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From conformal field theory spectra to CMB multipoles in quantum gravity cosmology
https://ir.soken.ac.jp/records/3337
https://ir.soken.ac.jp/records/3337c6736c05-98f0-44b5-9d16-be726662d521
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2013-01-24 | |||||
タイトル | ||||||
タイトル | From conformal field theory spectra to CMB multipoles in quantum gravity cosmology | |||||
タイトル | ||||||
タイトル | From conformal field theory spectra to CMB multipoles in quantum gravity cosmology | |||||
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, Ken-ji
× HAMADA, Ken-ji× HORATA, Shinichi× 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 | We study the inflation process of the Universe based on the renormalizable quantum gravity formulated as a conformal field theory. We show that the power-law conformal field theory spectrum approaches that of the Harrison-Zel’dovich-Peebles–type as the amplitude of gravitational potential gradually reduces during the inflation. The non-Gaussanity parameter is preserved within an order of unity due to the diffeomorphism invariance. Sharp falloff of the angular power spectrum of cosmic microwave background at large scale is understood as a consequence of the existence of dynamical scale of the quantum gravity ΛQG(≃1017 GeV). The angular power spectra are computed and compared with the WMAP5 and ACBAR data with a quality of χ2/dof≃1.1. | |||||
書誌情報 |
Physical Review D - Particles, Fields, Gravitation and Cosmology en : Physical Review D - Particles, Fields, Gravitation and Cosmology 巻 81, 号 8, 発行日 2010-04-28 |
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出版者 | ||||||
出版者 | American Physical Society | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 15507998 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | https://doi.org/10.1103/PhysRevD.81.083533 | |||||
関連名称 | 10.1103/PhysRevD.81.083533 | |||||
権利 | ||||||
権利情報 | © 2010 The American Physical Society |