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astro-ph.COOct 21, 2010
5
citations (OpenAlex)
authors
  • G. L. Alberghi
  • R. Casadio
arXiv abstractPDF
paper

Non-Gaussianity from Compositeness

arXiv:1010.4395

Abstract

By assuming the field seeding the curvature perturbations ζ is a dynamically arising condensate, we are able to derive the relation fNL2​≃108H/Mc​ between the non-Gaussianity parameter fNL​ and the ratio of the inflationary scale H to the cutoff scale Mc​ of the effective theory describing the condensate, thus relating the experimental bound on fNL​ to a bound on Mc​.

7 pages,1 figure

References in corpus (13)

  • Non-Gaussian features of primordial fluctuations in single field inflationary models
  • The inflationary prediction for primordial non-gaussianity
  • Limits on non-Gaussianities from WMAP data
  • Detecting a small perturbation through its non-Gaussianity
  • A new method for calculating the primordial bispectrum in the squeezed limit
  • The cosmological BCS mechanism and the Big Bang Singularity
  • On the squeezed limit of the bispectrum in general single field inflation
  • Scale-Dependent Non-Gaussianity as a Generalization of the Local Model
  • Testing gaussianity, homogeneity and isotropy with the cosmic microwave background
  • Gravity Induced Chiral Condensate Formation and the Cosmological Constant
  • Testing gravity with non-Gaussianity
  • CMB: A Look Inside the Inflaton
  • A fine tuning free resolution of the cosmological constant problem

Cited by in corpus (2)

  • Minimal Composite Inflation
  • BICEP2 constrains Composite Inflation
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