On the correction of conserved variables for numerical RMHD with staggered constrained transport
Jos\'e M. Mart\'i

TL;DR
This paper evaluates correction algorithms for conserved variables in numerical relativistic magnetohydrodynamics, demonstrating that relativistic correction methods significantly improve accuracy and robustness in highly magnetized flow simulations.
Contribution
It introduces and compares non-relativistic and relativistic correction algorithms, showing the superiority of relativistic approaches in highly magnetized relativistic flows.
Findings
Relativistic correction algorithms pass high-magnetization tests successfully.
Non-relativistic corrections fail to pass the test at any resolution.
The CA2' algorithm is robust across all tested resolutions.
Abstract
Despite the success of the combination of conservative schemes and staggered constrained transport algorithms in the last fifteen years, the accurate description of highly magnetized, relativistic flows with strong shocks represents still a challenge in numerical RMHD. The present paper focusses in the accuracy and robustness of several correction algorithms for the conserved variables, which has become a crucial ingredient in the numerical simulation of problems where the magnetic pressure dominates over the thermal pressure by more than two orders of magnitude. Two versions of non-relativistic and fully relativistic corrections have been tested and compared using a magnetized cylindrical explosion with high magnetization () as test. In the non-relativistic corrections, the total energy is corrected for the difference in the classical magnetic energy term between the…
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