{"created":"2021-03-01T06:13:48.634161+00:00","id":7164,"links":{},"metadata":{"_buckets":{"deposit":"1274cb7c-f951-42ab-9381-545ba29eb2d1"},"_deposit":{"id":"7164","owners":[],"pid":{"revision_id":0,"type":"depid","value":"7164"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00007164","sets":["336:695:696"]},"author_link":["19388","19389","19390"],"item_10_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-10","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"8","bibliographicPageEnd":"086009","bibliographicPageStart":"086009","bibliographicVolumeNumber":"74","bibliographic_titles":[{"bibliographic_title":"PHYSICAL REVIEW D","bibliographic_titleLang":"en"}]}]},"item_10_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We develop a general program of the unification of a matter-dominated era with an acceleration epoch for scalar-tensor theory or a dark fluid. The general reconstruction of the scalar-tensor theory is fulfilled. The explicit form of the scalar potential for which the theory admits a matter-dominated era, a transition to an acceleration, and an (asymptotically de Sitter) acceleration epoch consistent with Wilkinson Microwave Anisotropy Probe data is found. The interrelation of the epochs of deceleration-acceleration transition and matter dominance-dark energy transition for dark fluids with a general equation of state (EOS) is investigated. We give several examples of such models with explicit EOS (using redshift parametrization) where matter-dark energy domination transition may precede the deceleration-acceleration transition. As a by-product, the reconstruction scheme is applied to scalar-tensor theory to define the scalar potentials which may produce the dark matter effect. The obtained modification of Newton potential may explain the rotation curves of galaxies.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_10_identifier_60":{"attribute_name":"URI","attribute_value_mlt":[{"subitem_identifier_type":"HDL","subitem_identifier_uri":"http://hdl.handle.net/2237/8841"}]},"item_10_publisher_32":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"American Physical Society","subitem_publisher_language":"en"}]},"item_10_relation_11":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1103/PhysRevD.74.086009","subitem_relation_type_select":"DOI"}}]},"item_10_rights_12":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"Copyright: American Physical Society, All rights reserved.","subitem_rights_language":"en"}]},"item_10_select_15":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_select_item":"publisher"}]},"item_10_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1550-7998","subitem_source_identifier_type":"PISSN"}]},"item_10_text_14":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_text_value":"application/pdf"}]},"item_1615787544753":{"attribute_name":"出版タイプ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"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":"Nojiri, Shin'ichi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"19388","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Odintsov, Sergei D.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"19389","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Stefancic, Hrvoje","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"19390","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":"2018-02-19"}],"displaytype":"detail","filename":"PhysRevD_74-086009.pdf","filesize":[{"value":"172.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PhysRevD_74-086009.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/7164/files/PhysRevD_74-086009.pdf"},"version_id":"99a6190c-236c-4bda-b041-200c51ff53c9"}]},"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":"Transition from a matter-dominated era to a dark energy universe","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Transition from a matter-dominated era to a dark energy universe","subitem_title_language":"en"}]},"item_type_id":"10","owner":"1","path":["696"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2007-10-15"},"publish_date":"2007-10-15","publish_status":"0","recid":"7164","relation_version_is_last":true,"title":["Transition from a matter-dominated era to a dark energy universe"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-16T03:52:39.128058+00:00"}