| Autor: |
Aguilar, José Edgar Madriz, Zamarripa, J., Montes, M., Licea, J. A., Loza, C. De, Peraza, A. |
| Zdroj: |
European Physical Journal Plus; Jan2022, Vol. 137 Issue 1, p1-13, 13p |
| Abstrakt: |
In this paper assuming a 5D quantum pre-inflationary vacuum energy, we propose a manner to extend some Λ (t) -CDM models to the inflationary period by using dynamical foliations of the five-dimensional (5D) Ricci-flat space-time manifold, regarding a non-compact extra space-like coordinate. In this formalism, we achieve also a geometrical unification of inflation and the present accelerating epoch. In this approach, inflation is generated by a pre-inflationary quantum vacuum energy that maintains the 5D classical vacuum on cosmological scales. We obtain from geometrical conditions that we can model the presence of the pre-inflationary vacuum energy in 4D as a dynamical cosmological constant. In this model, the 4D inflationary period is governed by a power law expansion and for certain values of some parameters of the model, we obtain an spectral index satisfying 0.9607 ≤ n s ≤ 0.9691 and a scalar-to-tensor ratio r = 0.098 , values that fit well according to Planck 2018 results. The 4D inflationary potential is induced for the 5D geometry and the 4D pre-inflationary potential is determined by the model and its contribution is necessary so that n s and r can fit the observational data. We also show that in this theoretical framework, the present acceleration in the expansion of the universe can be explained due to a remanent of this pre-inflationary vacuum energy scaled to the present epoch and that its description can be done with the same Λ (t) . In this period, we obtain a deceleration parameter in agreement with Planck 2018 data under certain restrictions of the parameters of the model. From the geometrical point of view, Λ (t) is depending on the dynamical foliation of the 5D space-time manifold. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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