Quantum cosmological perturbations: predictions and observations

By V. Mukhanov. 2013

169 citations recorded by the source corpus.

I consider the generic model independent predictions of the theory of quantum cosmological perturbations. To describe the stage of cosmic inflation, where these perturbations are amplified, the hydrodynamical approach is used. The inflationary stage is completely characterized by the deviation of the equation of state from cosmological constant which is a smooth function of the number of e-folds until the end of inflation. It is shown that in this case the spectral index should deviate from the flat one at least by 3 percent irrespective of any particular scenario. Given the value of the spectral index a lower bound on the amount of gravitational waves produced is derived. Finally the relation between effective hydrodynamical description of inflation and inflationary scenarios is discussed.

Subfields: Astronomy and Astrophysics, Electrical and Electronic Engineering, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/755f40b4dd1ba2986f9b912f739c9a70711f121c

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

  1. Andrei Linde
  2. Marco Peloso
  3. R. Kallosh
  4. D. Roest
  5. Juan García-Bellido
  6. C. Caprini
  7. Daniel G. Figueroa
  8. P. Bin'etruy

In Electrical and Electronic Engineering

  1. C. Caprini
  2. P. Bin'etruy
  3. D. Roest
  4. L. Sorbo
  5. M. Pieroni
  6. S. Vagnozzi
  7. V. Domcke

In Nuclear and High Energy Physics

  1. Andrei Linde
  2. R. Kallosh
  3. Marco Peloso
  4. D. Roest
  5. C. Caprini
  6. Juan García-Bellido
  7. S. Vagnozzi
  8. Daniel G. Figueroa

Citations in the corpus