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Cosmological perturbation theory is a powerful tool to predict the statistics of large-scale structure in the weakly non-linear regime, but even at 1-loop order it results in computationally expensive mode-coupling integrals.
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2007
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J. Lazear, P. A. R. Ade, D. Benford, C. L. Bennett, D. T. Chuss, J. L. Dotson et al., The Primordial Inflation Polarization Explorer (PIPER) , in Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII , vol. 9153, p. 91531L, 2014 · 2014
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J. Blazek, Z. Vlah and U. Seljak, Tidal alignment of galaxies , JCAP 1508
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