WEKO3
インデックスリンク
アイテム
{"_buckets": {"deposit": "a45df00d-8d38-459a-8a61-578b18488bd3"}, "_deposit": {"created_by": 18, "id": "58387", "owners": [18], "pid": {"revision_id": 0, "type": "depid", "value": "58387"}, "status": "published"}, "_oai": {"id": "oai:kanazawa-u.repo.nii.ac.jp:00058387", "sets": ["937"]}, "author_link": ["144"], "item_4_biblio_info_8": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2017-09-20", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "1", "bibliographicPageStart": "012196", "bibliographicVolumeNumber": "888", "bibliographic_titles": [{"bibliographic_title": "Journal of Physics: Conference Series"}]}]}, "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": "The radiative neutrino mass model can relate neutrino masses to dark matter at TeV regions. In order for thermal leptogenesis to work well in this model, both nely degenerate mass of the right-handed neutrinos and a tiny neutrino Yukawa coupling are necessary for resonant out-of-equilibrium decay. We show these features could be realized through an extension of the model with a U(1) gauge symmetry. This extension can also bring about a small quartic scalar coupling between the Higgs doublet scalar and an inert doublet scalar, and the origin of the Z2 symmetry which guarantees the stability of dark matter. © Published under licence by IOP Publishing Ltd.", "subitem_description_type": "Abstract"}]}, "item_4_description_22": {"attribute_name": "内容記述", "attribute_value_mlt": [{"subitem_description": "Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.\nPublished under licence by IOP Publishing Ltd.", "subitem_description_type": "Other"}]}, "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": "10.24517/00064655", "subitem_identifier_reg_type": "JaLC"}]}, "item_4_publisher_17": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "Institute of Physics Publishing"}]}, "item_4_relation_12": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type": "isIdenticalTo", "subitem_relation_type_id": {"subitem_relation_type_id_text": "10.1088/1742-6596/888/1/012196", "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://iopscience.iop.org/1742-6596"}], "subitem_relation_type_id": {"subitem_relation_type_id_text": "http://iopscience.iop.org/1742-6596", "subitem_relation_type_select": "URI"}}]}, "item_4_rights_23": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "Copyright © Institute of Physics Publishing"}]}, "item_4_source_id_11": {"attribute_name": "NCID", "attribute_value_mlt": [{"subitem_source_identifier": "AA12839617", "subitem_source_identifier_type": "NCID"}]}, "item_4_source_id_9": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "1742-6588", "subitem_source_identifier_type": "ISSN"}, {"subitem_source_identifier": "1742-6596", "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": "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", "download_preview_message": "", "file_order": 0, "filename": "SC-PR-SUEMATSU-D-012196.pdf", "filesize": [{"value": "510.1 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_11", "mimetype": "application/pdf", "size": 510100.0, "url": {"label": "SC-PR-SUEMATSU-D-012196.pdf", "url": "https://kanazawa-u.repo.nii.ac.jp/record/58387/files/SC-PR-SUEMATSU-D-012196.pdf"}, "version_id": "a9da2140-1cba-4c79-a75b-94d966192fef"}]}, "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": "Radiative neutrino mass model with a TeV scale gauge symmetry", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Radiative neutrino mass model with a TeV scale gauge symmetry"}]}, "item_type_id": "4", "owner": "18", "path": ["937"], "permalink_uri": "https://doi.org/10.24517/00064655", "pubdate": {"attribute_name": "公開日", "attribute_value": "2022-01-07"}, "publish_date": "2022-01-07", "publish_status": "0", "recid": "58387", "relation": {}, "relation_version_is_last": true, "title": ["Radiative neutrino mass model with a TeV scale gauge symmetry"], "weko_shared_id": -1}
Radiative neutrino mass model with a TeV scale gauge symmetry
https://doi.org/10.24517/00064655
https://doi.org/10.24517/00064655d3175615-33ae-4eff-b0b5-15add7e8bd7a
名前 / ファイル | ライセンス | アクション |
---|---|---|
SC-PR-SUEMATSU-D-012196.pdf (510.1 kB)
|
Item type | 学術雑誌論文 / Journal Article(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2022-01-07 | |||||
タイトル | ||||||
タイトル | Radiative neutrino mass model with a TeV scale gauge symmetry | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
ID登録 | ||||||
ID登録 | 10.24517/00064655 | |||||
ID登録タイプ | JaLC | |||||
著者 |
Suematsu, Daijiro
× Suematsu, Daijiro |
|||||
著者別表示 |
末松, 大二郎
× 末松, 大二郎 |
|||||
提供者所属 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 金沢大学理工研究域数物科学系 | |||||
書誌情報 |
Journal of Physics: Conference Series 巻 888, 号 1, p. 012196, 発行日 2017-09-20 |
|||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1742-6588 | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1742-6596 | |||||
NCID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA12839617 | |||||
DOI | ||||||
関連タイプ | isIdenticalTo | |||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1088/1742-6596/888/1/012196 | |||||
出版者 | ||||||
出版者 | Institute of Physics Publishing | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The radiative neutrino mass model can relate neutrino masses to dark matter at TeV regions. In order for thermal leptogenesis to work well in this model, both nely degenerate mass of the right-handed neutrinos and a tiny neutrino Yukawa coupling are necessary for resonant out-of-equilibrium decay. We show these features could be realized through an extension of the model with a U(1) gauge symmetry. This extension can also bring about a small quartic scalar coupling between the Higgs doublet scalar and an inert doublet scalar, and the origin of the Z2 symmetry which guarantees the stability of dark matter. © Published under licence by IOP Publishing Ltd. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Published under licence by IOP Publishing Ltd. |
|||||
権利 | ||||||
権利情報 | Copyright © Institute of Physics Publishing | |||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
関連URI | ||||||
識別子タイプ | URI | |||||
関連識別子 | http://iopscience.iop.org/1742-6596 | |||||
関連名称 | http://iopscience.iop.org/1742-6596 |