Non-Gaussianity and Loop Corrections in a Quadratic Two-Field Slow-Roll Model of Inflation. Part I
Published 2007-04-30
Keywords
- :non-gaussianity,
- bispectrum,
- loop corrections
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Abstract
In this paper it is shown that it is possible to attain a high level of non-gaussianity in a particular quadratic two-field slow-roll model of inflation by taking care of loop corrections both in the spectrum and the bispectrum. A big fNL is obtained even if ζis generated during inflation. Five issues are in consideration when constraining the available parameter space: 1. we must be sure that we are in a perturbative regime; 2. We must apply the correct condition about the (possible) loop dominance in Bζor Pζ; 3. we must satisfy the spectrum normalisation condition; 4. We must satisfy the spectral tilt constraint; 5. we must have enough inflation to solve the horizon problem.
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References
[2] C.T. Byrnes, K. Koyama, M. Sasaki, D. Wands, “Diagrammatic Approach to Non-Gaussianity from Inflation”, Journal of Cosmology and Astroparticle Physics, 0711, 027 (2007).
[3] H.R.S. Cogollo, Y. Rodríguez, C.A. Valenzuela-Toledo, “Non-Gaussianityand Loop Corrections in a Quadratic Two-Field Slow-Roll Model of Inflation. Part I”, To be submitted.
[4] H.R.S. Cogollo, Y. Rodríguez, C.A. Valenzuela-Toledo, “Non-Gaussianity and Loop Corrections in a Quadratic Two-Field Slow-Roll Model of Inflation. Part II”, To be submitted.