{"created":"2023-07-27T06:55:55.263639+00:00","id":52402,"links":{},"metadata":{"_buckets":{"deposit":"4fba18ff-7d3b-45d1-9f32-5575d8ee6326"},"_deposit":{"created_by":18,"id":"52402","owners":[18],"pid":{"revision_id":0,"type":"depid","value":"52402"},"status":"published"},"_oai":{"id":"oai:kanazawa-u.repo.nii.ac.jp:00052402","sets":["2812:2813:4014"]},"author_link":["93677"],"item_9_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2021-05-27","bibliographicIssueDateType":"Issued"},"bibliographicPageStart":"9p.","bibliographicVolumeNumber":"2017-04-01 – 2021-03-31","bibliographic_titles":[{"bibliographic_title":"令和2(2020)年度 科学研究費補助金 若手研究(B) 研究成果報告書"},{"bibliographic_title":"2020 Fiscal Year Final Research Report","bibliographic_titleLang":"en"}]}]},"item_9_creator_33":{"attribute_name":"著者別表示","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Ishiwata, Koji"}],"nameIdentifiers":[{"nameIdentifier":"93677","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"40754271","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=40754271"}]}]},"item_9_description_21":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"本研究では、素粒子標準理論によって説明不可能な宇宙暗黒物質存在の謎の解明のため、いまだ未知の多いヒッグス粒子とそれを含むスカラー粒子に着眼し、具体的な暗黒物質探索方法を提示することを目的とした。その結果、ヒッグス粒子と相互作用する擬南部ゴールドストンスカラー粒子が暗黒物質となる場合には、直接探索実験とは違った探索実験が必要であることを示した。また超巨大質量を持つスカラー粒子が暗黒物質となる場合、先行研究に比べて非常に広い暗黒物質質量領域において発生しうる宇宙線全てについて網羅的にシミュレーションを行った結果、ガンマ線およびニュートリノ・反ニュートリノ宇宙線の観測が最も感度が高いことを示した。","subitem_description_type":"Abstract"},{"subitem_description":"The goal of this project is to propose concrete methods to detect dark matter of the Universe by focusing on the scalar sector including Higgs boson of the Standard Model. It was found that the pseudo-Nambu-Goldstone boson dark matter that interact with Higgs is hard detect in the future direct detection experiments, which indicates a new method required. For ultra-heavy dark matter, we simulated all kinds of cosmic-ray particles from dark matter in and outside the Galaxy. Consequently we found the gamma-ray and (anti)neutrino observations are most effective for the search of ultra-heavy dark matter.","subitem_description_type":"Abstract"}]},"item_9_description_22":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"研究課題/領域番号:17K14278, 研究期間(年度):2017-04-01 – 2021-03-31","subitem_description_type":"Other"},{"subitem_description":"出典：「宇宙暗黒物質とヒッグスから探る新物理」研究成果報告書　課題番号17K14278\n（KAKEN：科学研究費助成事業データベース（国立情報学研究所）） \n（https://kaken.nii.ac.jp/ja/report/KAKENHI-PROJECT-17K14278/17K14278seika/）を加工して作成","subitem_description_type":"Other"}]},"item_9_description_5":{"attribute_name":"提供者所属","attribute_value_mlt":[{"subitem_description":"金沢大学理工学域数物科学系","subitem_description_type":"Other"}]},"item_9_identifier_registration":{"attribute_name":"ID登録","attribute_value_mlt":[{"subitem_identifier_reg_text":"10.24517/00058696","subitem_identifier_reg_type":"JaLC"}]},"item_9_relation_28":{"attribute_name":"関連URI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"https://kaken.nii.ac.jp/ja/search/?kw=40754271"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://kaken.nii.ac.jp/ja/search/?kw=40754271","subitem_relation_type_select":"URI"}},{"subitem_relation_name":[{"subitem_relation_name_text":"https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-17K14278/"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-17K14278/","subitem_relation_type_select":"URI"}},{"subitem_relation_name":[{"subitem_relation_name_text":"https://kaken.nii.ac.jp/ja/report/KAKENHI-PROJECT-17K14278/17K14278seika/"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://kaken.nii.ac.jp/ja/report/KAKENHI-PROJECT-17K14278/17K14278seika/","subitem_relation_type_select":"URI"}}]},"item_9_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":"石渡, 弘治"}],"nameIdentifiers":[{"nameIdentifier":"93677","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"40754271","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=40754271"}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2022-02-21"}],"displaytype":"detail","filename":"SC-PR-ISHIWATA-K-kaken 2021-9p.pdf","filesize":[{"value":"503.7 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"SC-PR-ISHIWATA-K-kaken 2021-9p.pdf","url":"https://kanazawa-u.repo.nii.ac.jp/record/52402/files/SC-PR-ISHIWATA-K-kaken 2021-9p.pdf"},"version_id":"96791413-b15b-480e-a79c-94731ba6764b"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"research report","resourceuri":"http://purl.org/coar/resource_type/c_18ws"}]},"item_title":"宇宙暗黒物質とヒッグスから探る新物理","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"宇宙暗黒物質とヒッグスから探る新物理"},{"subitem_title":"New physics from dark matter and Higgs","subitem_title_language":"en"}]},"item_type_id":"9","owner":"18","path":["4014"],"pubdate":{"attribute_name":"公開日","attribute_value":"2022-02-21"},"publish_date":"2022-02-21","publish_status":"0","recid":"52402","relation_version_is_last":true,"title":["宇宙暗黒物質とヒッグスから探る新物理"],"weko_creator_id":"18","weko_shared_id":-1},"updated":"2024-07-01T05:19:28.249458+00:00"}