ログイン
言語:

WEKO3

  • トップ
  • ランキング
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

{"_buckets": {"deposit": "99a2ca47-3a42-4ea4-8717-4d70644cf2c3"}, "_deposit": {"id": "25692", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "25692"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00025692", "sets": ["696"]}, "author_link": ["76078", "76079", "76080"], "item_10_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2017-12-01", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "12", "bibliographicPageStart": "124003", "bibliographicVolumeNumber": "96", "bibliographic_titles": [{"bibliographic_title": "Physical Review D", "bibliographic_titleLang": "en"}]}]}, "item_10_description_4": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We make a theoretical prediction for the ratio of the dark energy to other components in the Universe based on the scenario of the sequestering mechanism which was recently proposed as one possible way to solve the cosmological constant problem. In order to evaluate the value of dark energy and the others, we assume a specific scale factor which describes the big-crunch scenario in the scalar-tensor theory. We specify the parameter region where the one can explain the observed dark energy-matter ratio.", "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.96.124003", "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": "2470-0010", "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": "Tsukamoto, Takuma", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "76078", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Katsuragawa, Taishi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "76079", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Nojiri, Shin’ichi", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "76080", "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": "2018-04-16"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "PhysRevD96_124003.pdf", "filesize": [{"value": "627.1 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 627100.0, "url": {"label": "PhysRevD96_124003", "objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/25692/files/PhysRevD96_124003.pdf"}, "version_id": "d73d5249-0a2a-48aa-9ad8-282d41b883d3"}]}, "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": "Sequestering mechanism in scalar-tensor gravity", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Sequestering mechanism in scalar-tensor gravity", "subitem_title_language": "en"}]}, "item_type_id": "10", "owner": "1", "path": ["696"], "permalink_uri": "http://hdl.handle.net/2237/00027903", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2018-04-16"}, "publish_date": "2018-04-16", "publish_status": "0", "recid": "25692", "relation": {}, "relation_version_is_last": true, "title": ["Sequestering mechanism in scalar-tensor gravity"], "weko_shared_id": -1}
  1. B100 理学部/理学研究科
  2. B100a 雑誌掲載論文
  3. 学術雑誌

Sequestering mechanism in scalar-tensor gravity

http://hdl.handle.net/2237/00027903
http://hdl.handle.net/2237/00027903
5eb5ad4a-b56a-4624-98c7-59f41586e1ff
名前 / ファイル ライセンス アクション
PhysRevD96_124003.pdf PhysRevD96_124003 (627.1 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2018-04-16
タイトル
タイトル Sequestering mechanism in scalar-tensor gravity
言語 en
著者 Tsukamoto, Takuma

× Tsukamoto, Takuma

WEKO 76078

en Tsukamoto, Takuma

Search repository
Katsuragawa, Taishi

× Katsuragawa, Taishi

WEKO 76079

en Katsuragawa, Taishi

Search repository
Nojiri, Shin’ichi

× Nojiri, Shin’ichi

WEKO 76080

en Nojiri, Shin’ichi

Search repository
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 © 2017 American Physical Society
抄録
内容記述 We make a theoretical prediction for the ratio of the dark energy to other components in the Universe based on the scenario of the sequestering mechanism which was recently proposed as one possible way to solve the cosmological constant problem. In order to evaluate the value of dark energy and the others, we assume a specific scale factor which describes the big-crunch scenario in the scalar-tensor theory. We specify the parameter region where the one can explain the observed dark energy-matter ratio.
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.96.124003
ISSN
収録物識別子タイプ PISSN
収録物識別子 2470-0010
書誌情報 en : Physical Review D

巻 96, 号 12, p. 124003, 発行日 2017-12-01
著者版フラグ
値 publisher
戻る
0
views
See details
Views

Versions

Ver.1 2021-03-01 13:25:37.908454
Show All versions

Share

Mendeley Twitter Facebook Print Addthis

Cite as

エクスポート

OAI-PMH
  • OAI-PMH JPCOAR
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX

Confirm


Powered by WEKO3


Powered by WEKO3