{"created":"2023-05-15T15:23:36.933645+00:00","id":10500,"links":{},"metadata":{"_buckets":{"deposit":"e0af02ed-f3b3-455c-8e47-75ceb772f4b9"},"_deposit":{"created_by":3,"id":"10500","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"10500"},"status":"published"},"_oai":{"id":"oai:sucra.repo.nii.ac.jp:00010500","sets":["94:430"]},"author_link":["28724","16582","17787"],"item_115_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2008","bibliographicIssueDateType":"Issued"},"bibliographic_titles":[{"bibliographic_title":"arXiv"}]}]},"item_115_date_31":{"attribute_name":"作成日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2008-04-23","subitem_date_issued_type":"Created"}]},"item_115_description_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_description":"http://arxiv.org/abs/hep-ph/0505160v1 | http://arxiv.org/abs/hep-ph/0505160v1","subitem_description_type":"Other"}]},"item_115_description_19":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We study the line gamma ray signature from the Galactic Center originating from Bino-like dark matter pair annihilation, when CP is not conserved. We consider the case that the Bino is nearly degenerate with a sfermion in mass. Although an indirect detection of Bino-like dark matter is difficult in general, the signal of Bino-like dark matter pair annihialtion in this case is enormously enhanced due to the threshold singularity.","subitem_description_type":"Abstract"}]},"item_115_description_29":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"subitem_description":"text","subitem_description_type":"Other"}]},"item_115_description_30":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_115_text_3":{"attribute_name":"著者 ローマ字","attribute_value_mlt":[{"subitem_text_value":"Matsumoto, Shigeki"},{"subitem_text_value":"Sato, Joe"},{"subitem_text_value":"Sato, Yoshio"}]},"item_115_text_32":{"attribute_name":"アイテムID","attribute_value_mlt":[{"subitem_text_value":"A1002546"}]},"item_115_text_4":{"attribute_name":"著者 所属","attribute_value_mlt":[{"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"}]},"item_115_text_5":{"attribute_name":"著者 所属(別言語)","attribute_value_mlt":[{"subitem_text_value":"Theory Group, KEK"},{"subitem_text_value":"Department of Physics, Saitama University"},{"subitem_text_value":"Physik-Department, Techniche Universitat Munchen"}]},"item_115_text_9":{"attribute_name":"年月次","attribute_value_mlt":[{"subitem_text_value":"2005-8"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Matsumoto, Shigeki"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"佐藤, 丈"},{"creatorName":"サトウ, ジョウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{},{}]},{"creatorNames":[{"creatorName":"Sato, Yoshio"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2018-01-23"}],"displaytype":"detail","filename":"A1002546.pdf","filesize":[{"value":"249.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"A1002546.pdf","url":"https://sucra.repo.nii.ac.jp/record/10500/files/A1002546.pdf"},"version_id":"e79b1570-6cda-4acb-81af-14a34b46700f"}]},"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":"other","resourceuri":"http://purl.org/coar/resource_type/c_1843"}]},"item_title":"Enhancement of line gamma ray signature from Bino-like dark matter annihilation due to CP violation","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Enhancement of line gamma ray signature from Bino-like dark matter annihilation due to CP violation"}]},"item_type_id":"115","owner":"3","path":["430"],"pubdate":{"attribute_name":"公開日","attribute_value":"2008-04-23"},"publish_date":"2008-04-23","publish_status":"0","recid":"10500","relation_version_is_last":true,"title":["Enhancement of line gamma ray signature from Bino-like dark matter annihilation due to CP violation"],"weko_creator_id":"3","weko_shared_id":3},"updated":"2023-05-15T19:28:24.714686+00:00"}