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PhysRevLett.127.091602.pdf | 360.47 kB | Adobe PDF | 見る/開く |
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DCフィールド | 値 | 言語 |
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dc.contributor.author | Aoki, Katsuki | en |
dc.contributor.author | Tran Quang Loc | en |
dc.contributor.author | Noumi, Toshifumi | en |
dc.contributor.author | Tokuda, Junsei | en |
dc.contributor.alternative | 青木, 勝輝 | ja |
dc.date.accessioned | 2022-10-14T07:05:09Z | - |
dc.date.available | 2022-10-14T07:05:09Z | - |
dc.date.issued | 2021-08 | - |
dc.identifier.uri | http://hdl.handle.net/2433/276729 | - |
dc.description.abstract | We study compatibility of the standard model of particle physics and general relativity by means of gravitational positivity bounds, which provide a necessary condition for a low-energy gravitational theory to be UV completable within the weakly coupled regime of gravity. In particular, we identify the cutoff scale of the standard model coupled to gravity by studying consistency of light-by-light scattering. While the precise value depends on details of the Pomeron effects in QCD, the cutoff scale reads 10¹⁶ GeV if the single-Pomeron exchange picture works well up to this scale. We also demonstrate that the cutoff scale is lowered to 10¹³ GeV if we consider the electroweak theory without the QCD sector. | en |
dc.language.iso | eng | - |
dc.publisher | American Physical Society (APS) | en |
dc.rights | Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3. | en |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | - |
dc.subject | Effective field theory | en |
dc.subject | Electroweak interaction | en |
dc.subject | General relativity | en |
dc.subject | Quantum gravity | en |
dc.subject | Scattering amplitudes | en |
dc.subject | Strong interaction | en |
dc.subject | Particles & Fields | en |
dc.subject | Gravitation, Cosmology & Astrophysics | en |
dc.title | Is the Standard Model in the Swampland? Consistency Requirements from Gravitational Scattering | en |
dc.type | journal article | - |
dc.type.niitype | Journal Article | - |
dc.identifier.jtitle | Physical Review Letters | en |
dc.identifier.volume | 127 | - |
dc.identifier.issue | 9 | - |
dc.relation.doi | 10.1103/PhysRevLett.127.091602 | - |
dc.textversion | publisher | - |
dc.identifier.artnum | 091602 | - |
dc.identifier.pmid | 34506162 | - |
dcterms.accessRights | open access | - |
datacite.awardNumber | 19J00895 | - |
datacite.awardNumber | 20K14468 | - |
datacite.awardNumber | 17H02894 | - |
datacite.awardNumber | 20H01902 | - |
datacite.awardNumber | 21H00075 | - |
datacite.awardNumber | 21K13922 | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-19J00895/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-20K14468/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-17H02894/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-20H01902/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PUBLICLY-21H00075/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-21K13922/ | - |
dc.identifier.pissn | 0031-9007 | - |
dc.identifier.eissn | 1079-7114 | - |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.awardTitle | 基礎物理から探る重力理論の拡張とその観測検証 | ja |
jpcoar.awardTitle | 初期宇宙観測を用いた重力場の基本変数の検証 | ja |
jpcoar.awardTitle | 自発的対称性の破れで解明するCMBアノーマリーの起源 | ja |
jpcoar.awardTitle | 「弱い重力予想」に基づく素粒子論・宇宙論:量子重力理論への現象論的アプローチ | ja |
jpcoar.awardTitle | 量子重力で探るニュートリノ質量の起源 | ja |
jpcoar.awardTitle | ユニタリー性を鍵とするインフレーション宇宙の観測に基づく超弦理論の検証 | ja |
出現コレクション: | 学術雑誌掲載論文等 |
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