{"created":"2023-07-27T06:59:06.227479+00:00","id":58369,"links":{},"metadata":{"_buckets":{"deposit":"977bc991-3a67-4991-b960-b136a533fb50"},"_deposit":{"created_by":18,"id":"58369","owners":[18],"pid":{"revision_id":0,"type":"depid","value":"58369"},"status":"published"},"_oai":{"id":"oai:kanazawa-u.repo.nii.ac.jp:00058369","sets":["934:935:937"]},"author_link":["144"],"item_4_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2012-03","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"3","bibliographicPageStart":"1951","bibliographicVolumeNumber":"72","bibliographic_titles":[{"bibliographic_title":"European Physical Journal C"}]}]},"item_4_creator_33":{"attribute_name":"著者別表示","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"末松, 大二郎"}],"nameIdentifiers":[{"nameIdentifier":"144","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"90206384","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=90206384"},{"nameIdentifier":"90206384","nameIdentifierScheme":"金沢大学研究者情報","nameIdentifierURI":"http://ridb.kanazawa-u.ac.jp/public/detail.php?kaken=90206384"},{"nameIdentifier":"90206384","nameIdentifierScheme":"研究者番号","nameIdentifierURI":"https://nrid.nii.ac.jp/nrid/1000090206384"}]}]},"item_4_description_21":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"It is known that the radiative neutrino mass model proposed by Ma could be a consistent framework for dark matter, leptogenesis and suppressed lepton flavor violation if a neutral component of the inert doublet is identified as dark matter and the right-handed neutrinos are of O(107) GeV or more. In the same model we explore another scenario such that right-handed neutrinos are in TeV regions and their lightest one is dark matter. It is shown that this scenario requires fine mass degeneracy to generate the appropriate baryon number asymmetry as in the case of resonant leptogenesis. As long as we impose the model to induce the baryon number asymmetry on the basis of thermal leptogenesis, we find that dark matter abundance cannot be explained. If this scenario is adopted, the model has to be extended to include some new mechanism to explain it. © 2012 Springer-Verlag / Società Italiana di Fisica.","subitem_description_type":"Abstract"}]},"item_4_description_5":{"attribute_name":"提供者所属","attribute_value_mlt":[{"subitem_description":"金沢大学理工研究域数物科学系","subitem_description_type":"Other"}]},"item_4_identifier_registration":{"attribute_name":"ID登録","attribute_value_mlt":[{"subitem_identifier_reg_text":"10.24517/00064637","subitem_identifier_reg_type":"JaLC"}]},"item_4_publisher_17":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Springer New York LLC"}]},"item_4_relation_12":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1140/epjc/s10052-012-1951-z","subitem_relation_type_select":"DOI"}}]},"item_4_relation_28":{"attribute_name":"関連URI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"http://epjc.epj.org/"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://epjc.epj.org/","subitem_relation_type_select":"URI"}}]},"item_4_rights_23":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"The final publication is available at www.springerlink.com/article/10.1140/epjc/s10052-012-1951-z"},{"subitem_rights":"Copyright © 2012 Springer-Verlag / Società Italiana di Fisica."}]},"item_4_source_id_11":{"attribute_name":"NCID","attribute_value_mlt":[{"subitem_source_identifier":"AA11188397","subitem_source_identifier_type":"NCID"}]},"item_4_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1434-6044","subitem_source_identifier_type":"ISSN"}]},"item_4_version_type_25":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_ab4af688f83e57aa","subitem_version_type":"AM"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Suematsu, Daijiro"}],"nameIdentifiers":[{"nameIdentifier":"144","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"90206384","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=90206384"},{"nameIdentifier":"90206384","nameIdentifierScheme":"金沢大学研究者情報","nameIdentifierURI":"http://ridb.kanazawa-u.ac.jp/public/detail.php?kaken=90206384"},{"nameIdentifier":"90206384","nameIdentifierScheme":"研究者番号","nameIdentifierURI":"https://nrid.nii.ac.jp/nrid/1000090206384"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2022-01-07"}],"displaytype":"detail","filename":"SC-PR-SUEMATSU-D-1951.pdf","filesize":[{"value":"359.2 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"SC-PR-SUEMATSU-D-1951.pdf","url":"https://kanazawa-u.repo.nii.ac.jp/record/58369/files/SC-PR-SUEMATSU-D-1951.pdf"},"version_id":"35392d01-b1a4-4787-a3a3-8b563ae621b1"}]},"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":"Thermal leptogenesis in a TeV scale model for neutrino masses","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Thermal leptogenesis in a TeV scale model for neutrino masses"}]},"item_type_id":"4","owner":"18","path":["937"],"pubdate":{"attribute_name":"公開日","attribute_value":"2022-01-07"},"publish_date":"2022-01-07","publish_status":"0","recid":"58369","relation_version_is_last":true,"title":["Thermal leptogenesis in a TeV scale model for neutrino masses"],"weko_creator_id":"18","weko_shared_id":-1},"updated":"2024-06-20T06:09:14.472487+00:00"}