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Inflation with explicit parametric connection between General Relativity and Scalar-Tensor gravity

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abstract

In this paper we consider the cosmological inflation within scalar-tensor gravity and compare it with standard inflation based on general relativity. The difference is determined by the value of the parameter $\Delta$. This approach is associated with using the special ansatz which links a function that defines a type of gravity with a scale factor of the universe.

fields

hep-th 1

years

2021 1

verdicts

UNVERDICTED 1

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