{"created":"2021-03-01T06:34:19.438261+00:00","id":26397,"links":{},"metadata":{"_buckets":{"deposit":"13ad5492-895e-49ca-8e18-c8a6cb1a9349"},"_deposit":{"id":"26397","owners":[],"pid":{"revision_id":0,"type":"depid","value":"26397"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00026397","sets":["336:695:696"]},"author_link":["86732","86733","86734"],"item_10_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-07-15","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageStart":"024005","bibliographicVolumeNumber":"98","bibliographic_titles":[{"bibliographic_title":"Physical Review D","bibliographic_titleLang":"en"}]}]},"item_10_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We revisit the concept of turnaround radius in cosmology, in the context of modified gravity. While preliminary analyses were limited to scalar-tensor/F(R) gravity, we extend the definition and the study of this quantity to a much broader class of theories including also quantum R^2 gravity. The turnaround radius is computed in terms of the parameters of the theory, and it is shown that a deviation not larger than 10% of this quantity from its value in Einstein’s theory could constrain the model parameters and even rule out some current theories.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"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.98.024005","subitem_relation_type_select":"DOI"}}]},"item_10_rights_12":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 2018 American Physical Society","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_61":{"attribute_name":"ISSN（print）","attribute_value_mlt":[{"subitem_source_identifier":"2470-0010","subitem_source_identifier_type":"PISSN"}]},"item_10_source_id_62":{"attribute_name":"ISSN（Online）","attribute_value_mlt":[{"subitem_source_identifier":"2470-0029","subitem_source_identifier_type":"EISSN"}]},"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":"86732","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Odintsov, Sergei D.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"86733","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Faraoni, Valerio","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"86734","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":"2018-10-09"}],"displaytype":"detail","filename":"PhysRevD98_024005.pdf","filesize":[{"value":"216.1 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PhysRevD98_024005","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/26397/files/PhysRevD98_024005.pdf"},"version_id":"e059dd89-10be-4df5-b772-63c3413327cd"}]},"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":"Effects of modified gravity on the turnaround radius in cosmology","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Effects of modified gravity on the turnaround radius in cosmology","subitem_title_language":"en"}]},"item_type_id":"10","owner":"1","path":["696"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2018-10-09"},"publish_date":"2018-10-09","publish_status":"0","recid":"26397","relation_version_is_last":true,"title":["Effects of modified gravity on the turnaround radius in cosmology"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-16T04:16:58.497739+00:00"}