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A Fourier-space variance in three dimensions is scale invariant when the dimensionless power per logarithmic wavenumber interval,
is independent of . For a massless inflaton mode at late times,
so is constant.

Ancestors (10)

  1. Bunch-Davies vacuum
  2. Canonically rescaled de Sitter scalar mode
  3. Inflationary scalar Fourier mode
  4. Inflaton action in an expanding universe
  5. Inflaton
  6. Cosmic inflation
  7. Cosmology
  8. Branch of physics
  9. Physics
  10. Home