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On Classification of Models of Large Local-Type Non-Gaussianity

Published 10 Sep 2010 in astro-ph.CO, gr-qc, hep-ph, and hep-th | (1009.1979v1)

Abstract: We classify models generating large local-type non-Gaussianity into some categories by using some "consistency relations" among the non-linearity parameters f_{NL}{local}, \tau_{NL}{local} and g_{NL}{local}, which characterize the size of bispectrum for the former and trispectrum for the later two. Then we discuss how one can discriminate models of large local-type non-Gaussianity with such relations. We first classify the models by using the ratio of \tau_{NL}{local}/(6f_{NL}{local}/5)2, which is unity for "single-source" models and deviates from unity for "multi-source" ones. We can make a further classification of models in each category by utilizing the relation between f_{NL}{local} and g_{NL}{local}. Our classification suggests that observations of trispectrum would be very helpful to distinguish models of large non-Gaussianity and may reveal the generation mechanism of primordial fluctuations.

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