The art of simulating the early Universe. Part II. Non-canonical cases & gravitational waves
Jorge Baeza-Ballesteros, Daniel G. Figueroa, Adrien Florio, Joanes Lizarraga, Nicol\'as Loayza, Kenneth Marschall, Toby Opferkuch, Ben A. Stefanek, Francisco Torrent\'i, Ander Urio

TL;DR
This paper extends lattice simulation techniques to non-canonical field theories and gravitational wave dynamics, providing a comprehensive framework for modeling complex early Universe phenomena with new interactions and configurations.
Contribution
It introduces lattice implementations for non-canonical interactions, initial condition setups, and gravitational wave dynamics, expanding simulation capabilities beyond canonical models.
Findings
Developed methods for simulating non-minimal scalar-gravity couplings
Implemented lattice techniques for axion-like particle interactions
Extended scalar field discretization to arbitrary spatial dimensions
Abstract
We present a discussion on lattice techniques for the simulation of non-canonical field theory circumstances, complementing our previous monograph (arXiv:2006.15122) on canonical cases. We begin by reviewing basic aspects of lattice field theory, including symplectic and non-symplectic evolution algorithms. We then introduce lattice implementations of non-canonical interactions, considering scalars with a non-minimal coupling to gravity, , non-minimal scalar kinetic theories, , and axion-like particle (ALP) interactions with Abelian gauge fields, . Next, we discuss methods to set up special field configurations, including the creation of cosmic defect networks towards scaling (e.g. cosmic strings and domain walls), field configurations based on arbitrary power spectra…
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Taxonomy
TopicsCosmology and Gravitation Theories · Particle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions
