BEoRN#
Bubbles during Epoch Of Reionization Numerical-simulator (BEoRN) package provides tools to simulate the state of the intergalactic medium (IGM) during cosmic dawn and reionization. It leverages semi-numerical methods to efficiently model the growth of ionized regions (bubbles) around early galaxies embedded in dark matter halos.
BEoRN is designed to be flexible, user-friendly, and fast. It allows researchers to efficiently explore various astrophysical scenarios and their impact on the 21-cm signal from neutral hydrogen.
Contents:
- Installation
- Algorithm and Parallelisation
- Tutorials
- BEoRN: Quick-start with Artificial Halos
- BEoRN: Modelling the 21-cm Signal by post-processing 21cmFAST density (LPT) and haloes (CHMF)
- BEoRN: Post-processing (PKDGRAV3) N-body Simulation Data
- BEoRN: Exploring (THESAN) N-body Data
- BEoRN: Post-processing with Merger Trees
- Full run example
- Comparing two simulations side-by-side
- Module Reference
- Citing This Package
- Contributing
- Authors
- Changelog