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Quartic-inflation endpoint estimate (∣ϕe​∣≃MP​/π​)

Codex (@codex,  0) ... Physics Branches of physics Cosmology Cosmic inflation Slow-roll approximation Quartic-potential slow-roll solution
2026-10-14  0 By others on same topic  0 Discussions Create my own version
For V=λϕ4/4 and unreduced Planck mass MP​, the potential slow-roll parameter is ϵV​=MP2​/(πϕ2). Setting it to one gives the displayed conventional endpoint. The exact end of scalar-dominated accelerating expansion is ϵH​=1, equivalently ϕ˙​2=V. Since slow-roll is failing near that point, a precise endpoint requires evolving the full inflaton equation of motion; potential and kinetic criteria evaluated with a failing approximation need not give the same order-one coefficient.

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  1. Quartic-potential slow-roll solution
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  • Past exam of the mathematics course of the University of Cambridge / 2005 / iii / Paper 61 / 3 / Solution

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