Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
Zhenyuan Wang, Donghui Jeong, Atsushi Taruya, Takahiro Nishimichi, Ken, Osato

TL;DR
This paper introduces a new perturbation theory scheme that accurately models the nonlinear density field, outperforming standard methods and matching simulation results across various cosmologies without free parameters.
Contribution
The paper proposes the $n$EPT scheme, a novel analytical approach that improves nonlinear density modeling beyond standard perturbation theory with high accuracy.
Findings
Excellent agreement with N-body simulations across cosmologies
Outperforms two-loop Standard Perturbation Theory
Extends reliable modeling to higher wavenumbers at high redshift
Abstract
We present a novel EPT (th-order Eulerian Perturbation Theory) scheme to model the nonlinear density field by the summation up to 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 -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 at 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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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
