A User-Friendly Dark Energy Model Generator
Kyle A. Hinton, Adam Becker, Dragan Huterer

TL;DR
This paper introduces a user-friendly software tool with a graphical interface that enables researchers to simulate and analyze a broad range of dark energy models involving multiple scalar fields, facilitating easier exploration of their cosmological implications.
Contribution
The paper presents a novel software with GUI for calculating dark energy model phenomenology, supporting model selection, initial conditions, and Monte Carlo parameter scans.
Findings
Supports multiple scalar field models
Calculates energy density, equation of state, and perturbation growth
Provides outputs in various parametrizations
Abstract
We provide software with a graphical user interface to calculate the phenomenology of a wide class of dark energy models featuring multiple scalar fields. The user chooses a subclass of models and, if desired, initial conditions, or else a range of initial parameters for Monte Carlo. The code calculates the energy density of components in the universe, the equation of state of dark energy, and the linear growth of density perturbations, all as a function of redshift and scale factor. The output also includes an approximate conversion into the average equation of state, as well as the common parametrization. The code is available here: http://github.com/kahinton/Dark-Energy-UI-and-MC
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Astronomy and Astrophysical Research
