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Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory

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arxiv 2309.10133 v2 pith:UW2LQ6XJ submitted 2023-09-18 astro-ph.CO hep-phhep-th

Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory

classification astro-ph.CO hep-phhep-th
keywords forestalphadataexpansionexponentialfieldlymanmodel
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We derive an effective field theory (EFT) for cosmological Lyman alpha forest fluctuations valid for the power spectrum at the one-loop order. The ``bottom-up'' EFT expansion at the level of the transmitted flux is identical to the line-of-sight dependent bias model first derived by Desjacques et al. We confirm this result by a ``top-down'' derivation based on the exponential map of the optical depth field. Specifically, we show that the combination of the exponential map and conditions of renormalizability generates the same EFT expansion as the ``bottom-up'' approach. In passing, we point out inconsistencies of the tree-level perturbative expansion of the exponential map without counterterms. To facilitate practical applications, we generalize the FFTLog method for efficient calculations of one-loop integrals from new line-of-sight dependent operators. Finally, we compare the one-loop EFT model against data from the Sherwood hydrodynamic simulation. The theory fits the data with sub percent accuracy up to $k= $ 3 $h$Mpc$^{-1}$ at $z= 2.8$ for both 3D and 1D correlations. Our model can be readily used for cosmological full-shape analyses of Lyman alpha forest data.

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Forward citations

Cited by 14 Pith papers

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

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