{"created":"2021-03-01T06:20:00.388738+00:00","id":13009,"links":{},"metadata":{"_buckets":{"deposit":"79aa3573-4d55-40f7-b831-04ad608eecff"},"_deposit":{"id":"13009","owners":[],"pid":{"revision_id":0,"type":"depid","value":"13009"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00013009","sets":["336:635:636"]},"author_link":["40887","40888"],"item_12_alternative_title_19":{"attribute_name":"その他のタイトル","attribute_value_mlt":[{"subitem_alternative_title":"Super-Kamiokandeにおける上向きミューオン事象を用いた太陽及び地球方向WIMP間接探索","subitem_alternative_title_language":"ja"}]},"item_12_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2011-03-25","bibliographicIssueDateType":"Issued"}}]},"item_12_date_granted_64":{"attribute_name":"学位授与年月日","attribute_value_mlt":[{"subitem_dategranted":"2011-03-25"}]},"item_12_degree_grantor_62":{"attribute_name":"学位授与機関","attribute_value_mlt":[{"subitem_degreegrantor":[{"subitem_degreegrantor_language":"ja","subitem_degreegrantor_name":"名古屋大学"},{"subitem_degreegrantor_language":"en","subitem_degreegrantor_name":"Nagoya University"}],"subitem_degreegrantor_identifier":[{"subitem_degreegrantor_identifier_name":"13901","subitem_degreegrantor_identifier_scheme":"kakenhi"}]}]},"item_12_degree_name_61":{"attribute_name":"学位名","attribute_value_mlt":[{"subitem_degreename":"博士(理学)","subitem_degreename_language":"ja"}]},"item_12_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We present the result of an indirect search for high energy neutrinos from WIMP annihilation in the Sun and in the Earth using upward-going muon events at Super-Kamiokande. Datasets from SKI-SKIII (3109.6 days) were used for the analysis. We looked for excesses of neutrino signal from the Sun and the Earth as compared with the expected atmospheric neutrino background in three types of upward-going muon categories: stopping, nonshowering, and showering. No significant excess was observed. The 90% C.L. upper limits of upward-going muon flux induced by WIMPs of 100 GeV/c2 which annihilate in the Sun were 2.1 ×10^3 km^−2 y^−1 and 1.3 ×10^3 km^−2 y^−1 for the soft and hard annihilation channels, respectively. Those of the Earth were 1.1 ×10^3 km^−2 y^−1 and 9.0 ×10^2 km^−2 y^−1 for the soft and hard annihilation channels, respectively. The flux limits from the Sun correspond to upper limits of 4.5 ×10^−3 pb and 2.7 ×10^−4 pb for spin-dependent WIMP-nucleon scattering cross sections in the soft and hard annihilation channels, respectively. Those from the Earth correspond to upper limits of 8.1×10^−6 pb and 7.0 ×10^−7 pb for spin-independent WIMP-nucleon scattering cross sections in the soft and hard annihilation channels, respectively.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_12_description_5":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"名古屋大学博士学位論文 学位の種類:博士(理学) (課程) 学位授与年月日:平成23年3月25日","subitem_description_language":"ja","subitem_description_type":"Other"}]},"item_12_dissertation_number_65":{"attribute_name":"学位授与番号","attribute_value_mlt":[{"subitem_dissertationnumber":"甲第9175号"}]},"item_12_identifier_60":{"attribute_name":"URI","attribute_value_mlt":[{"subitem_identifier_type":"HDL","subitem_identifier_uri":"http://hdl.handle.net/2237/14904"}]},"item_12_select_15":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_select_item":"publisher"}]},"item_12_text_63":{"attribute_name":"学位授与年度","attribute_value_mlt":[{"subitem_text_value":"2010"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"open access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_abf2"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Tanaka, Takayuki","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"40887","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"田中, 隆之","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"40888","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":"2018-02-20"}],"displaytype":"detail","filename":"k9175.pdf","filesize":[{"value":"15.0 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"k9175.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/13009/files/k9175.pdf"},"version_id":"0e5a0299-9286-4ee8-a5ce-2e22ced8817e"}]},"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":"doctoral thesis","resourceuri":"http://purl.org/coar/resource_type/c_db06"}]},"item_title":"An indirect search for WIMPs in the Sun and the Earth using upward-going muon events in Super-Kamiokande","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"An indirect search for WIMPs in the Sun and the Earth using upward-going muon events in Super-Kamiokande","subitem_title_language":"en"}]},"item_type_id":"12","owner":"1","path":["636"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2011-05-30"},"publish_date":"2011-05-30","publish_status":"0","recid":"13009","relation_version_is_last":true,"title":["An indirect search for WIMPs in the Sun and the Earth using upward-going muon events in Super-Kamiokande"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-16T03:59:53.936141+00:00"}