{"created":"2021-03-01T06:13:48.573308+00:00","id":7163,"links":{},"metadata":{"_buckets":{"deposit":"40542832-c61c-411c-b409-dc66f224d454"},"_deposit":{"id":"7163","owners":[],"pid":{"revision_id":0,"type":"depid","value":"7163"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00007163","sets":["336:695:696"]},"author_link":["19386","19387"],"control_number":"7163","item_10_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-10","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"8","bibliographicPageEnd":"086005","bibliographicPageStart":"086005","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 the general scheme for modified f(R) gravity reconstruction from any realistic Friedmann-Robertson-Walker (FRW) cosmology. We formulate several versions of modified gravity compatible with solar system tests where the following sequence of cosmological epochs occurs: (a) matter dominated phase (with or without usual matter), transition from deceleration to acceleration, accelerating epoch consistent with recent WMAP data, (b) ΛCDM cosmology without cosmological constant. As a rule, such modified gravities are expressed implicitly (in terms of special functions) with late-time asymptotics of known type (for instance, the model with negative and positive powers of curvature). In the alternative approach, it is demonstrated that even simple versions of modified gravity may lead to the unification of matter dominated and accelerated phases at the price of the introduction of compensating dark energy.","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/2237/8840"}]},"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.74.086005","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":"19386","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Odintsov, Sergei D.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"19387","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_74-086005.pdf","filesize":[{"value":"203.9 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PhysRevD_74-086005.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/7163/files/PhysRevD_74-086005.pdf"},"version_id":"9d0700fd-0fd0-4ae7-a669-cf25edbf6e3c"}]},"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":"Modified f (R) gravity consistent with realistic cosmology: From a matter dominated epoch to a dark energy universe","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Modified f (R) gravity consistent with realistic cosmology: From a matter dominated epoch 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":"7163","relation_version_is_last":true,"title":["Modified f (R) gravity consistent with realistic cosmology: From a matter dominated epoch to a dark energy universe"],"weko_creator_id":"1","weko_shared_id":3},"updated":"2023-01-16T03:52:41.367103+00:00"}