Chromo-natural inflation in the axiverse
書誌事項
- 公開日
- 2015-09-16
- 資源種別
- journal article
- 権利情報
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- ©2015 American Physical Society
- DOI
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- 10.1103/physrevd.92.063516
- 10.48550/arxiv.1412.7620
- 公開者
- American Physical Society (APS)
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説明
We study chromo-natural inflation in the axiverse. More precisely, we investigate natural inflation with two axions coupled with a SU(2) gauge field. Assuming a hierarchy between the coupling constants, we find that for certain initial conditions, conventional natural inflation commences and continues for tens of e-foldings, and subsequently chromo-natural inflation takes over from natural inflation. For these solutions, we expect that the predictions are in agreement with observations on CMB scales. Moreover, since chromo-natural inflation occurs in the latter part of the inflationary stage, chiral primordial gravitational waves are produced in the interesting frequency range higher than $10^{-10}$Hz, which might be detectable by future gravitational wave observations.
16 pages, 3 figures
収録刊行物
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- Physical Review D
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Physical Review D 92 (6), 063516-063516, 2015-09-16
American Physical Society (APS)
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キーワード
- High Energy Physics - Theory
- Cosmology and Nongalactic Astrophysics (astro-ph.CO)
- FOS: Physical sciences
- General Relativity and Quantum Cosmology (gr-qc)
- General Relativity and Quantum Cosmology
- High Energy Physics - Phenomenology
- High Energy Physics - Phenomenology (hep-ph)
- High Energy Physics - Theory (hep-th)
- Astrophysics - Cosmology and Nongalactic Astrophysics
詳細情報 詳細情報について
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- CRID
- 1050294045371017472
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- NII論文ID
- 120005971341
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- ISSN
- 15502368
- 15507998
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- HANDLE
- 20.500.14094/90003794
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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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