WEKO3
アイテム
{"_buckets": {"deposit": "197b250c-44f7-494c-85d2-c2fff2aa12f8"}, "_deposit": {"created_by": 1, "id": "79705", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "79705"}, "status": "published"}, "_oai": {"id": "oai:repo.qst.go.jp:00079705", "sets": ["2"]}, "author_link": ["862362", "862354", "862360", "862357", "862364", "862361", "862359", "862363", "862365", "862356", "862358", "862355", "862353"], "item_10003_biblio_info_7": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2020-03", "bibliographicIssueDateType": "Issued"}, "bibliographicPageStart": "011028", "bibliographicVolumeNumber": "31", "bibliographic_titles": [{"bibliographic_title": "JPS Conference Proceedings"}]}]}, "item_10003_description_5": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We have proposed a short-lived radioisotope 98Tc as the nuclear cosmochronometer to evaluate the time from the last supernova neutirno-process to the solar system formation (SSF). We have calculated the supernova neutirno-process using a SN 1987A model with neutrino-induced reaction cross sections. The calculated result is consistent with the observed upper limit of 98Tc/98Ru at the SSF.", "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.31.011028", "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/abs/10.7566/JPSCP.31.011028", "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": "Hayakawa, Takehito"}], "nameIdentifiers": [{"nameIdentifier": "862353", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kusakabe, Motohiko"}], "nameIdentifiers": [{"nameIdentifier": "862354", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kajino, Toshitaka"}], "nameIdentifiers": [{"nameIdentifier": "862355", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Myung-Ki, Cheoun"}], "nameIdentifiers": [{"nameIdentifier": "862356", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Ko, Heamin"}], "nameIdentifiers": [{"nameIdentifier": "862357", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "J. Mathews, Grant"}], "nameIdentifiers": [{"nameIdentifier": "862358", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Tolstov, Alexey"}], "nameIdentifiers": [{"nameIdentifier": "862359", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Ken’ichi, Nomoto"}], "nameIdentifiers": [{"nameIdentifier": "862360", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Chiba, Satoshi"}], "nameIdentifiers": [{"nameIdentifier": "862361", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kawano, Toshihiko"}], "nameIdentifiers": [{"nameIdentifier": "862362", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Masa-aki, Hashimoto"}], "nameIdentifiers": [{"nameIdentifier": "862363", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Ono, Masaomi"}], "nameIdentifiers": [{"nameIdentifier": "862364", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Hayakawa, Takehito", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "862365", "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": "Nuclear Cosmochronometer for Supernova Neutrino process", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Nuclear Cosmochronometer for Supernova Neutrino process"}]}, "item_type_id": "10003", "owner": "1", "path": ["2"], "permalink_uri": "https://repo.qst.go.jp/records/79705", "pubdate": {"attribute_name": "公開日", "attribute_value": "2020-03-27"}, "publish_date": "2020-03-27", "publish_status": "0", "recid": "79705", "relation": {}, "relation_version_is_last": true, "title": ["Nuclear Cosmochronometer for Supernova Neutrino process"], "weko_shared_id": -1}
Nuclear Cosmochronometer for Supernova Neutrino process
https://repo.qst.go.jp/records/79705
https://repo.qst.go.jp/records/797054095a979-3f3e-4b94-8c70-b5ee339fb676
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2020-03-27 | |||||
タイトル | ||||||
タイトル | Nuclear Cosmochronometer for Supernova Neutrino process | |||||
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_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
Hayakawa, Takehito
× Hayakawa, Takehito× Kusakabe, Motohiko× Kajino, Toshitaka× Myung-Ki, Cheoun× Ko, Heamin× J. Mathews, Grant× Tolstov, Alexey× Ken’ichi, Nomoto× Chiba, Satoshi× Kawano, Toshihiko× Masa-aki, Hashimoto× Ono, Masaomi× Hayakawa, Takehito |
|||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | We have proposed a short-lived radioisotope 98Tc as the nuclear cosmochronometer to evaluate the time from the last supernova neutirno-process to the solar system formation (SSF). We have calculated the supernova neutirno-process using a SN 1987A model with neutrino-induced reaction cross sections. The calculated result is consistent with the observed upper limit of 98Tc/98Ru at the SSF. | |||||
書誌情報 |
JPS Conference Proceedings 巻 31, p. 011028, 発行日 2020-03 |
|||||
出版者 | ||||||
出版者 | JPS | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2435-3892 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | 10.7566/JPSCP.31.011028 | |||||
関連サイト | ||||||
識別子タイプ | URI | |||||
関連識別子 | https://journals.jps.jp/doi/abs/10.7566/JPSCP.31.011028 |