{"created":"2023-05-15T14:58:45.227565+00:00","id":79706,"links":{},"metadata":{"_buckets":{"deposit":"7ff770ae-600f-48b5-be23-9156c44520a5"},"_deposit":{"created_by":1,"id":"79706","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"79706"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00079706","sets":["2"]},"author_link":["862345","862350","862351","862346","862352","862349","862347","862348"],"item_10003_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2020-03","bibliographicIssueDateType":"Issued"},"bibliographicPageStart":" 31, 011027","bibliographicVolumeNumber":"31","bibliographic_titles":[{"bibliographic_title":"JPS Conference Proceedings"}]}]},"item_10003_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We investigate nuclear abundances produced from the neutrino neutrino-process in supernova explosions. By adopting an equi-partitioned neutrino-luminosity for each neutrino flavor, we have calculated the neutrino-\nflux propagation including both its modification by neutrino self-interaction (neutrino-SI) near the neutrino-sphere and the Mikheyev-Smirnov-Wolfenstein (MSW) effect in the outer O-Ne-Mg layer. The abundances of heavier\nisotopes 92Nb, 98Tc and 138La are largely enhanced by the neutrino-SI for the inverted mass hierarchy. The ratio of 7Li/11B is lower in the inverted hierarchy than in the normal hierarchy.","subitem_description_type":"Abstract"}]},"item_10003_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"JPS"}]},"item_10003_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"10.7566/JPSCP.31.011027","subitem_relation_type_select":"DOI"}}]},"item_10003_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://journals.jps.jp/doi/10.7566/JPSCP.31.011027","subitem_relation_type_select":"URI"}}]},"item_10003_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"2435-3892","subitem_source_identifier_type":"ISSN"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Ko, Heamin"}],"nameIdentifiers":[{"nameIdentifier":"862345","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Myung-Ki, Cheoun"}],"nameIdentifiers":[{"nameIdentifier":"862346","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kusakabe, Motohiko"}],"nameIdentifiers":[{"nameIdentifier":"862347","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hayakawa, Takehito"}],"nameIdentifiers":[{"nameIdentifier":"862348","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Sasaki, Hirokazu"}],"nameIdentifiers":[{"nameIdentifier":"862349","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kajino, Toshitaka"}],"nameIdentifiers":[{"nameIdentifier":"862350","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"J. Mathews, Grant"}],"nameIdentifiers":[{"nameIdentifier":"862351","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hayakawa, Takehito","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"862352","nameIdentifierScheme":"WEKO"}]}]},"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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"Neutrino self-interaction and MSW eects by an equi-partitioned Fermi-Dirac neutrino luminosity on the supernova neutrino-process","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Neutrino self-interaction and MSW eects by an equi-partitioned Fermi-Dirac neutrino luminosity on the supernova neutrino-process"}]},"item_type_id":"10003","owner":"1","path":["2"],"pubdate":{"attribute_name":"公開日","attribute_value":"2020-03-27"},"publish_date":"2020-03-27","publish_status":"0","recid":"79706","relation_version_is_last":true,"title":["Neutrino self-interaction and MSW eects by an equi-partitioned Fermi-Dirac neutrino luminosity on the supernova neutrino-process"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T22:05:04.303466+00:00"}