Second-order corrections to Starobinsky inflation
Higher-order theories of gravity are extensions to general relativity (GR) motivated mainly by high-energy physics searching for GR ultraviolet completeness. They are characterized by the inclusion of correction terms in the Einstein–Hilbert action that leads to higher-order field equations. In this...
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Published in: | The European physical journal. C, Particles and fields Vol. 83; no. 11; pp. 1032 - 19 |
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Main Authors: | , |
Format: | Journal Article |
Language: | English |
Published: |
Berlin/Heidelberg
Springer Berlin Heidelberg
01-11-2023
Springer Springer Nature B.V SpringerOpen |
Subjects: | |
Online Access: | Get full text |
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Summary: | Higher-order theories of gravity are extensions to general relativity (GR) motivated mainly by high-energy physics searching for GR ultraviolet completeness. They are characterized by the inclusion of correction terms in the Einstein–Hilbert action that leads to higher-order field equations. In this paper, we propose investigating inflation due to the GR extension built with all correction terms up to the second-order involving only the scalar curvature
R
, namely,
R
2
,
R
3
,
R
□
R
. We investigate inflation within the Friedmann cosmological background, where we study the phase space of the model, as well as explore inflation in slow-roll leading-order. Furthermore, we describe the evolution of scalar perturbations and properly establish the curvature perturbation. Finally, we confront the proposed model with recent observations from Planck, BICEP3/Keck, and BAO data. |
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ISSN: | 1434-6052 1434-6044 1434-6052 |
DOI: | 10.1140/epjc/s10052-023-12149-8 |