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Analyzing WMAP observation by quantum gravity
https://ir.soken.ac.jp/records/3948
https://ir.soken.ac.jp/records/3948b69103e2-7ac4-4341-bf71-5e95447f59ea
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2013-09-17 | |||||
タイトル | ||||||
タイトル | Analyzing WMAP observation by quantum gravity | |||||
タイトル | ||||||
タイトル | Analyzing WMAP observation by quantum gravity | |||||
言語 | en | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
HAMADA, Keri-ji
× HAMADA, Keri-ji× HORATA, Shinichi× SUGIYAMA, Naoshi× YUKAWA, Tetsuyuki |
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著者別名 |
湯川, 哲之
× 湯川, 哲之 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The angular power spectra of cosmic microwave background are analyzed under the light of the evolutional scenario of the universe based on the renormalizable quantum theory of gravity in four dimensions. The equation of evolution is solved numerically fixing the power law spectrum predicted by the conformal gravity for the initial condition. The equation requires to introduce a dynamical energy scale about 1017GeV, where the inflationary spacetime evolution makes a transition to the big-bang of the conventional Friedmann universe. The quality of fit to the three-year data of WMAP implies the possibility to understand the observation by quantum gravity. | |||||
書誌情報 |
Progress of Theoretical Physics en : Progress of Theoretical Physics 巻 119, 号 2, p. 253-262, 発行日 2008-02 |
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出版者 | ||||||
出版者 | The Physical Society of Japan | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0033-068X | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | https://doi.org/10.1143/PTP.119.253 | |||||
関連名称 | 10.1143/PTP.119.253 | |||||
権利 | ||||||
権利情報 | © 2013 The Physical Society of Japan |