The one-loop bispectrum of galaxies in redshift space from the Effective Field Theory of Large-Scale Structure

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Main Authors: D'Amico, Guido, Donath, Yaniv, Lewandowski, Matthew, Senatore, Leonardo, Zhang, Pierre
Format: Preprint
Published: 2022
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author D'Amico, Guido
Donath, Yaniv
Lewandowski, Matthew
Senatore, Leonardo
Zhang, Pierre
author_facet D'Amico, Guido
Donath, Yaniv
Lewandowski, Matthew
Senatore, Leonardo
Zhang, Pierre
contents We derive the kernels and the Effective Field Theory of Large-Scale Structure counterterms for the one-loop bispectrum of dark matter and of biased tracers in real and redshift space. This requires the expansion of biased tracers up to fourth order in fluctuations. In the process, we encounter several subtleties related to renormalization. One is the fact that, in renormalizing the momentum, a local counterterm contributes non-locally. A second subtlety is related to the renormalization of local products of the velocity fields, which need to be expressed in terms of the renormalized velocity in order to preserve Galilean symmetry. We check that the counterterms we identify are necessary and sufficient to renormalize the one-loop bispectrum at leading and subleading order in the derivative expansion. The kernels that we originally present here have already been used for the first analyses of the one-loop bispectrum in BOSS data [1, 2].
format Preprint
id arxiv_https___arxiv_org_abs_2211_17130
institution arXiv
publishDate 2022
record_format arxiv
spellingShingle The one-loop bispectrum of galaxies in redshift space from the Effective Field Theory of Large-Scale Structure
D'Amico, Guido
Donath, Yaniv
Lewandowski, Matthew
Senatore, Leonardo
Zhang, Pierre
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We derive the kernels and the Effective Field Theory of Large-Scale Structure counterterms for the one-loop bispectrum of dark matter and of biased tracers in real and redshift space. This requires the expansion of biased tracers up to fourth order in fluctuations. In the process, we encounter several subtleties related to renormalization. One is the fact that, in renormalizing the momentum, a local counterterm contributes non-locally. A second subtlety is related to the renormalization of local products of the velocity fields, which need to be expressed in terms of the renormalized velocity in order to preserve Galilean symmetry. We check that the counterterms we identify are necessary and sufficient to renormalize the one-loop bispectrum at leading and subleading order in the derivative expansion. The kernels that we originally present here have already been used for the first analyses of the one-loop bispectrum in BOSS data [1, 2].
title The one-loop bispectrum of galaxies in redshift space from the Effective Field Theory of Large-Scale Structure
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2211.17130