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Constraining running non-gaussianity

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2];  [3];  [4];  [5]
  1. Institut de Physique Théorique, CEA, IPhT, F-91191 Gif-sur-Yvette (France)
  2. DAMTP, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA (United Kingdom)
  3. Center for Astrophysics, Harvard University, Cambridge, MA 02138 (United States)
  4. Center for Particle Astrophysics, Fermilab, Batavia, IL 60510 (United States)
  5. Laboratory for Elementary Particle Physics, Cornell University, Ithaca, NY 14853 (United States)

The primordial non-Gaussian parameter f{sub NL} has been shown to be scale-dependent in several models of inflation with a variable speed of sound, such as Dirac-Born-Infeld (DBI) models. We perform a Fisher matrix analysis of the bispectra of the temperature and polarization of the Cosmic Microwave Background (CMB) radiation and derive the expected constraints on the parameter n{sub NG} that quantifies the running of f{sub NL}(k) for current and future CMB missions. We find that CMB information alone, in the event of a significant detection of the non-Gaussian component, corresponding to f{sub NL} = 50 for the local model and f{sub NL} = 100 for the equilateral model of non-Gaussianity, is able to determine n{sub NG} with a 1-σ uncertainty of n{sub NG} ≅ 0.1 and Δn{sub NG} ≅ 0.3, respectively, for the Planck mission and a factor of two better for CMBPol. In addition, we show how future large-scale structure observations should achieve results comparable to or even better than those from the CMB, while showing some complementarity due to the different distribution of the non-Gaussian signal over the relevant range of scales. Finally, we compare our findings to the predictions on the amplitude and running of non-Gaussianity of DBI inflation, showing how the constraints on a scale-dependent f{sub NL}(k) translate into constraints on the parameter space of the theory.

OSTI ID:
22273131
Journal Information:
Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 12 Vol. 2009; ISSN 1475-7516
Country of Publication:
United States
Language:
English

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