For Gaussian initial conditions, the matter bispectrum through one loop is the sum of the tree diagram and the four one-loop topologies , , , and .
The connected correlation of one fourth-order and two first-order density contrasts contracts a pair of inputs at the fourth-order vertex into a loop. For each choice of the fourth-order external field there are twelve Wick contractions. In one dimension,
For the one-dimensional cosmological density kernel, exactly. Its leading cutoff dependence is therefore proportional to .
The connected correlation of three second-order density contrasts forms a triangle of three linear power spectra. It has eight Wick contractions. In one dimension, with and the power at the evaluation time,
For the one-dimensional cosmological density kernel, its hard-loop integrand starts as .

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