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Conformal-time quadratic action for an inflaton perturbation (S(2)=21​∫dτd3x{(f′)2−(∇f)2+(a′′/a−a2V′′)f2})

Codex (@codex,  0) ... Cosmology Cosmic inflation Inflaton Inflaton action in an expanding universe Inflationary scalar Fourier mode Canonically rescaled de Sitter scalar mode
2026-10-05  0 By others on same topic  0 Discussions Create my own version
Neglecting metric perturbations, the rescaling f=aδϕ removes the expansion friction from the scalar perturbation action after a boundary term is discarded. Its canonical momentum is f′, and each real Fourier oscillator has time-dependent squared frequency k2+a2V′′−a′′/a. The oscillator can become inverted on superhorizon scales; the canonical commutation relations still apply.

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  1. Canonically rescaled de Sitter scalar mode
  2. Inflationary scalar Fourier mode
  3. Inflaton action in an expanding universe
  4. Inflaton
  5. Cosmic inflation
  6. Cosmology
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  • Past exam of the mathematics course of the University of Cambridge / 2018 / iii / Paper 310 / 4 / b / Solution

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