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README.md

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<img src="docs/source/figures/wallgo.svg" alt="WallGoLogo" width="200"/>
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<img src="https://raw.githubusercontent.com/Wall-Go/WallGo/refs/heads/main/docs/source/figures/wallgo.svg" alt="WallGoLogo" width="200"/>
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# WallGo
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## About this project
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[**WallGo**](https://wallgo.readthedocs.io) is an open source code for the computation of the bubble wall velocity and bubble wall width in first-order cosmological phase transitions.
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The main WallGo Python package determines the wall velocity and width by solving the scalar field(s) equation of motion, the Boltzmann equations and energy-momentum conservation for the fluid velocity and temperature.
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The main WallGo Python package determines the wall velocity and width by solving the scalar field(s) equation of motion, the Boltzmann equations and energy-momentum conservation for the fluid velocity and temperature. The physical and mathematical details are explained in [the associated paper](https://arxiv.org/abs/2411.04970).
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The [**WallGo**](https://github.com/Wall-Go/WallGo) package is accompanied by two subsidiary software packages:
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- [**WallGoCollision**](https://github.com/Wall-Go/WallGoCollision) performs the higher-dimensional integrals to obtain the collision terms in the Boltzmann equations, and is written in C++. It also has Python bindings so that it can be called directly from Python, but still benefits from the speedup from compiled C++ code.

docs/source/faqs.rst

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- **How should I cite WallGo?**
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WallGo is free and open source, but if you use WallGo in your work, we ask that you
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support us by please citing the WallGo paper, `arXiv:2410.00000 <https://arxiv.org/abs/2410.00000>`_.
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support us by please citing the WallGo paper, `arXiv:2411.04970 <https://arxiv.org/abs/2411.04970>`_. The complete BibTex citation from `Inspire <https://inspirehep.net/literature/2846423>`_ is::
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@article{Ekstedt:2024fyq,
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author = "Ekstedt, Andreas and Gould, Oliver and Hirvonen, Joonas and Laurent, Benoit and Niemi, Lauri and Schicho, Philipp and van de Vis, Jorinde",
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title = "{How fast does the WallGo? A package for computing wall velocities in first-order phase transitions}",
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eprint = "2411.04970",
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archivePrefix = "arXiv",
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primaryClass = "hep-ph",
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reportNumber = "CERN-TH-2024-174, DESY-24-162, HIP-2024-21/TH",
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month = "11",
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year = "2024"
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}
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Installation
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============

docs/source/index.rst

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WallGo documentation
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======================================
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WallGo is an open source code for the computation of the bubble wall velocity and bubble wall width in first-order cosmological phase transitions. If you use WallGo, please cite arXiv:....
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WallGo is an open source code for the computation of the bubble wall velocity and bubble wall width in first-order cosmological phase transitions. If you use WallGo, please cite the WallGo paper `arXiv:2411.04970 <https://arxiv.org/abs/2411.04970>`_. :footcite:p:`Ekstedt:2024fyq`
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As the universe cooled after the Hot Big Bang, it may have gone through any number of cosmological first-order phase transitions. Such transitions proceed via the nucleation and growth of bubbles, as shown in the image below. :footcite:p:`Weir_2016` The collisions of these bubbles may lead to an observable gravitational wave signal today, depending on the speed of the bubble walls as they collide.
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docs/source/refs.bib

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pages = "096015",
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year = "2021"
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}
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@article{Ekstedt:2024fyq,
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author = "Ekstedt, Andreas and Gould, Oliver and Hirvonen, Joonas and Laurent, Benoit and Niemi, Lauri and Schicho, Philipp and van de Vis, Jorinde",
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title = "{How fast does the WallGo? A package for computing wall velocities in first-order phase transitions}",
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eprint = "2411.04970",
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archivePrefix = "arXiv",
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primaryClass = "hep-ph",
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reportNumber = "CERN-TH-2024-174, DESY-24-162, HIP-2024-21/TH",
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month = "11",
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year = "2024",
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journal = "arXiv"
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}

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