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Article overview
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General-Relativistic MHD for the Numerical Construction of Dynamical Spacetimes | Thomas W. Baumgarte
; Stuart L. Shapiro
; | Date: |
14 Nov 2002 | Journal: | Astrophys.J. 585 (2003) 921-929 | Subject: | astro-ph gr-qc | Abstract: | We assemble the equations of general relativistic magnetohydrodynamics (MHD) in 3+1 form. These consist of the complete coupled set of Maxwell equations for the electromagnetic field, Einstein’s equations for the gravitational field, and the equations of relativistic MHD for a perfectly conducting ideal gas. The adopted form of the equations is suitable for evolving numerically a relativistic MHD fluid in a dynamical spacetime characterized by a strong gravitational field. | Source: | arXiv, astro-ph/0211340 | Services: | Forum | Review | PDF | Favorites |
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