{"created":"2024-10-31T02:33:18.442132+00:00","id":2020413,"links":{},"metadata":{"_buckets":{"deposit":"ada6d68f-3428-416b-9169-52a26c387c88"},"_deposit":{"created_by":7,"id":"2020413","owners":[7],"pid":{"revision_id":0,"type":"depid","value":"2020413"},"status":"published"},"_oai":{"id":"oai:ocu-omu.repo.nii.ac.jp:02020413","sets":["1623632832836:1721355153493"]},"author_link":[],"item_1617186331708":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Gravastar formation: What can be the evidence of a black hole?","subitem_title_language":"en"}]},"item_1617186419668":{"attribute_name":"作成者","attribute_type":"creator","attribute_value_mlt":[{"creatorAffiliations":[{"affiliationNames":[{"affiliationName":"Osaka City University","affiliationNameLang":"en"}]}],"creatorNames":[{"creatorName":"Nakao, Ken-ichi","creatorNameLang":"en"},{"creatorName":"ナカオ, ケンイチ","creatorNameLang":"ja-Kana"},{"creatorName":"中尾, 憲一","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"1000090263061","nameIdentifierScheme":"KAKEN2","nameIdentifierURI":"https://nrid.nii.ac.jp/nrid/1000090263061"},{"nameIdentifier":"0000-0002-5434-3880","nameIdentifierScheme":"ORCID","nameIdentifierURI":"https://orcid.org/0000-0002-5434-3880"}]},{"creatorAffiliations":[{"affiliationNames":[{"affiliationName":"Nagoya University","affiliationNameLang":"en"}]}],"creatorNames":[{"creatorName":"Yoo, Chul-moon","creatorNameLang":"en"},{"creatorName":"リュウ, チョルムン","creatorNameLang":"ja-Kana"},{"creatorName":"柳, 哲文","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"1000060467404","nameIdentifierScheme":"KAKEN2","nameIdentifierURI":"https://nrid.nii.ac.jp/nrid/1000060467404"},{"nameIdentifier":"7000006347","nameIdentifierScheme":"RESEARCHMAP","nameIdentifierURI":"https://researchmap.jp/7000006347"}]},{"creatorAffiliations":[{"affiliationNames":[{"affiliationName":"Rikkyo University","affiliationNameLang":"en"}]}],"creatorNames":[{"creatorName":"Harada, Tomohiro","creatorNameLang":"en"},{"creatorName":"ハラダ, トモヒロ","creatorNameLang":"ja-Kana"},{"creatorName":"原田, 知広","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"1000060402773","nameIdentifierScheme":"KAKEN2","nameIdentifierURI":"https://nrid.nii.ac.jp/nrid/1000060402773"},{"nameIdentifier":"0000-0002-9085-9905","nameIdentifierScheme":"ORCID","nameIdentifierURI":"https://orcid.org/0000-0002-9085-9905"}]}]},"item_1617186499011":{"attribute_name":"権利情報","attribute_value_mlt":[{"subitem_rights":"© 2019 American Physical Society. This article may be downloaded for personal use only. Any other use requires prior permission of the author and American Physical Society. The following article appeared in Physical Review D and may be found at https://doi.org/10.1103/PhysRevD.99.044027","subitem_rights_language":"en"}]},"item_1617186609386":{"attribute_name":"主題","attribute_value_mlt":[{"subitem_subject":"ブラック・ホール","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"black hole","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"item_1617186626617":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"Any observer outside black holes cannot detect any physical signal produced by the black holes themselves, since, by definition, the black holes are not located in the causal past of the outside observer. In fact, what we regard as black hole candidates in our view are not black holes but will be gravitationally contracting objects. As well known, a black hole will form by a gravitationally collapsing object in the infinite future in the views of distant observers like us. At the very late stage of the gravitational collapse, the gravitationally contracting object behaves as a blackbody due to its gravity....","subitem_description_language":"en","subitem_description_type":"Abstract"},{"subitem_description":"This work was supported by JSPS KAKENHI Grant No. JP16K17688 (C. Y.).","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_1617186643794":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"American Physical Society","subitem_publisher_language":"en"}]},"item_1617186783814":{"attribute_name":"識別子","attribute_value_mlt":[{"subitem_identifier_type":"DOI","subitem_identifier_uri":"https://doi.org/10.1103/PhysRevD.99.044027"}]},"item_1617186920753":{"attribute_name":"収録物識別子","attribute_value_mlt":[{"subitem_source_identifier":"2470-0029","subitem_source_identifier_type":"ISSN"}]},"item_1617187056579":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2019-02-15","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"4","bibliographicPageStart":"044027","bibliographicVolumeNumber":"99","bibliographic_titles":[{"bibliographic_title":"Physical Review D","bibliographic_titleLang":"en"}]}]},"item_1617258105262":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_1617265215918":{"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_1722232185104":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2019-05-27"}],"displaytype":"detail","filename":"24700029-99-4-044027.pdf","filesize":[{"value":"814.9 KB"}],"format":"application/pdf","mimetype":"application/pdf","url":{"label":"本文","objectType":"fulltext","url":"https://ocu-omu.repo.nii.ac.jp/record/2020413/files/24700029-99-4-044027.pdf"},"version_id":"5e108f2a-5063-4e21-8528-61e47c537642"}]},"item_1722577087681":{"attribute_name":"記事種別等","attribute_value_mlt":[{"subitem_description":"Editors' Suggestion","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_1725590125188":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_title":"Gravastar formation: What can be the evidence of a black hole?","item_type_id":"40002","owner":"7","path":["1721355153493"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2019-05-27"},"publish_date":"2019-05-27","publish_status":"0","recid":"2020413","relation_version_is_last":true,"title":["Gravastar formation: What can be the evidence of a black hole?"],"weko_creator_id":"7","weko_shared_id":-1},"updated":"2024-10-31T02:33:28.172107+00:00"}