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Halo/Galaxy Bispectrum with Equilateral-type Primordial Trispectrum · Around

2015

Halo/Galaxy Bispectrum with Equilateral-type Primordial Trispectrum

Mizuno, Shuntaro, Yokoyama, Shuichiro

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We investigate the effect of equilateral-type primordial trispectrum on the halo/galaxy bispectrum.

We consider three types of equilateral primordial trispectra which are generated by quartic operators naturally appeared in the effective field theory of inflation and can be characterized by three non-linearity parameters, $g_{\rm NL} ^{\dot{\sigma}^4}$, $g_{\rm NL} ^{\dot{\sigma}^2 (\partial \sigma)^2}$, and $g_{\rm NL} ^{(\partial \sigma)^4}$.
Recently, constraints on these parameters have been investigated from CMB observations by using WMAP9 data.
In order to consider the halo/galaxy bispectrum with the equilateral-type primordial trispectra, we adopt the integrated Perturbation Theory (iPT) in which the effects of primordial non-Gaussianity are wholly encapsulated in the linear primordial polyspectrum for the evaluation of the biased polyspectrum.

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