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KAClough merged 2 commits into from
May 5, 2026
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Final paper edits #37

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Update paper.bib
JCAurre May 4, 2026
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Update paper.md
JCAurre May 4, 2026
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2 changes: 1 addition & 1 deletion paper/paper.bib
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Expand Up @@ -192,7 +192,7 @@ @article{Aurrekoetxea:2024cqd
}

@article{Andrade:2021rbd,
author = {Andrade, Tomas and Areste-Salo, Llibert and Aurrekoetxea, Josu C. and Bamber, Jamie and Clough, Katy and Croft, Robin and de Jong, Eloy and Drew, Amelia and Duran, Alejandro and Ferreira, Pedro G. and Figueras, Pau and Finkel, Hal and Fran\c{c}a, Tiago and Ge, Bo-Xuan and Gu, Chenxia and Helfer, Thomas and Jäykkä, Juha and Joana, Cristian and Kunesch, Markus and Kornet, Kacper and Lim, Eugene A. and Muia, Francesco and Nazari, Zainab and Radia, Miren and Ripley, Justin and Shellard, Paul and Sperhake, Ulrich and Traykova, Dina and Tunyasuvunakool, Saran and Wang, Zipeng and Widdicombe, James Y. and Wong, Kaze},
author = {Andrade, Tomas and Arest\'e Sal\'o, Llibert and Aurrekoetxea, Josu C. and Bamber, Jamie and Clough, Katy and Croft, Robin and de Jong, Eloy and Drew, Amelia and Duran, Alejandro and Ferreira, Pedro G. and Figueras, Pau and Finkel, Hal and Fran\c{c}a, Tiago and Ge, Bo-Xuan and Gu, Chenxia and Helfer, Thomas and Jäykkä, Juha and Joana, Cristian and Kunesch, Markus and Kornet, Kacper and Lim, Eugene A. and Muia, Francesco and Nazari, Zainab and Radia, Miren and Ripley, Justin and Shellard, Paul and Sperhake, Ulrich and Traykova, Dina and Tunyasuvunakool, Saran and Wang, Zipeng and Widdicombe, James Y. and Wong, Kaze},
title = "{GRChombo: An adaptable numerical relativity code for fundamental physics}",
eprint = "2201.03458",
archivePrefix = "arXiv",
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2 changes: 1 addition & 1 deletion paper/paper.md
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Expand Up @@ -108,7 +108,7 @@ The key features of GRTresna are as follows.

- Methods: GRTresna incorporates the CTTK and CTTK-Hybrid methods to solve the Hamiltonian and momentum constraints. These methods offer several advantages when dealing with fundamental fields, as discussed in @Aurrekoetxea:2022mpw. The method code is also templated, so users can easily implement their preferred methods.

- Initial conditions: The code supports analytical initial data for the matter fields, as well as the option to read grids and data from an existing HDF5 file. This functionality is especially useful when combined with our code that evolves matter on fixed metric backgrounds GRDzhadzha [@Aurrekoetxea:2023fhl], meaning that we can upgrade the resulting matter configurations to full NR simulations with backreaction.
- Initial conditions: The code supports analytical initial data for the matter fields, as well as the option to read grids and data from an existing HDF5 file. This functionality is especially useful when combined with our GRDzhadzha code [@Aurrekoetxea:2023fhl], which evolves matter on fixed metric backgrounds, meaning that we can upgrade the resulting matter configurations to full NR simulations with backreaction.

- Boundary conditions: The code implements extrapolating, reflective, and periodic boundary conditions, compatible with those in the NR evolution code GRChombo [@Andrade:2021rbd;@Clough:2015sqa].

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