{"created":"2023-05-15T15:25:38.358310+00:00","id":13355,"links":{},"metadata":{"_buckets":{"deposit":"ba3c606b-6b74-4225-b809-8533fa7b0a55"},"_deposit":{"created_by":3,"id":"13355","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"13355"},"status":"published"},"_oai":{"id":"oai:sucra.repo.nii.ac.jp:00013355","sets":["94:426"]},"author_link":["21651","21650","21649","16582","28929","28930"],"item_119_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2008","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"5","bibliographicPageEnd":"055007-4","bibliographicPageStart":"055007-1","bibliographicVolumeNumber":"78","bibliographic_titles":[{"bibliographic_title":"PHYSICAL REVIEW D"}]}]},"item_119_date_31":{"attribute_name":"作成日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2008-12-03","subitem_date_issued_type":"Created"}]},"item_119_description_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_description":"http://link.aps.org/abstract/PRD/v78/e055007 | http://link.aps.org/abstract/PRD/v78/e055007","subitem_description_type":"Other"}]},"item_119_description_19":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"A scenario of the big-bang nucleosynthesis is analyzed within the minimal supersymmetric standard model, which is consistent with a stau-neutralino coannihilation scenario to explain the relic abundance of dark matter. We find that we can account for the possible discrepancy of the abundance of Li-7 between the observation and the prediction of the big-bang nucleosynthesis by taking the mass of the neutralino as 300 GeV and the mass difference between the stau and the neutralino as (100-120) MeV. We can therefore simultaneously explain the abundance of the dark matter and that of Li-7 by these values of parameters. The lifetime of staus in this scenario is predicted to be O(100-1000) sec","subitem_description_type":"Abstract"}]},"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_relation_16":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"info:doi/10.1103/PhysRevD.78.055007","subitem_relation_type_select":"DOI"}}]},"item_119_source_id_14":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"15507998","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":"Jittoh, Toshifumi"},{"subitem_text_value":"Kohri, Kazunori"},{"subitem_text_value":"Koike, Masafumi"},{"subitem_text_value":"Sato, Joe"},{"subitem_text_value":"Shimomura, Takashi"},{"subitem_text_value":"Yamanaka, Masato"}]},"item_119_text_32":{"attribute_name":"アイテムID","attribute_value_mlt":[{"subitem_text_value":"A1002801"}]},"item_119_text_4":{"attribute_name":"著者 所属","attribute_value_mlt":[{"subitem_text_value":"埼玉大学大学院理工学研究科物質科学部門"},{"subitem_text_value":"&EMPTY&"},{"subitem_text_value":"埼玉大学大学院理工学研究科物質科学部門"},{"subitem_text_value":"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":"Department of Physics, Saitama University"},{"subitem_text_value":"&EMPTY&"},{"subitem_text_value":"Department of Physics, Saitama University"},{"subitem_text_value":"Department of Physics, Saitama University"}]},"item_119_text_9":{"attribute_name":"年月次","attribute_value_mlt":[{"subitem_text_value":"2008-9"}]},"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":"実藤, 俊史"},{"creatorName":"ジットウ, トシフミ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kohri, Kazunori"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小池, 正史"},{"creatorName":"コイケ, マサフミ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"佐藤, 丈"},{"creatorName":"サトウ, ジョウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{},{}]},{"creatorNames":[{"creatorName":"Shimomura, Takashi"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yamanaka, Masato"}],"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":"A1002801.pdf","filesize":[{"value":"212.6 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"A1002801.pdf","url":"https://sucra.repo.nii.ac.jp/record/13355/files/A1002801.pdf"},"version_id":"f486173e-295b-450d-b80c-d4acbc8a546a"}]},"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":"Big-bang nucleosynthesis and the relic abundance of dark matter in a stau-neutralino coannihilation scenario","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Big-bang nucleosynthesis and the relic abundance of dark matter in a stau-neutralino coannihilation scenario"}]},"item_type_id":"119","owner":"3","path":["426"],"pubdate":{"attribute_name":"公開日","attribute_value":"2008-12-03"},"publish_date":"2008-12-03","publish_status":"0","recid":"13355","relation_version_is_last":true,"title":["Big-bang nucleosynthesis and the relic abundance of dark matter in a stau-neutralino coannihilation scenario"],"weko_creator_id":"3","weko_shared_id":3},"updated":"2023-05-15T19:15:23.776948+00:00"}