{"created":"2021-03-01T06:37:29.116527+00:00","id":29306,"links":{},"metadata":{"_buckets":{"deposit":"bbda4270-b884-4b1d-b4f3-02ccb263792b"},"_deposit":{"id":"29306","owners":[],"pid":{"revision_id":0,"type":"depid","value":"29306"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00029306","sets":["336:695:696"]},"author_link":["95948","95949","95950","95951"],"item_10_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2019-10-25","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"8","bibliographicPageStart":"084060","bibliographicVolumeNumber":"100","bibliographic_titles":[{"bibliographic_title":"Physical Review D","bibliographic_titleLang":"en"}]}]},"item_10_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We study the static and spherical symmetric configurations in the nonminimal model of the de Rham-Gabadadze-Tolley (dRGT) massive gravity with a flat reference metric. Considering the modified Tolman-Oppenheimer-Volkof equation, the Bianchi identity, and energy-momentum conservation, we find a new algebraic equation for the radial coordinate of the reference metric. We demonstrate that this equation suggests an absence of the Vainshtein mechanism in the minimal model of the dRGT massive gravity, while it has two branches of solutions where one connects with the Schwarzschild spacetime and another implies the significant deviation from the asymptotically flat spacetime in the nonminimal model. We also briefly discuss the boundary conditions for the relativistic stars in the dRGT massive gravity and a potential relation with the mass-radius relation of the stars.","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.100.084060","subitem_relation_type_select":"DOI"}}]},"item_10_rights_12":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 2019 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":"Yamazaki, Masashi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"95948","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Katsuragawa, Taishi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"95949","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Odintsov, Sergei D.","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"95950","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Nojiri, Shin’ichi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"95951","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":"2020-02-12"}],"displaytype":"detail","filename":"PhysRevD100_084060.pdf","filesize":[{"value":"219.7 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PhysRevD100_084060","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/29306/files/PhysRevD100_084060.pdf"},"version_id":"12af583d-cdba-4c75-9500-13776bfdb291"}]},"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":"Screened and unscreened solutions for relativistic star in de Rham-Gabadadze-Tolley massive gravity","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Screened and unscreened solutions for relativistic star in de Rham-Gabadadze-Tolley massive gravity","subitem_title_language":"en"}]},"item_type_id":"10","owner":"1","path":["696"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2020-02-12"},"publish_date":"2020-02-12","publish_status":"0","recid":"29306","relation_version_is_last":true,"title":["Screened and unscreened solutions for relativistic star in de Rham-Gabadadze-Tolley massive gravity"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-16T04:22:25.098344+00:00"}