4.6 Article

Signatures of non-Gaussianity in the curvaton model

出版社

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2008/09/012

关键词

cosmological perturbation theory; cosmology of theories beyond the SM; physics of the early universe

资金

  1. Scientific Research from the Ministry of Education, Science, Sports, and Culture of Japan [19740145 (TT)]
  2. Academy of Finland Finnish-Japanese Core Programme [112420]
  3. Academy of Finland (AKA) [112420, 112420] Funding Source: Academy of Finland (AKA)

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We discuss the signatures of non-Gaussianity in the curvaton model where the potential includes also a non-quadratic term. In such a case the non-linearity parameter f(NL) can become very small, and we show that non-Gaussianity is then encoded in the non-reducible non-linearity parameter gNL of the trispectrum, which can be very large. Thus the place to look for the non-Gaussianity in the curvaton model may be the trispectrum rather than the bispectrum. We also show that gNL measures directly the deviation of the curvaton potential from the purely quadratic form. While gNL depends on the strength of the non-quadratic terms relative to the quadratic one, we find that for reasonable cases roughly gNL similar to O(-10(4))-O(-10(5)), which are values that may well be accessible by future observations.

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