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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
1 The Einstein equations for g mn can now be written in terms of a reduced 3 by 3 symmetric metric matrix q ij
2 q ij has 9 components of which 6 are independent
in Table To:

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