Precision calculation of the EFT likelihood with primordial non-Gaussianities

Abstract We perform a precision calculation of the effective field theory (EFT) conditional likelihood for large-scale structure (LSS) using the saddle-point expansion method in the presence of primordial non-Gaussianities (PNG). The precision is manifested at two levels: one corresponding to the consideration of higher-order noise terms, and the other to the inclusion of contributions from the saddle-point fluctuations. When computing the latter, we encounter the same issue of the negative modes as in the context of false vacuum decay, which necessitates deforming the original integration contour into a combination of the steepest descent contours to ensure a convergent and real result. We demonstrate through detailed calculations that, upon incorporating leading-order PNG, both types of extensions introduce irreducible field-dependent contributions to the conditional likelihood. This insight motivates the systematic inclusion of additional effective terms within the forward modeling framework. Our work facilitates Bayesian forward modeling under non-Gaussian initial conditions, thereby enabling more stringent constraints on the parameters describing PNG.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-09-01
DOI
https://doi.org/10.1088/1475-7516/2025/09/029
Citations
1
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
1.15
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article

Precision calculation of the EFT likelihood with primordial non-Gaussianities

Yun Wang, Ping He, Ji-Yuan Ke
1 citations
Journal of Cosmology and Astroparticle Physics
Galaxies: Formation, Evolution, Phenomena
1.15
article

Precision calculation of the EFT likelihood with primordial non-Gaussianities

Yun Wang, Ping He, Ji-Yuan Ke
article en
1 citations

Abstract

Abstract We perform a precision calculation of the effective field theory (EFT) conditional likelihood for large-scale structure (LSS) using the saddle-point expansion method in the presence of primordial non-Gaussianities (PNG). The precision is manifested at two levels: one corresponding to the consideration of higher-order noise terms, and the other to the inclusion of contributions from the saddle-point fluctuations. When computing the latter, we encounter the same issue of the negative modes as in the context of false vacuum decay, which necessitates deforming the original integration contour into a combination of the steepest descent contours to ensure a convergent and real result. We demonstrate through detailed calculations that, upon incorporating leading-order PNG, both types of extensions introduce irreducible field-dependent contributions to the conditional likelihood. This insight motivates the systematic inclusion of additional effective terms within the forward modeling framework. Our work facilitates Bayesian forward modeling under non-Gaussian initial conditions, thereby enabling more stringent constraints on the parameters describing PNG.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(09)
Jilin University (CN), Peking University (CN)
Openalex Percentile: Top 17%
Galaxies: Formation, Evolution, Phenomena
1.15
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