The 2-loop matter power spectrum and the IR-safe integrand
John Joseph M. Carrasco, Simon Foreman, Daniel Green, and Leonardo, Senatore

TL;DR
This paper introduces a new IR-safe method for computing the 2-loop matter power spectrum in the Effective Field Theory of Large Scale Structures, improving numerical stability and accuracy for cosmological predictions.
Contribution
The authors develop a novel technique to compute all 2-loop diagrams as a single IR-divergence-free integral, simplifying calculations and enhancing reliability.
Findings
Method produces IR-safe, cutoff-independent results
Applicable to scaling universes with power-law spectra
Method generalizes to higher-loop computations
Abstract
Large scale structure surveys are likely the next leading probe of cosmological information. It is therefore crucial to reliably predict their observables. The Effective Field Theory of Large Scale Structures (EFTofLSS) provides a manifestly convergent perturbation theory for the weakly non-linear regime, where dark matter correlation functions are computed in an expansion of the wavenumber k over the wavenumber associated to the non-linear scale knl. To push the predictions to higher wavenumbers, it is necessary to compute the 2-loop matter power spectrum. For equal-time correlators, exactly as with standard perturturbation theory, there are IR divergences present in each diagram that cancel completely in the final result. We develop a method by which all 2-loop diagrams are computed as one integral, with an integrand that is manifestly free of any IR divergences. This allows us to…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
