{"created":"2023-07-27T06:59:06.472306+00:00","id":58374,"links":{},"metadata":{"_buckets":{"deposit":"7b26252d-3b1d-44de-8221-9377345c653a"},"_deposit":{"created_by":18,"id":"58374","owners":[18],"pid":{"revision_id":0,"type":"depid","value":"58374"},"status":"published"},"_oai":{"id":"oai:kanazawa-u.repo.nii.ac.jp:00058374","sets":["934:935:937"]},"author_link":["144","16721","86407"],"item_4_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2012-09-11","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"5","bibliographicPageStart":"053001","bibliographicVolumeNumber":"86","bibliographic_titles":[{"bibliographic_title":"Physical Review D - Particles, Fields, Gravitation and Cosmology"}]}]},"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":[{},{},{},{}]}]},"item_4_description_21":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The radiative neutrino mass model with an inert doublet scalar has been considered as a promising candidate which can explain neutrino masses, dark matter abundance and baryon number asymmetry if dark matter is identified with the lightest neutral component of the inert doublet. We reexamine these properties by imposing all the data of the neutrino oscillation, which are recently suggested by the reactor experiments. We find that the sufficient baryon number asymmetry seems not to be easily generated in a consistent way with all the data of the neutrino masses and mixing as long as the right-handed neutrinos are kept in TeV regions. Two possible modifications of the model are examined. © 2012 American Physical Society.","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":"10.24517/00064642","subitem_identifier_reg_type":"JaLC"}]},"item_4_publisher_17":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"American Physical Society"}]},"item_4_relation_12":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1103/PhysRevD.86.053001","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://prd.aps.org/"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://prd.aps.org/","subitem_relation_type_select":"URI"}}]},"item_4_rights_23":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"Copyright © American Physical Society"}]},"item_4_source_id_11":{"attribute_name":"NCID","attribute_value_mlt":[{"subitem_source_identifier":"AA00773624","subitem_source_identifier_type":"NCID"}]},"item_4_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1550-7998","subitem_source_identifier_type":"ISSN"},{"subitem_source_identifier":"1550-2368","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":"Kashiwase, Shoichi"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Suematsu, Daijiro"}],"nameIdentifiers":[{},{}]}]},"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-053001.pdf","filesize":[{"value":"454.4 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"SC-PR-SUEMATSU-D-053001.pdf","url":"https://kanazawa-u.repo.nii.ac.jp/record/58374/files/SC-PR-SUEMATSU-D-053001.pdf"},"version_id":"297a74d3-0040-425f-b64e-170e5b19543f"}]},"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":"Baryon number asymmetry and dark matter in the neutrino mass model with an inert doublet","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Baryon number asymmetry and dark matter in the neutrino mass model with an inert doublet"}]},"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":"58374","relation_version_is_last":true,"title":["Baryon number asymmetry and dark matter in the neutrino mass model with an inert doublet"],"weko_creator_id":"18","weko_shared_id":-1},"updated":"2023-07-27T14:00:40.052258+00:00"}