We investigate a (super-)renormalizable and ghost-free theory of gravity, showing that under a natural (exponential) ansatz of the form factor and a suitable truncation it can give rise to the Starobinsky inflationary theory in cosmological frameworks, and thus offering a theoretical justification of its origin. We study the corresponding inflationary evolution and we examine the generation of curvature perturbations, adapting the f(R)-like equations in a symmetry-reduced Friedmann-Lemaıˆtre-Robertson-Walker metric. Furthermore, we analyze how the ultraviolet regime of a simply renormalizable and unitary theory of gravity is also compatible with the Starobinsky action, and hence we show that such a theory could account for an inflationary phase of the Universe in the ultraviolet regime.

Briscese, F., Antonino, M., Leonardo, M., Emmanuel, N.S. (2013). Inflation in (Super-)renormalizable Gravity. PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, 87(8), 1-7 [10.1103/PhysRevD.87.083507].

Inflation in (Super-)renormalizable Gravity

Briscese F;
2013-01-01

Abstract

We investigate a (super-)renormalizable and ghost-free theory of gravity, showing that under a natural (exponential) ansatz of the form factor and a suitable truncation it can give rise to the Starobinsky inflationary theory in cosmological frameworks, and thus offering a theoretical justification of its origin. We study the corresponding inflationary evolution and we examine the generation of curvature perturbations, adapting the f(R)-like equations in a symmetry-reduced Friedmann-Lemaıˆtre-Robertson-Walker metric. Furthermore, we analyze how the ultraviolet regime of a simply renormalizable and unitary theory of gravity is also compatible with the Starobinsky action, and hence we show that such a theory could account for an inflationary phase of the Universe in the ultraviolet regime.
Briscese, F., Antonino, M., Leonardo, M., Emmanuel, N.S. (2013). Inflation in (Super-)renormalizable Gravity. PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, 87(8), 1-7 [10.1103/PhysRevD.87.083507].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/427113
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