Past exam of the mathematics course of the University of Cambridge 2019 iii Paper 312 2 i Solution Created 2026-10-03 Updated 2026-10-14
Use the one-loop matter power spectrum convention in which is one ordering of . Thenwith the P22 contribution to the one-loop matter power spectrumand the P13 contribution to the one-loop matter power spectrumThe factors two and three count Wick contractions. The mixed contains an odd number of zero-mean Gaussian fields, so .
One-loop contributions to the matter power spectrum
. The two one-loop power-spectrum topologies. Solid lines attach external density fields to kernels; dashed lines pair linear fields and carry a linear power spectrum. The P13 topology has two external orderings. Details.For , the ultraviolet softness of the second-order density kernel gives , soThe third-order kernel has , givingThese integrals expose the sensitivity to unresolved short-scale dynamics. The effective sound-speed counterterm in large-scale structure has exactly the required deterministic shape:Here absorbs the time and normalization conventions and has dimensions of length squared. A stochastic correction begins at and can absorb the corresponding short-scale sensitivity of .
Past exam of the mathematics course of the University of Cambridge 2021 iii Paper 312 3 c Solution 2026-09-28
The effective field theory of large-scale structure supplements the one-loop prediction by the leading deterministic counterterm and a stochastic term,where the normalization scale may be absorbed into and mass and momentum conservation make at small . The ultraviolet part of the P13 contribution to the one-loop matter power spectrum hasIts cutoff dependence has exactly the form of the effective sound-speed counterterm in large-scale structure, so the running of cancels it. The stochastic and higher-derivative counterterms similarly absorb the allowed analytic ultraviolet dependence of and higher orders.
For internal momentum , the P22 contribution to the one-loop matter power spectrum starts at , while twice the P13 contribution to the one-loop matter power spectrum starts at . The latter has the same momentum dependence as the effective sound-speed counterterm in large-scale structure. Short-scale stochastic contributions start at by mass and momentum conservation.
