Inflation from a generalized exponential plateau: towards extra suppressed tensor-to-scalar ratios
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| Format: | Preprint |
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2025
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| _version_ | 1866909898996973568 |
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| author | Kouniatalis, Gerasimos Saridakis, Emmanuel N. |
| author_facet | Kouniatalis, Gerasimos Saridakis, Emmanuel N. |
| contents | We investigate a standard minimally-coupled scalar-field inflationary scenario, which is based on a new potential, with suitably generalized plateau features, that leads to extra small tensor-to-scalar ratios. In particular, we consider a specific three-parameter potential, which has a flatter plateau and a steeper well compared to the Starobinsky potential in the Einstein frame. We study the inflationary realization and we show that it guarantees a prolonged period of slow-roll inflation and a successful exit. Additionally, the steeper minimum leads to significantly suppressed tensor perturbations, and thus to an extra-small tensor-to-scalar ratio $r$, and we show that we are able to obtain $r$ values less than $10^{-5}$. Moreover, we calculate the reheating temperature showing that in order to be in agreement with observations one of the potential parameters should remain within specific bounds. Finally, performing an inverse conformal transformation to the Jordan frame we show that the considered potential corresponds to higher-order corrections to Starobinsky potential in the Einstein frame, and these corrections are the reason for the improved behavior of the tensor-to-scalar ratio. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2507_17721 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Inflation from a generalized exponential plateau: towards extra suppressed tensor-to-scalar ratios Kouniatalis, Gerasimos Saridakis, Emmanuel N. Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology We investigate a standard minimally-coupled scalar-field inflationary scenario, which is based on a new potential, with suitably generalized plateau features, that leads to extra small tensor-to-scalar ratios. In particular, we consider a specific three-parameter potential, which has a flatter plateau and a steeper well compared to the Starobinsky potential in the Einstein frame. We study the inflationary realization and we show that it guarantees a prolonged period of slow-roll inflation and a successful exit. Additionally, the steeper minimum leads to significantly suppressed tensor perturbations, and thus to an extra-small tensor-to-scalar ratio $r$, and we show that we are able to obtain $r$ values less than $10^{-5}$. Moreover, we calculate the reheating temperature showing that in order to be in agreement with observations one of the potential parameters should remain within specific bounds. Finally, performing an inverse conformal transformation to the Jordan frame we show that the considered potential corresponds to higher-order corrections to Starobinsky potential in the Einstein frame, and these corrections are the reason for the improved behavior of the tensor-to-scalar ratio. |
| title | Inflation from a generalized exponential plateau: towards extra suppressed tensor-to-scalar ratios |
| topic | Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2507.17721 |