OurBigBook About$ Donate
 Sign in Sign up

Running of the scalar spectral index (αs​=dns​/dlogk≃16ϵV​ηV​−24ϵV2​−2ξV2​)

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
2026-10-14  0 By others on same topic  0 Discussions Create my own version
The running describes the scale dependence of the scalar spectral index. Differentiating ns​−1≃−6ϵV​+2ηV​ with the potential slow-roll flow equations gives the displayed second-order slow-roll result. It includes the third potential slow-roll parameter and is generally smaller than the leading spectral tilt.

 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. Branches of physics
  12. Physics
  13.  Home

 Incoming links (2)

  • Past exam of the mathematics course of the University of Cambridge / 2009 / iii / Paper 55 / 5 / e / Solution
  • Third potential slow-roll parameter

 View article source

 Discussion (0)

New discussion

There are no discussions about this article yet.

 Articles by others on the same topic (0)

There are currently no matching articles.
  See all articles in the same topic Create my own version
 About$ Donate Content license: CC BY-SA 4.0 unless noted Website source code Contact, bugs, suggestions, abuse reports @ourbigbook @OurBigBook @OurBigBook