$\texttt{Hi-COLA}$: Fast, approximate simulations of structure formation in Horndeski gravity
Bill S. Wright, Ashim Sen Gupta, Tessa Baker, Georgios Valogiannis and, Bartolomeo Fiorini

TL;DR
Hi-COLA is a fast, adaptable simulation code for studying non-linear structure formation in various Horndeski gravity theories, enabling efficient exploration of modified gravity effects on cosmic structures.
Contribution
The paper introduces Hi-COLA, a general and efficient simulation tool for non-linear structure formation in Horndeski gravity, capable of handling different theories with screening mechanisms.
Findings
Validated against traditional N-body simulations with 2.5% accuracy.
First simulations of an extended shift-symmetric gravity theory.
Dissected contributions of background, growth, and fifth force to matter power spectrum.
Abstract
We introduce , a code designed to run fast, approximate -body simulations of non-linear structure formation in reduced Horndeski gravity. Given an input Lagrangian, dynamically constructs the appropriate field equations and consistently solves for the cosmological background, linear growth, and screened fifth force of that theory. Hence is a general, adaptable, and useful tool that allows the mildly non-linear regime of many Horndeski theories to be investigated for the first time, at low computational cost. In this work, we first describe the screening approximations and simulation setup of for theories with Vainshtein screening. We validate the code against traditional -body simulations for cubic Galileon gravity, finding agreement up to . To…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Geophysics and Gravity Measurements
