WEKO3
アイテム
{"_buckets": {"deposit": "43311cc2-0a31-44f7-b2d9-b7cc0b287223"}, "_deposit": {"id": "26365", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "26365"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00026365", "sets": ["1926"]}, "author_link": ["85278"], "item_10_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2018-05-22", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "10", "bibliographicPageStart": "104037", "bibliographicVolumeNumber": "97", "bibliographic_titles": [{"bibliographic_title": "Physical Review D"}]}]}, "item_10_description_4": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "The direct detection of gravitational waves (GWs) from merging binary black holes and neutron stars marks the beginning of a new era in gravitational physics, and it brings forth new opportunities to test theories of gravity. To this end, it is crucial to search for anomalous deviations from general relativity in a model-independent way, irrespective of gravity theories, GW sources, and background spacetimes. In this paper, we propose a new universal framework for testing gravity with GWs, based on the generalized propagation of a GW in an effective field theory that describes modification of gravity at cosmological scales. Then, we perform a parameter estimation study, showing how well the future observation of GWs can constrain the model parameters in the generalized models of GW propagation.", "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.97.104037", "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": "Nishizawa, Atsushi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "85278", "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": "2018-09-12"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "PhysRevD97_104037.pdf", "filesize": [{"value": "613.3 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 613300.0, "url": {"label": "PhysRevD97_104037", "objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/26365/files/PhysRevD97_104037.pdf"}, "version_id": "2606d149-7629-4a8e-bf75-687b65a747ca"}]}, "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": "Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation", "subitem_title_language": "en"}]}, "item_type_id": "10", "owner": "1", "path": ["1926"], "permalink_uri": "http://hdl.handle.net/2237/00028568", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2018-09-12"}, "publish_date": "2018-09-12", "publish_status": "0", "recid": "26365", "relation": {}, "relation_version_is_last": true, "title": ["Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation"], "weko_shared_id": -1}
Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
http://hdl.handle.net/2237/00028568
http://hdl.handle.net/2237/0002856855bd3f8f-3a37-4f28-bd16-7d35b8af78fb
名前 / ファイル | ライセンス | アクション |
---|---|---|
PhysRevD97_104037 (613.3 kB)
|
|
Item type | 学術雑誌論文 / Journal Article(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2018-09-12 | |||||
タイトル | ||||||
タイトル | Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation | |||||
言語 | en | |||||
著者 |
Nishizawa, Atsushi
× Nishizawa, Atsushi |
|||||
アクセス権 | ||||||
アクセス権 | open access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_abf2 | |||||
権利 | ||||||
言語 | en | |||||
権利情報 | © 2018 American Physical Society | |||||
抄録 | ||||||
内容記述 | The direct detection of gravitational waves (GWs) from merging binary black holes and neutron stars marks the beginning of a new era in gravitational physics, and it brings forth new opportunities to test theories of gravity. To this end, it is crucial to search for anomalous deviations from general relativity in a model-independent way, irrespective of gravity theories, GW sources, and background spacetimes. In this paper, we propose a new universal framework for testing gravity with GWs, based on the generalized propagation of a GW in an effective field theory that describes modification of gravity at cosmological scales. Then, we perform a parameter estimation study, showing how well the future observation of GWs can constrain the model parameters in the generalized models of GW propagation. | |||||
言語 | en | |||||
内容記述タイプ | Abstract | |||||
出版者 | ||||||
言語 | en | |||||
出版者 | American Physical Society | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプresource | http://purl.org/coar/resource_type/c_6501 | |||||
タイプ | journal article | |||||
出版タイプ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
DOI | ||||||
関連タイプ | isVersionOf | |||||
識別子タイプ | DOI | |||||
関連識別子 | https://doi.org/10.1103/PhysRevD.97.104037 | |||||
ISSN(print) | ||||||
収録物識別子タイプ | PISSN | |||||
収録物識別子 | 2470-0010 | |||||
ISSN(Online) | ||||||
収録物識別子タイプ | EISSN | |||||
収録物識別子 | 2470-0029 | |||||
書誌情報 |
Physical Review D 巻 97, 号 10, p. 104037, 発行日 2018-05-22 |
|||||
著者版フラグ | ||||||
値 | publisher |