{"created":"2023-06-19T09:12:41.692009+00:00","id":24560,"links":{},"metadata":{"_buckets":{"deposit":"c7152ab3-68ad-4249-9372-91dd6c1f9c8d"},"_deposit":{"created_by":12,"id":"24560","owners":[12],"pid":{"revision_id":0,"type":"depid","value":"24560"},"status":"published"},"_oai":{"id":"oai:kumadai.repo.nii.ac.jp:00024560","sets":["448:538","585:614:1055"]},"author_link":["155830","155831","155832","155811"],"item_15_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"226","bibliographicPageStart":"217","bibliographicVolumeNumber":"13","bibliographic_titles":[{"bibliographic_title":"Physics Reports of Kumamoto University","bibliographic_titleLang":"en"}]}]},"item_15_description_5":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"We investigate Big-Bang nucleosynthesis in the Brans-Dicke model with a variable cosmological term (BDA) for the coupling constant ω=10^4. The model parameters are constrained from comparison between the resulting abundance of ^4He, D and ^7Li and the observed ones. Furthermore, we examine the magnitude redshift (m-z) relation for the BDA with and without another constant cosmological term in a flat universe. Observational data of Type Ia Supernovae (SNIa) are used in the redshift range 0.01<z<2. It is found that BDA is inconsistent with the present accelerating universe but the model with a constant cosmological term with the value 0.7 can explain the SNIa data. The model parameters are insensitive to the m-z relation.","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_15_publisher_36":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"熊本大学","subitem_publisher_language":"ja"}]},"item_15_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0303-4070","subitem_source_identifier_type":"PISSN"}]},"item_15_source_id_9":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00774081","subitem_source_identifier_type":"NCID"}]},"item_15_subject_20":{"attribute_name":"日本十進分類法","attribute_value_mlt":[{"subitem_subject":"443.5","subitem_subject_scheme":"NDC"}]},"item_15_version_type_19":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Thushari, E.P.B.A.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155830","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Nakamura, Riou","creatorNameLang":"en"},{"creatorName":"中村, 理央","creatorNameLang":"ja"},{"creatorName":"ナカムラ, リオウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"155831","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hashimoto, Masa-aki","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155832","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Arai, Kenzo","creatorNameLang":"en"},{"creatorName":"荒井, 賢三","creatorNameLang":"ja"},{"creatorName":"アライ, ケンゾウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"155811","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":"2020-03-02"}],"displaytype":"detail","filename":"PR0013_217-226.pdf","filesize":[{"value":"2.0 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PR0013_217-226.pdf","url":"https://kumadai.repo.nii.ac.jp/record/24560/files/PR0013_217-226.pdf"},"version_id":"b8124c0f-8363-4d31-9b4d-75f30753973f"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Observational Constraints on Brans-Dicke Theory with a Variable Cosmological Term","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Observational Constraints on Brans-Dicke Theory with a Variable Cosmological Term","subitem_title_language":"en"}]},"item_type_id":"15","owner":"12","path":["538","1055"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2011-02-25"},"publish_date":"2011-02-25","publish_status":"0","recid":"24560","relation_version_is_last":true,"title":["Observational Constraints on Brans-Dicke Theory with a Variable Cosmological Term"],"weko_creator_id":"12","weko_shared_id":-1},"updated":"2023-10-17T06:40:53.267354+00:00"}