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Equation 69 for cosmological constant domination simplifies to Φ′′ + 3HΦ′ + 3H2 + 5 Φ = 0, (112) where we usedc2 s,T = 0, wef f= −Ωe ∼ −(1 + ΩK) = − 1 + 1 H2 · 2000

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astro-ph.CO 1

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2025 1

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Cosmological Perturbations from a New Approach to Inflation

astro-ph.CO · 2025-01-08 · conditional · novelty 6.0

A nearly static 'lingering' phase before inflation is unstable, and the growth of perturbations during that phase could seed the transition to inflation and leave observable curvature or transplanckian signatures.

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  • Cosmological Perturbations from a New Approach to Inflation astro-ph.CO · 2025-01-08 · conditional · none · ref 3

    A nearly static 'lingering' phase before inflation is unstable, and the growth of perturbations during that phase could seed the transition to inflation and leave observable curvature or transplanckian signatures.