Primordial gravitational waves in bimetric gravity
抄録
We study primordial tensor power-spectra generated during inflation in bimetric gravity. More precisely, we examine a homogeneous expanding spacetime in a minimal bimetric model with an inflaton and calculate tensor perturbations on the homogeneous background under slow-roll approximation. In terms of the mass eigenstates, only the power-spectrum of the massless state remains constant and both the power-spectrum of the massive state and the cross power-spectrum rapidly decay during inflation. The amplitude of the physical power-spectrum is suppressed due to the flavor mixing. All power-spectra in the flavor eigenstates coincide with each other up to the first order of the slow-roll parameter.
収録刊行物
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- Journal of Cosmology and Astroparticle Physics
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Journal of Cosmology and Astroparticle Physics 2015 2015-09-02
IOP Publishing
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詳細情報 詳細情報について
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- CRID
- 1050845760768361984
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- NII論文ID
- 120005841437
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- ISSN
- 14757516
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- HANDLE
- 2433/216583
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- 本文言語コード
- en
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- 資料種別
- journal article
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- データソース種別
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- IRDB
- CiNii Articles