{"created":"2023-07-27T06:26:56.411787+00:00","id":10871,"links":{},"metadata":{"_buckets":{"deposit":"c96cdd14-6cb8-484f-80d8-da5a049a68a7"},"_deposit":{"created_by":3,"id":"10871","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"10871"},"status":"published"},"_oai":{"id":"oai:kanazawa-u.repo.nii.ac.jp:00010871","sets":["934:935:937"]},"author_link":["16722","16721","16724","16723"],"item_4_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2016-07-30","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"20-21","bibliographicPageStart":"1650121","bibliographicVolumeNumber":"31","bibliographic_titles":[{"bibliographic_title":"International Journal of Modern Physics A"}]}]},"item_4_description_21":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"In this paper, we study a two-loop induced radiative neutrino model at TeV scale with global U(1) symmetry, in which we analyze dark matter and resonant leptogenesis. The model includes two kinds of dark matter candidates. We discuss what kind of dark matter can satisfy the observed relic density as well as the current direct detection bound, and be simultaneously compatible with the leptogenesis. We also discuss whether our resonant leptogenesis can be differentiated from the other scenarios at TeV scale or not. © 2016 World Scientific Publishing Company.","subitem_description_type":"Abstract"}]},"item_4_description_22":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"Embargo Period 12 months","subitem_description_type":"Other"}]},"item_4_publisher_17":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"World Scientific Publishing Co. Pte Ltd"}]},"item_4_relation_12":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1142/S0217751X16501219","subitem_relation_type_select":"DOI"}}]},"item_4_source_id_11":{"attribute_name":"NCID","attribute_value_mlt":[{"subitem_source_identifier":"AA10669072","subitem_source_identifier_type":"NCID"}]},"item_4_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0217-751X","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":[{"nameIdentifier":"16721","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Okada, Hiroshi"}],"nameIdentifiers":[{"nameIdentifier":"16722","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Orikasa, Yuta"}],"nameIdentifiers":[{"nameIdentifier":"16723","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Toma, Takashi"}],"nameIdentifiers":[{"nameIdentifier":"16724","nameIdentifierScheme":"WEKO"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2017-10-03"}],"displaytype":"detail","filename":"SC-PR-KASHIWASE-S-1650121.pdf","filesize":[{"value":"580.9 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SC-PR-KASHIWASE-S-1650121.pdf","url":"https://kanazawa-u.repo.nii.ac.jp/record/10871/files/SC-PR-KASHIWASE-S-1650121.pdf"},"version_id":"088d41ea-7d19-4046-b606-4e6e0e6b029b"}]},"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":"Two loop neutrino model with dark matter and leptogenesis","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Two loop neutrino model with dark matter and leptogenesis"}]},"item_type_id":"4","owner":"3","path":["937"],"pubdate":{"attribute_name":"公開日","attribute_value":"2017-10-03"},"publish_date":"2017-10-03","publish_status":"0","recid":"10871","relation_version_is_last":true,"title":["Two loop neutrino model with dark matter and leptogenesis"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2024-06-20T06:09:28.964224+00:00"}