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arxiv: 1009.1979 · v1 · pith:P55MPRA7new · submitted 2010-09-10 · 🌌 astro-ph.CO · gr-qc· hep-ph· hep-th

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

classification 🌌 astro-ph.CO gr-qchep-phhep-th
keywords localmodelslargenon-gaussianityclassificationlocal-typeclassifyrelations
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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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