{"created":"2023-07-27T06:59:05.179248+00:00","id":58344,"links":{},"metadata":{"_buckets":{"deposit":"4996e827-b990-47ee-b486-c6b04eb7d990"},"_deposit":{"created_by":18,"id":"58344","owners":[18],"pid":{"revision_id":0,"type":"depid","value":"58344"},"status":"published"},"_oai":{"id":"oai:kanazawa-u.repo.nii.ac.jp:00058344","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":"2015","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"612","bibliographicPageStart":"603","bibliographicVolumeNumber":"749","bibliographic_titles":[{"bibliographic_title":"Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics"}]}]},"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":"We propose a non-thermal scenario for the generation of baryon number asymmetry in a radiative neutrino mass model which is modified to realize inflation at the early Universe. In this scenario, inflaton plays a crucial role in both generation of neutrino masses and lepton number asymmetry. Lepton number asymmetry is firstly generated in the dark matter sector through direct decay of inflaton. It is transferred to the lepton sector via the dark matter annihilation and then converted to the baryon number asymmetry due to the sphaleron interaction. All of the neutrino masses, the baryon number asymmetry and the dark matter are intimately connected to each other through the inflaton. © 2015 The Authors.","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":"10.24517/00064612","subitem_identifier_reg_type":"JaLC"}]},"item_4_publisher_17":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Elsevier B.V."}]},"item_4_relation_12":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1016/j.physletb.2015.08.062","subitem_relation_type_select":"DOI"}}]},"item_4_relation_28":{"attribute_name":"関連URI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"https://www.journals.elsevier.com/physics-letters-b/"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://www.journals.elsevier.com/physics-letters-b/","subitem_relation_type_select":"URI"}}]},"item_4_rights_23":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"Copyright © 2015 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/)"}]},"item_4_source_id_11":{"attribute_name":"NCID","attribute_value_mlt":[{"subitem_source_identifier":"AA11537044","subitem_source_identifier_type":"NCID"}]},"item_4_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0370-2693","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_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"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":"2022-01-21"}],"displaytype":"detail","filename":"SC-PR-SUEMATSU-D-603.pdf","filesize":[{"value":"516.7 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"SC-PR-SUEMATSU-D-603.pdf","url":"https://kanazawa-u.repo.nii.ac.jp/record/58344/files/SC-PR-SUEMATSU-D-603.pdf"},"version_id":"644dfefb-8cd4-446b-8a2e-f8adc3a76a41"}]},"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":"Lepton number asymmetry via inflaton decay in a modified radiative seesaw model","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Lepton number asymmetry via inflaton decay in a modified radiative seesaw model"}]},"item_type_id":"4","owner":"18","path":["937"],"pubdate":{"attribute_name":"公開日","attribute_value":"2022-01-21"},"publish_date":"2022-01-21","publish_status":"0","recid":"58344","relation_version_is_last":true,"title":["Lepton number asymmetry via inflaton decay in a modified radiative seesaw model"],"weko_creator_id":"18","weko_shared_id":-1},"updated":"2023-07-27T13:56:24.898817+00:00"}