code for cosmological gravitational wave backgrounds
Project description
CosmoGW v1.0
CosmoGW is a Python package for the analysis and modeling of cosmological gravitational wave (GW) backgrounds from different sources in the early Universe, including analytical models, templates, and data analysis routines.
v1.0 (August 2025) focuses on the production of GWs from sound waves and MHD turbulence from cosmological phase transitions.
Other sources of GWs will be included in future versions, contact me if you are interested in contributing and becoming a developer.
CosmoGW is an extension of GW_turbulence, created in December 2021, used for calculations of GWs produced by MHD turbulence.
Contact
Author: Alberto Roper Pol
Email: alberto.roperpol@unige.ch
GitHub: albertoroperpol
If you use any of the cosmoGW results, please cite this repository, the [manual] (coming soon) and the relevant references listed in the routines.
Feel free to reach out for questions, issues, or collaboration! I would also love to hear about your interest for this project and your work, so feel free to reach out for questions, issues, or collaboration!
Installation
CosmoGW is a Python package that can be installed using pip from PyPI:
pip install cosmoGW
Or directly from GitHub (last version but not necessarily stable):
pip install git+https://github.com/cosmoGW/cosmoGW.git
Requirements:
Python >= 3.8, numpy, scipy, matplotlib, astropy, pandas
To use the plotting routines available in the tutorials and in plot_sets, make sure to install latex for Python:
sudo apt install cm-super dvipng texlive-latex-extra texlive-latex-recommended
File Structure
The main routines of cosmoGW are stored under src/cosmoGW:
cosmology.py: Cosmological calculations.GW_analytical.py: Analytical calculations and mathematical functions.GW_back.py: Functions for cosmological GW backgrounds.GW_models.py: Theoretical and numerical models for sources of GWs.GW_templates.py: Templates for GW backgrounds from different sources.hydro_bubbles.py: Fluid perturbations from bubbles in first-order phase transitions.interferometry.py: Response and sensitivity functions for GW detectors (LISA, Taiji).utils.py: Utility functions and reference values for CosmoGW.tests/: Unit tests and example data.resources/: Data files used in the code (numerical data, sensitivity curves, ...)tutorials/: Tutorials showing how to use CosmoGW for different applications.
Documentation
Comprehensive documentation is available at Read the Docs.
- API Reference: Detailed documentation for all modules and functions.
- Tutorials: Step-by-step guides and example workflows.
- Theory: Background information and mathematical details.
To build the documentation locally:
cd docs
make html
Tutorials
Tutorials and example notebooks are available in the tutorials/ directory:
These tutorials can be run from Google Colab by loading the notebooks from GitHub.
When using Colab, latex needs to be installed, together with CosmoGW, for plotting routines. For the installation, uncomment and execute the first cell of the tutorials:
pip install cosmoGW
sudo apt-get update
sudo apt-get install -y cm-super dvipng texlive-latex-extra texlive-latex-recommended
Tests
Unit tests are provided in the tests/ directory.
To run all tests (from cosmoGW directory):
pytest
Make sure all required test data files are present in the tests directory.
Resources
Data files are available in cosmoGW that are required by some of the libraries.
They are stored in src/cosmoGW/resources:
cosmology: Cosmological evolution files and Friedmann equation tutorial.interferometry: Space-based GW interferometry calculations and tutorials.detector_sensitivity: Sensitivity of various detectors; see the README.higgsless: Data sets from Higgsless simulations of phase transitions.
📄 License
This project is licensed under the MIT License.
🚀 Enjoy exploring the early Universe with gravitational waves! 🪐
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