POWER CORRELATIONS IN COSMOLOGY - LIMITS ON PRIMORDIAL NON-GAUSSIAN DENSITY FIELDS

We probe the statistical nature of the primordial density field by mea suring correlations between the power in adjacent Fourier modes. For c ertain types of non-Gaussian field, these k-space correlations would b e expected to be more extended than for a Gaussian field, providing a useful discriminatory test for Gaussian fields. We apply this test to the combined QDOT and 1.2-Jy IRAS galaxy survey and find the observed density field to be in good agreement with having Gaussian density flu ctuations for modes with k less than or similar to 0.1 h Mpc(-1). From this result we are able to set quantitative limits on a class of poss ible non-Gaussian distributions - the product of a Gaussian field with an independent stochastic field. The maximum sensitivity is to modula tions of a Gaussian field with coherence scales of similar to 30 h(-1) Mpc, and the rms modulation on this scale cannot greatly exceed unity . We discuss the improvements to this limit likely to be set by future surveys.