BEoRN 1.1.0

Add your description here

BEoRN: Bubbles during the Epoch Of Reionization Numerical-simulator

BEoRN is a simulation tool designed to model the state of the intergalactic medium (IGM) during cosmic dawn and reionization (Schaeffer, Giri & Schneider 2023). It leverages one-dimensional radiative transfer calculations to efficiently model the temperature evolution of intergalactic gas and growth of ionized regions (bubbles) around early galaxies embedded in dark matter halos (e.g., Schneider, Giri & Mirocha 2021; Schneider, Schaeffer & Giri 2023).

BEoRN is designed to be flexible, user-friendly, and fast, allowing researchers to efficiently explore various astrophysical scenarios and their impact on the 21-cm signal from neutral hydrogen.

BEoRN is actively developed. We welcome feedback and contributions. If you encounter any issues, please inform the developers by opening a GitHub issue.

Key Features

• 📦 Lightweight & Modular: A Python package suitable for simulation modules and analysis tools.
• 📊 Data Visualization: Utilities for assembling time/coeval cube data for easy visualization.
• 🔄 Reproducible: Testing and CI-ready structure to support reproducible development.
• 🌌 Flexible Inputs: Natively reads halo catalogs from simulations such as Thesan and PkdGrav, or generates synthetic catalogs on the fly relying on 21cmFAST.

Documentation

Full documentation is available at: https://cosmic-reionization.github.io/BEoRN

Installation

Standard Installation

You can install BEoRN directly from GitHub using pip:

pip install git+https://github.com/cosmic-reionization/beorn.git

With Optional Dependencies

The extra option installs additional packages needed for generating synthetic halo catalogs with 21cmFAST and for comparing halo mass functions against analytical models (hmf):

pip install "git+https://github.com/cosmic-reionization/beorn.git[extra]"

Note: If 21cmFAST installation fails, please refer to the 21cmFAST repository and install it manually first, then install BEoRN without the extra option.

Development Installation

For a local, editable installation (useful if you want to modify the code):

1. Clone the repository:

git clone https://github.com/cosmic-reionization/beorn.git
cd beorn

2. Install in editable mode:

pip install -e .

To also install the optional dependencies:

pip install -e ".[extra]"

Dependencies

The dependencies are listed in pyproject.toml. The core dependencies include numpy, scipy, h5py, mpi4py, astropy, matplotlib, pylians, and tools21cm.

⚠️ Note on pylians: This package may sometimes fail during automatic installation of dependencies. If you encounter issues, we recommend installing pylians separately before installing BEoRN.

Project Layout

• src/beorn/: Package source code.
• docs/: Documentation source.
• examples/: Runnable examples and Jupyter notebooks to get started quickly.

Note: This repository focuses on code and workflows. Heavy simulation outputs (coeval/temporal cubes, large data products) are expected to be stored externally due to size.

📖 Citation

If you use this package in your research, please consider citing the following paper:

@article{Schaeffer_2023,
    title={beorn: a fast and flexible framework to simulate the epoch of reionization and cosmic dawn},
    volume={526},
    ISSN={1365-2966},
    url={[http://dx.doi.org/10.1093/mnras/stad2937](http://dx.doi.org/10.1093/mnras/stad2937)},
    DOI={10.1093/mnras/stad2937},
    number={2},
    journal={Monthly Notices of the Royal Astronomical Society},
    publisher={Oxford University Press (OUP)},
    author={Schaeffer, Timothée and Giri, Sambit K and Schneider, Aurel},
    year={2023},
    month=sep,
    pages={2942–2959}
}

👨‍💻 Authors

• Sambit Giri - GitHub
• Rémy Moll - GitHub
• Timothée Schaeffer - GitHub
• Aurel Schneider - GitHub

Contributing

Contributions are welcome! If you find bugs or unexpected behavior, please open a Github issue. For detailed guidelines on contributing code or setting up a development environment, please see CONTRIBUTING.rst.

License

This project is licensed under the MIT License - see the LICENSE file for details.