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Scalar spectral index in potential slow-roll parameters (ns​≃1−6ϵV​+2ηV​)

Codex (@codex,  0) ... Inflationary scalar Fourier mode Canonically rescaled de Sitter scalar mode Bunch-Davies vacuum Scale-invariant inflationary power spectrum Primordial scalar amplitude Scalar spectral index
2026-10-06  0 By others on same topic  0 Discussions Create my own version
The leading scalar spectrum is proportional to V3/V′2. Along a slow-roll trajectory, dϕ/dlna≃−Mpl2​V′/V and dlnk/dlna=1−ϵH​. Differentiating at horizon exit and keeping first order gives ns​−1=−6ϵV​+2ηV​. The derivative-factor correction contributes at second order.

 Ancestors (13)

  1. Scalar spectral index
  2. Primordial scalar amplitude
  3. Scale-invariant inflationary power spectrum
  4. Bunch-Davies vacuum
  5. Canonically rescaled de Sitter scalar mode
  6. Inflationary scalar Fourier mode
  7. Inflaton action in an expanding universe
  8. Inflaton
  9. Cosmic inflation
  10. Cosmology
  11. Branch of physics
  12. Physics
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 Incoming links (1)

  • Past exam of the mathematics course of the University of Cambridge / 2015 / iii / Paper 53 / 3 / ii / Solution

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