{"created":"2021-03-01T06:33:05.705285+00:00","id":25087,"links":{},"metadata":{"_buckets":{"deposit":"6279df9c-ed8b-450c-baa5-69cd0111da7d"},"_deposit":{"id":"25087","owners":[],"pid":{"revision_id":0,"type":"depid","value":"25087"},"status":"published"},"_oai":{"id":"oai:nagoya.repo.nii.ac.jp:00025087","sets":["1924:1925:1926"]},"author_link":["74816"],"item_10_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2017-11-16","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"101303(R)","bibliographicPageStart":"101303(R)","bibliographicVolumeNumber":"96","bibliographic_titles":[{"bibliographic_title":"Physical Review D"}]}]},"item_10_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The direct detections of gravitational waves (GW) from merging binary black holes (BBH) by aLIGO have brought us a new opportunity to utilize BBH for a measurement of the Hubble constant. In this paper, we point out that there exists a small number of BBH that gives significantly small sky localization volume so that a host galaxy is uniquely identified. Then a redshift of a BBH is obtained from a spectroscopic follow-up observation of the host galaxy. Using these redshift-identified BBH, we show that the Hubble constant is measured at a level of precision better than 1% with advanced detectors like aLIGO at design sensitivity. Since a GW observation is completely independent of other astrophysical means, this qualitatively new probe will help resolve a well-known value discrepancy problem on the Hubble constant from cosmological measurements and local measurements.","subitem_description_language":"en","subitem_description_type":"Abstract"}]},"item_10_identifier_60":{"attribute_name":"URI","attribute_value_mlt":[{"subitem_identifier_type":"DOI","subitem_identifier_uri":"http://doi.org/10.1103/PhysRevD.96.101303"},{"subitem_identifier_type":"HDL","subitem_identifier_uri":"http://hdl.handle.net/2237/27306"}]},"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.96.101303","subitem_relation_type_select":"DOI"}}]},"item_10_rights_12":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 2017 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_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"2470-0029","subitem_source_identifier_type":"PISSN"}]},"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":"Nishizawa, Atsushi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"74816","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":"2018-02-22"}],"displaytype":"detail","filename":"PhysRevD_96_101303.pdf","filesize":[{"value":"412.5 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PhysRevD_96_101303.pdf","objectType":"fulltext","url":"https://nagoya.repo.nii.ac.jp/record/25087/files/PhysRevD_96_101303.pdf"},"version_id":"6b570303-9edf-44c7-b7cc-5846dbd4dcbd"}]},"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":"Measurement of Hubble constant with stellar-mass binary black holes","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Measurement of Hubble constant with stellar-mass binary black holes","subitem_title_language":"en"}]},"item_type_id":"10","owner":"1","path":["1926"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2018-01-29"},"publish_date":"2018-01-29","publish_status":"0","recid":"25087","relation_version_is_last":true,"title":["Measurement of Hubble constant with stellar-mass binary black holes"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-01-16T04:50:24.573935+00:00"}