucra.repo.nii.ac.jp:00013168","sets":["94:426"]},"author_link":["16582","21158"],"item_119_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1995","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"5","bibliographicPageEnd":"3080","bibliographicPageStart":"3076","bibliographicVolumeNumber":"52","bibliographic_titles":[{"bibliographic_title":"PHYSICAL REVIEW D"}]}]},"item_119_date_31":{"attribute_name":"作成日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2008-03-26","subitem_date_issued_type":"Created"}]},"item_119_description_19":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We study the possibility of an intermediate scale existing in supersymmetric SO(10) grand unified theories. The intermediate scale is required to be around 1012 GeV so that neutrinos can obtain masses suitable for explaining the experimental data on the deficit of solar neutrinos with the Mikheyev-Smirnov-Wolfenstein solution and the existence of hot dark matter. We show that any Pati-Salam-type intermediate symmetries are excluded by requiring reasonable conditions and only SU(2)L×SU(2)R×SU(3)C×U(1)B-L is likely to be realized as an intermediate symmetry.","subitem_description_type":"Abstract"}]},"item_119_description_21":{"attribute_name":"注記","attribute_value_mlt":[{"subitem_description":"Copyright notice(c)1995 American Physical Society. All rights reserved. \nPublisher's version: http://link.aps.org/abstract/PRD/v52/p3076","subitem_description_type":"Other"}]},"item_119_description_29":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"subitem_description":"text","subitem_description_type":"Other"}]},"item_119_description_30":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_119_publisher_11":{"attribute_name":"出版者名","attribute_value_mlt":[{"subitem_publisher":"American Physical Society"}]},"item_119_source_id_14":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"05562821","subitem_source_identifier_type":"ISSN"}]},"item_119_text_27":{"attribute_name":"版","attribute_value_mlt":[{"subitem_text_value":"[出版社版]"}]},"item_119_text_3":{"attribute_name":"著者 ローマ字","attribute_value_mlt":[{"subitem_text_value":"Bando, Masako"},{"subitem_text_value":"Sato, Joe"},{"subitem_text_value":"Takahashi, Tomohiko"}]},"item_119_text_32":{"attribute_name":"アイテムID","attribute_value_mlt":[{"subitem_text_value":"A1002499"}]},"item_119_text_4":{"attribute_name":"著者 所属","attribute_value_mlt":[{"subitem_text_value":"愛知大学"},{"subitem_text_value":"京都大学理学部物理学科(現 : 埼玉大学大学院理工学研究科物質科学部門)"}]},"item_119_text_5":{"attribute_name":"著者 所属(別言語)","attribute_value_mlt":[{"subitem_text_value":"Physics Division, Aichi University"},{"subitem_text_value":"Department of Physics, Kyoto University(Present : Graduate School of Science and Engineering, Saitama University)"},{"subitem_text_value":"Department of Physics, Kyoto University"}]},"item_119_text_9":{"attribute_name":"年月次","attribute_value_mlt":[{"subitem_text_value":"1995-9"}]},"item_119_version_type_28":{"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":"坂東, 昌子"},{"creatorName":"バンドウ, マサコ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"佐藤, 丈"},{"creatorName":"サトウ, ジョウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{},{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2018-01-24"}],"displaytype":"detail","filename":"A1002499.pdf","filesize":[{"value":"593.9 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"A1002499.pdf","url":"https://sucra.repo.nii.ac.jp/record/13168/files/A1002499.pdf"},"version_id":"28c1a1bc-422a-4566-bbe5-d90917f3e712"}]},"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":"POSSIBLE CANDIDATES FOR A SUPERSYMMETRIC SO(10) MODEL WITH AN INTERMEDIATE SCALE","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"POSSIBLE CANDIDATES FOR A SUPERSYMMETRIC SO(10) MODEL WITH AN INTERMEDIATE SCALE"}]},"item_type_id":"119","owner":"3","path":["426"],"pubdate":{"attribute_name":"公開日","attribute_value":"2008-03-26"},"publish_date":"2008-03-26","publish_status":"0","recid":"13168","relation_version_is_last":true,"title":["POSSIBLE CANDIDATES FOR A SUPERSYMMETRIC SO(10) MODEL WITH AN INTERMEDIATE SCALE"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-05-16T12:39:29.412368+00:00"}