Basic HTML version of Foils prepared 15 March 1996

Foil 25 Structure of Numerical Relativity Equations in terms of 3 by 3 matrices q and K

From Numerical Formulation and Solution of Collision 0f two Black Holes CPSP713 Case studies in Computational Science -- Spring Semester 1996. by Geoffrey C. Fox
1 K is a Symmetric 3 by 3 matrix
2 And we now have 14 equations:
in Table To:

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