HELP! * GREY=local LOCAL HTML version of Foils prepared 15 March 1996

Foil 19 Structure of Numerical Relativity Equations in terms of 3 by 3 matrices q and K

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

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