WEKO3
アイテム
{"_buckets": {"deposit": "a2b69aae-47c8-4659-a8e1-663a71ab195d"}, "_deposit": {"id": "27916", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "27916"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00027916", "sets": ["1926"]}, "author_link": ["90892", "90893"], "item_10_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2018-12-15", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "12", "bibliographicPageStart": "124018", "bibliographicVolumeNumber": "98", "bibliographic_titles": [{"bibliographic_title": "Physical Review D"}]}]}, "item_10_description_4": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We consider gravitational waves (GWs) in generic parity-violating gravity, including recently proposed ghost-free theories with parity violation as well as Chern-Simons (CS) modified gravity, and study the implications of observational constraints from GW170817/GRB 170817A. Whereas GWs propagate at the speed of light, c, in CS gravity, we point out that this is specific to CS gravity and the GW propagation speed deviates from c, in general, in parity-violating gravity. Therefore, contrary to the previous literature in which only CS gravity is studied as a concrete example, we show that GW170817/GRB 170817A can, in fact, be used to limit gravitational parity violation. Our argument implies that the constraint on the propagation speed of GWs can pin down the parity-violating sector, if any, to CS gravity.", "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.98.124018", "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": "90892", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kobayashi, Tsutomu", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "90893", "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": "2019-05-08"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "PhysRevD98_124018.pdf", "filesize": [{"value": "151.5 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 151500.0, "url": {"label": "PhysRevD98_124018", "objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/27916/files/PhysRevD98_124018.pdf"}, "version_id": "1d1c86b6-f6a7-42f9-8560-fdf14c812ad5"}]}, "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": "Parity-violating gravity and GW170817", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Parity-violating gravity and GW170817", "subitem_title_language": "en"}]}, "item_type_id": "10", "owner": "1", "path": ["1926"], "permalink_uri": "http://hdl.handle.net/2237/00030115", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2019-05-08"}, "publish_date": "2019-05-08", "publish_status": "0", "recid": "27916", "relation": {}, "relation_version_is_last": true, "title": ["Parity-violating gravity and GW170817"], "weko_shared_id": -1}
Parity-violating gravity and GW170817
http://hdl.handle.net/2237/00030115
http://hdl.handle.net/2237/00030115cc76b4f4-ffc1-489f-8c39-5498c1653863
名前 / ファイル | ライセンス | アクション |
---|---|---|
![]() |
|
Item type | 学術雑誌論文 / Journal Article(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2019-05-08 | |||||
タイトル | ||||||
タイトル | Parity-violating gravity and GW170817 | |||||
言語 | en | |||||
著者 |
Nishizawa, Atsushi
× Nishizawa, Atsushi× Kobayashi, Tsutomu |
|||||
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 | We consider gravitational waves (GWs) in generic parity-violating gravity, including recently proposed ghost-free theories with parity violation as well as Chern-Simons (CS) modified gravity, and study the implications of observational constraints from GW170817/GRB 170817A. Whereas GWs propagate at the speed of light, c, in CS gravity, we point out that this is specific to CS gravity and the GW propagation speed deviates from c, in general, in parity-violating gravity. Therefore, contrary to the previous literature in which only CS gravity is studied as a concrete example, we show that GW170817/GRB 170817A can, in fact, be used to limit gravitational parity violation. Our argument implies that the constraint on the propagation speed of GWs can pin down the parity-violating sector, if any, to CS gravity. | |||||
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.98.124018 | |||||
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 98, 号 12, p. 124018, 発行日 2018-12-15 |
|||||
著者版フラグ | ||||||
値 | publisher |