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High-order methods for the simulation of hydromagnetic instabilities in core-collapse supernovae

Published online by Cambridge University Press:  08 June 2011

T. Rembiasz ,
M. Obergaulinger ,
M. Angel Aloy ,
P. Cerdá-Durán  and
E. Müller
T. Rembiasz*
Affiliation:
Max-Planck-Institut für Astrophysik, 85748 Garching, Germany
M. Obergaulinger
Affiliation:
Max-Planck-Institut für Astrophysik, 85748 Garching, Germany
M. Angel Aloy
Affiliation:
Universitat de València, 46100 Burjassot (Valencia), Spain
P. Cerdá-Durán
Affiliation:
Max-Planck-Institut für Astrophysik, 85748 Garching, Germany
E. Müller
Affiliation:
Max-Planck-Institut für Astrophysik, 85748 Garching, Germany
*
*email: [email protected]
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Abstract

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We present an assessment of the accuracy of a recently developed MHD code used to study hydromagnetic flows in supernovae and related events. The code, based on the constrained transport formulation, incorporates unprecedented ultra-high-order methods (up to 9th order) for the reconstruction and the most accurate approximate Riemann solvers. We estimate the numerical resistivity of these schemes in tearing instability simulations.

Keywords

reconstruction schemesRiemann solvershydromagnetic instabilities
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 479 - 481
Copyright
Copyright © International Astronomical Union 2011

References

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