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[ascl:2306.039]
GRChombo: Numerical relativity simulator

Andrade, Tomas; Salo, Llibert; Aurrekoetxea, Josu; Bamber, Jamie; Clough, Katy; Croft, Robin; de Jong, Eloy; Drew, Amelia; Duran, Alejandro; Ferreira, Pedro; Figueras, Pau; Finkel, Hal; França, Tiago; Ge, Bo-Xuan; Gu, Chenxia; Helfer, Thomas; Jäykkä, Juha; Joana, Cristian; Kunesch, Markus; Kornet, Kacper; Lim, Eugene; Muia, Francesco; Nazari, Zainab; Radia, Miren; Ripley, Justin; Shellard, Paul; Sperhake, Ulrich; Traykova, Dina; Tunyasuvunakool, Saran; Wang, Zipeng; Widdicombe, James; Wong, Kaze

GRChombo performs numerical relativity simulations. It uses Chombo (ascl:1202.008) for adaptive mesh refinement and can evolve standard spacetimes such as binary black hole mergers and scalar collapses into black holes. The code supports non-trivial *many-boxes-in-many-boxes* mesh hierarchies and massive parallelism and evolves the Einstein equation using the standard BSSN formalism. GRChombo is written in C++14 and uses hybrid MPI/OpenMP parallelism and vector intrinsics to achieve good performance.

[ascl:2312.014]
GRFolres: Extension to GRChombo for modified gravity simulations

Aresté Saló, Llibert; Brady, Sam E.; Clough, Katy; Doneva, Daniela; Evstafyeva, Tamara; Figueras, Pau; França, Tiago; Rossi, Lorenzo; Yao, Shunhui; Andrade, Tomas; Aurrekoetxea, Josu; Bamber, Jamie; Croft, Robin; de Jong, Eloy; Drew, Amelia; Duran, Alejandro; Ferreira, Pedro; Finkel, Hal; Ge, Bo-Xuan; Gu, Chenxia; Helfer, Thomas; Jäykkä, Juha; Joana, Cristian; Kunesch, Markus; Kornet, Kacper; Lim, Eugene; Muia, Francesco; Nazari, Zainab; Radia, Miren; Ripley, Justin; Shellard, Paul; Sperhake, Ulrich; Traykova, Dina; Tunyasuvunakool, Saran; Wang, Zipeng; Widdicombe, James; Wong, Kaze

GRFolres performs simulations in modified theories of gravity. It is based on GRChombo (ascl:2306.039) and inherits all of the capabilities of the main GRChombo code, which makes use of the Chombo library (ascl:1202.008) for adaptive mesh refinement. The code implements the 4∂ST theory of modified gravity and the cubic Horndeski theory in (3+1)-dimensional numerical relativity. GRFolres can be used for stable gauge evolution, solving the modified energy and momentum constraints for initial conditions, and monitoring the constraint violation and calculating the energy densities associated with the different scalar terms in the action. It can also extract data for the tensor and scalar gravitational waveforms.