The bispectrum in Lagrangian perturbation theory

Abstract We study the bispectrum in Lagrangian perturbation theory. Extending past results for the power spectrum, we describe a method to efficiently compute the bispectrum in LPT, focusing on the Zeldovich approximation, in which contributions due to linear displacements are captured to all orders in a manifestly infrared (IR) safe way. We then isolate the effects of these linear displacements on oscillatory components of the power spectrum like baryon acoustic oscillations or inflationary primordial features and show that the Eulerian perturbation theory (EPT) prescription wherein their effects are resummed by a Gaussian damping of the oscillations arise as a saddle-point approximation of our calculation. These two methods of IR resummation are in excellent agreement at 1-loop in the bispectrum. At tree level, resummed EPT does less well to capture the nonlinear damping of the oscillations, and the LPT calculation does not require an artificial split of the power spectrum into smooth and oscillatory components, making the latter particularly useful for modeling exotic features. We finish by extending our analysis of IR resummation in LPT to N-point functions of arbitrary order.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2024-11-01
DOI
https://doi.org/10.1088/1475-7516/2024/11/012
Citations
9
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.98
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article

The bispectrum in Lagrangian perturbation theory

Shi-Fan Chen, Zvonimir Vlah, Martin White
9 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
2.98
article

The bispectrum in Lagrangian perturbation theory

Shi-Fan Chen, Zvonimir Vlah, Martin White
article en
9 citations

Abstract

Abstract We study the bispectrum in Lagrangian perturbation theory. Extending past results for the power spectrum, we describe a method to efficiently compute the bispectrum in LPT, focusing on the Zeldovich approximation, in which contributions due to linear displacements are captured to all orders in a manifestly infrared (IR) safe way. We then isolate the effects of these linear displacements on oscillatory components of the power spectrum like baryon acoustic oscillations or inflationary primordial features and show that the Eulerian perturbation theory (EPT) prescription wherein their effects are resummed by a Gaussian damping of the oscillations arise as a saddle-point approximation of our calculation. These two methods of IR resummation are in excellent agreement at 1-loop in the bispectrum. At tree level, resummed EPT does less well to capture the nonlinear damping of the oscillations, and the LPT calculation does not require an artificial split of the power spectrum into smooth and oscillatory components, making the latter particularly useful for modeling exotic features. We finish by extending our analysis of IR resummation in LPT to N-point functions of arbitrary order.

Journal of Cosmology and Astroparticle PhysicsVol. 2024(11)
Wilberforce University (US), University of Cambridge (GB), Institute for Advanced Study (US), Ruđer Bošković Institute (HR), University of California, Berkeley (US)
Openalex Percentile: Top 9%
Cosmology and Gravitation Theories
2.98
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