Basic HTML version of Foils prepared 15 March 1996

Foil 22 Projection of Einstein's Equations onto Spacial Surfaces

From Numerical Formulation and Solution of Collision 0f two Black Holes CPSP713 Case studies in Computational Science -- Spring Semester 1996. by Geoffrey C. Fox
The Einstein equations for g mn can now be written in terms of a reduced 3 by 3 symmetric metric matrix q ij
q ij has 9 components of which 6 are independent

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