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
  • Additional Dependencies
• Tutorials
  • BEoRN: Quick-start with Artificial Halos
  • BEoRN: Modelling the 21-cm Signal from the Epoch of Reionization
  • 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
  • Parameters
  • Data Structures
  • Input data
  • Precomputations
  • Painting
  • IO
  • Plotting
• Citing This Package
• Contributing
  • Bug reports/Feedback/Questions
  • Adding new features
• Authors
• Changelog
  • v2.1.0
  • v1.2.0
  • v1.1.0
  • v0.1.0

Indices and tables

• Index

• Module Index