strong dynamics and inflation: a review
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ID: 137926
2015
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Abstract
In this article, we review how strong dynamics can be efficiently employed as a viable alternative to study the mechanism of cosmic inflation. We examine single-field inflation in which the inflaton emerges as a bound state stemming from various strongly interacting field theories. We constrain the number of e-foldings for composite models of inflation in order to obtain a successful inflation. We study a set of cosmological parameters, e.g., the primordial spectral index ns and tensor-to-scalar ratio r, and confront the predicted results with the joint Planck data, and with the recent BICEP2 data.
| Reference Key |
channuie2015nuclearstrong
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|---|---|
| Authors | ;Phongpichit Channuie |
| Journal | biology and fertility of soils |
| Year | 2015 |
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