On the superstring-inspired quantum correction to the Starobinsky model of inflation
arXiv:2211.01546 · doi:10.1088/1475-7516/2022/12/032
Abstract
Superstring/M-theory is the theory of quantum gravity that can provide the UV-completion to viable inflation models. We modify the Starobinsky inflation model by adding the Bel-Robinson tensor squared term proposed as the leading quantum correction inspired by superstring theory. The model under consideration has two parameters: the inflaton mass and the string-inspired positive parameter . We derive the equations of motion in the Friedmann-Lemaitre-Robertson-Walker universe and investigate its solutions. We find the physical bounds on the value of the parameter by demanding the absence of ghosts and consistency of the derived inflationary observables with the measurements of the cosmic microwave background radiation.
24 pages, 5 figures, LaTeX; the version to appear in JCAP
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- Stability investigations of isotropic and anisotropic exponential inflation in the Starobinsky-Bel-Robinson gravity
- Starobinsky inflation beyond the leading order
- New one-parametric extension of the Starobinsky inflationary model
- Black hole solutions to Einstein-Bel-Robinson gravity
- More accurate slow-roll approximations for inflation in scalar-tensor theories
- Anisotropic solutions for gravity model with a scalar field
- Stability investigations of de Sitter inflationary solutions in power-law extensions of the Starobinsky model
- Starobinsky inflation and Swampland conjectures
- Effect of on the stability of de Sitter solution of the generalized Einsteinian cubic gravity
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