A Simflowny-based high-performance 3D code for the generalized induction equation

DOI10.1016/j.cpc.2018.11.022arXiv1811.08198OpenAlexW2901952476WikidataQ128832695 ScholiaQ128832695MaRDI QIDQ6046279

Daniele Viganò, A. Arbona, Joan Massó, B. Miñano, Federico Carrasco, Carlos Palenzuela, Carles Bona, J. A. Pons, David Martínez-Gómez

Publication date: 10 May 2023

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1811.08198

zbMATH Keywords

AMRMHDmagnetic fieldsneutron starshigh resolution shock capturing

Mathematics Subject Classification ID

Astronomy and astrophysics (85-XX) Relativity and gravitational theory (83-XX)

Related Items (3)

Essentially non-oscillatory and weighted essentially non-oscillatory schemes ⋮ Magneto-thermal evolution of neutron stars with coupled ohmic, Hall and ambipolar effects via accurate finite-volume simulations ⋮ Global high-order numerical schemes for the time evolution of the general relativistic radiation magneto-hydrodynamics equations

Cites Work

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• Magneto-thermal evolution of neutron stars
• Summation by parts and dissipation for domains with excised regions
• Managing application complexity in the SAMRAI object‐oriented framework
• Magnetic field dissipation in neutron star crusts: from magnetars to isolated neutron stars

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