activity
20002025
most citedGRChombo: An adaptable numerical relativity code for fundamental physics

96 citations · 259 across the 10 of their papers we have counts for

collaborators

10 papers

gr-qc2025

MHDuet : a high-order General Relativistic Radiation MHD code for CPU and GPU architectures

Carlos Palenzuela, Miguel Bezares, Steven Liebling +12

We present MHDuet, an open source evolution code for general relativistic magnetohydrodynamics with neutrino transport. The code solves the full set of Einstein equations coupled t…

gr-qc2022★ 96 cited

GRChombo: An adaptable numerical relativity code for fundamental physics

Tomas Andrade, Llibert Areste Salo, Josu C. Aurrekoetxea +29

GRChombo is an open-source code for performing Numerical Relativity time evolutions, built on top of the publicly available Chombo software for the solution of PDEs. Whilst GRChomb…

physics.flu-dyn2015★ 2 cited

The decay of wall-bounded MHD turbulence at low Rm

Kacper Kornet, Alban Potherat

We present Direct Numerical Simulations of decaying Magnetohydrodynamic (MHD) turbulence at low magnetic Reynolds number. The domain considered is bounded by periodic boundary cond…

physics.flu-dyn2014★ 1 cited

Spectral Direct Numerical Simulations of low Rm MHD channel flows based on the least dissipative modes

Kacper Kornet, Alban Pothérat

We put forward a new type of spectral method for the direct numerical simulation of flows where anisotropy or very fine boundary layers are present. The mean idea is to take advant…

astro-ph2008★ 18 cited

PIERNIK mhd code - a multi-fluid, non-ideal extension of the relaxing-TVD scheme (II)

Michał Hanasz, Kacper Kowalik, Dominik Wóltański +2

We present a new multi-fluid, grid MHD code PIERNIK, which is based on the Relaxing TVD scheme (Jin and Xin, 1995). The original scheme (see Trac & Pen (2003) and Pen et al. (2003)…

astro-ph2006★ 40 cited

Formation of giant planets around stars with various masses

Kacper Kornet, Sebastian Wolf, Michal Rozyczka

We examine the predictions of the core accretion - gas capture model concerning the efficiency of planet formation around stars with various masses. First, we follow the evolution…