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Added arXiv links (#356)
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og113 authored Nov 13, 2024
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4 changes: 2 additions & 2 deletions README.md
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<img src="docs/source/figures/wallgo.svg" alt="WallGoLogo" width="200"/>
<img src="https://raw.githubusercontent.com/Wall-Go/WallGo/refs/heads/main/docs/source/figures/wallgo.svg" alt="WallGoLogo" width="200"/>


# WallGo
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## About this project

[**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.
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 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).

The [**WallGo**](https://github.com/Wall-Go/WallGo) package is accompanied by two subsidiary software packages:
- [**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.
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14 changes: 13 additions & 1 deletion docs/source/faqs.rst
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- **How should I cite WallGo?**

WallGo is free and open source, but if you use WallGo in your work, we ask that you
support us by please citing the WallGo paper, `arXiv:2410.00000 <https://arxiv.org/abs/2410.00000>`_.
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::

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


Installation
============
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WallGo documentation
======================================

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:....
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`

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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12 changes: 12 additions & 0 deletions docs/source/refs.bib
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pages = "096015",
year = "2021"
}

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

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