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Inflationary Epoch

Inflation proposes a period of extremely rapid exponential expansion in the very early universe, driven by a hypothetical scalar field (the inflaton).
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The statement of the theorem

Inflation is modeled by the action S=d4xg(12MPl2R12gμνμϕνϕV(ϕ))S = \int d^4 x \sqrt{-g} \left( \frac{1}{2} M_{Pl}^2 R - \frac{1}{2} g^{\mu\nu} \partial_\mu \phi \partial_\nu \phi - V(\phi) \right). Assuming a slow-roll regime, the equation of motion for the inflaton field ϕ\phi is approximated by the Klein-Gordon equation in a curved background:\nϕ¨+3Hϕ˙+V(ϕ)=0\ddot{\phi} + 3H \dot{\phi} + V'(\phi) = 0The slow-roll conditions require 12MPl2(V(ϕ)V(ϕ))21\frac{1}{2} M_{Pl}^2 \left(\frac{V'(\phi)}{V(\phi)}\right)^2 \ll 1 and MPl2V(ϕ)V(ϕ)1M_{Pl}^2 \left|\frac{V''(\phi)}{V(\phi)}\right| \ll 1, ensuring ϕ¨3Hϕ˙\ddot{\phi} \ll 3H \dot{\phi}.
Source: Wikipedia