Magnetohydrodynamics of rotating compact stars with spectral methods: description of the algorithm and tests

DOI10.1088/0264-9381/24/12/S15zbMath1117.85020arXivgr-qc/0612049MaRDI QIDQ5293856

Laura Villain, Michał Bejger, Silvano Bonazzola

Publication date: 4 July 2007

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0612049

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (3)

A spectral method for the wave equation of divergence-free vectors and symmetric tensors inside a sphere ⋮ Weyl's gauge argument ⋮ A study on relativistic Lagrangian field theories with non-topological soliton solutions

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• HARM

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