4.6 Article

Estimators for local non-Gaussianities

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IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2007/03/019

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CMBR experiments; CMBR theory; cosmological perturbation theory

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We study the Likelihood function of data given f(NL) for the so-called local type of non-Gaussianity. In this case the curvature perturbation is a nonlinear function, local in real space, of a Gaussian random field. We compute the Cramer-Rao bound for f(NL) and show that for small values of f(NL) the three-point function estimator saturates the bound and is equivalent to calculating the full Likelihood of the data. However, for sufficiently large f(NL), the naive three-point function estimator has a much larger variance than previously thought. In the limit in which the departure from Gaussianity is detected with high confidence, error bars on f(NL) only decrease as 1/N-pix(2) rather than N-pix-1/2 as the size of the data set increases. We identify the physical origin of this behaviour and explain why it only affects the local type of non-Gaussianity, where the contribution of the first multipoles is always relevant. We find a simple improvement to the three-point function estimator that makes the square root of its variance decrease as N-pix(-1/2) even for large f(NL), asymptotically approaching the Cramer-Rao bound. We show that using the modified estimator is practically equivalent to computing the full Likelihood of f(NL) given the data. Thus other statistics of the data, such as the four-point function and Minkowski functionals, contain no additional information on f(NL). In particular, we explicitly show that the recent claims about the relevance of the four-point function are not correct. By direct inspection of the Likelihood, we show that the data do not contain enough information for

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