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A wide range of multifield inflationary models generate non-Gaussian initial conditions in which the initial adiabatic fluctuation is of the form (zeta_G + g_{NL} zeta_G^3).
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2008
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2008
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S. Matarrese and L. Verde, “The effect of primordial non-Gaussianity on halo bias,” Astrophys. J
2008
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2008
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2004
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P. Creminelli and M. Zaldarriaga, “Single field consistency relation for the 3-point function,” JCAP
2004
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V. Springel, “The cosmological simulation code GADGET-2,” Mon. Not. Roy. Astron. Soc
2005
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M. Sasaki, J. Valiviita, and D. Wands, “Non-gaussianity of the primordial perturbation in the curvaton model,” Phys. Rev
2006
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M. S. Warren, K. Abazajian, D. E. Holz, and L. Teodoro, “Precision Determination of the Mass Function of Dark Matter Halos,” Astrophys. J
2006
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M. Crocce, S. Pueblas, and R. Scoccimarro, “Transients from Initial Conditions in Cosmological Simulations,” Mon. Not. Roy. Astron. Soc
2006
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P. Creminelli and L. Senatore, “A smooth bouncing cosmology with scale invariant spectrum,” JCAP
2007
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2009
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2009
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P. Chingangbam and Q.-G. Huang, “The Curvature Perturbation in the Axion-type Curvaton Model,” JCAP
2009
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2009
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C. T. Byrnes and G. Tasinato, “Non-Gaussianity beyond slow roll in multi-field inflation,” JCAP
2009
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WMAP Collaboration, J. Dunkley et al
2009
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2010
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2010
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2010
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2010
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2010
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2010
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2010
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2011
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