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Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory

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arxiv 2209.00033 v1 pith:C4QF4DIS submitted 2022-08-31 astro-ph.CO

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keywords perturbationtheorydensityagreementdarkfieldmodelingstandard
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abstract

We present a novel $n$EPT ($n$th-order Eulerian Perturbation Theory) scheme to model the nonlinear density field by the summation up to $n$th-order density fields in perturbation theory. The obtained analytical power spectrum shows excellent agreement with the results from all 20 Dark-Quest suites of $N$-body simulations spreading over a broad range of cosmologies. The agreement is much better than the conventional two-loop Standard Perturbation Theory and would reach out to $k_{\rm max}\simeq 0.4~h/{\rm Mpc}$ at $z=3$ for the best-fitting Planck cosmology, without any free parameters. The method can accelerate the forward modeling of the non-linear cosmological density field, an indispensable probe of cosmic mysteries such as inflation, dark energy, and dark matter.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation

    astro-ph.CO 2025-04 conditional novelty 7.0 of 10

    Closed-form analytic covariance templates for the 2, 3, and 4 point galaxy correlation functions, built from a 1/k power-law power spectrum, reproduce Boltzmann-code results at percent level and trace sparsity to clos...

  2. Renormalized Perturbation Theory at Field-level: the LSS bootstrap in GridSPT

    astro-ph.CO 2025-06 conditional novelty 6.0 of 10

    A renormalized field-level perturbation theory is shown to recover the LSS bootstrap parameter consistently across different grid cutoffs, validated at third and fifth order against N-body simulations.

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