{"created":"2023-05-15T15:02:37.549806+00:00","id":84912,"links":{},"metadata":{"_buckets":{"deposit":"b8c16757-1b2e-43d8-9916-28bd9d3013cf"},"_deposit":{"created_by":1,"id":"84912","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"84912"},"status":"published"},"_oai":{"id":"oai:repo.qst.go.jp:00084912","sets":["1"]},"author_link":["1040915","1040919","1040918","1040916","1040914","1040920","1040921","1040917"],"item_8_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2022-01","bibliographicIssueDateType":"Issued"},"bibliographicPageStart":"29","bibliographicVolumeNumber":"924","bibliographic_titles":[{"bibliographic_title":"The Astrophysical Journal"}]}]},"item_8_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We calculate Galactic Chemical Evolution (GCE) of Mo and Ru by taking into account the contribution from neutrino p-process nucleosynthesis. We estimate yields of p-nuclei such as 92;94Mo and 96;98Ru through the neutrino p-process in various supernova (SN) progenitors based upon recent models. In particular,\nthe neutrino p-process in energetic hypernovae produces a large amount of p-nuclei compared to the yield in ordinary core-collapse SNe. We find that the neutrino p-process in hypernovae is the main contributor to the elemental abundance of 92Mo at low metallicity [Fe/H] < 2. Our theoretical prediction of the elemental abundances in metal-poor stars becomes more consistent with observational data when the neutrino p-process in hypernovae is taken into account.","subitem_description_type":"Abstract"}]},"item_8_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"IOP Publishing "}]},"item_8_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"10.3847/1538-4357/ac34f8","subitem_relation_type_select":"DOI"}}]},"item_8_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://iopscience.iop.org/article/10.3847/1538-4357/ac34f8","subitem_relation_type_select":"URI"}}]},"item_8_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0004-637X","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":"Sasaki, Hirokazu"}],"nameIdentifiers":[{"nameIdentifier":"1040914","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Yamazaki, Yuta"}],"nameIdentifiers":[{"nameIdentifier":"1040915","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kajino, Toshitaka"}],"nameIdentifiers":[{"nameIdentifier":"1040916","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kusakabe, Motohiko"}],"nameIdentifiers":[{"nameIdentifier":"1040917","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hayakawa, Takehito"}],"nameIdentifiers":[{"nameIdentifier":"1040918","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Myung-Ki, Cheoun"}],"nameIdentifiers":[{"nameIdentifier":"1040919","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Ko, Heamin"}],"nameIdentifiers":[{"nameIdentifier":"1040920","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Takehito, Hayakawa","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"1040921","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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Impact of hypernova p-process nucleosynthesis on the galactic chemical evolution of Mo and Ru","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Impact of hypernova p-process nucleosynthesis on the galactic chemical evolution of Mo and Ru"}]},"item_type_id":"8","owner":"1","path":["1"],"pubdate":{"attribute_name":"公開日","attribute_value":"2021-06-03"},"publish_date":"2021-06-03","publish_status":"0","recid":"84912","relation_version_is_last":true,"title":["Impact of hypernova p-process nucleosynthesis on the galactic chemical evolution of Mo and Ru"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-05-15T17:24:18.172984+00:00"}