Solve GR Equations with Regular Method

quZz
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Hi everyone,

I don't fully understand what is the regular method to state and solve problems in GR when no handy hints like spherical symmetry or homogeneity of time are assumed. If I find myself in arbitrary reference frame with coordinates x^0, x^1, x^2, x^3 the meaning of which is unknown beforehand (or known only locally), how do I proceed with boundary conditions and stress-energy tensor?

Consider the following simple problem: two point masses m_1, m_2 are separated by distance a. Obviously T_{\mu\nu} is a sum of two delta functions. Suppose the first mass is at the origin but where then is the second mass? Should I write \delta(x^1 - a) or \delta(\sqrt{(x^1)^2 + x^1 x^2} - a) or ...? You may say - OK, choose the coordinates in such a way that \delta(x^1 - a) would be valid. But there are only 4 possible coordinate transformations, what if I had thousands of point masses?

So it seems that in general a statement of a problem in GR is interconnected with its very solution, which is confusing: are all problems solvable? uniquely? what would a "real mccoy" equation look like?
 
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quZz said:
Hi everyone,

I don't fully understand what is the regular method to state and solve problems in GR when no handy hints like spherical symmetry or homogeneity of time are assumed. If I find myself in arbitrary reference frame with coordinates x^0, x^1, x^2, x^3 the meaning of which is unknown beforehand (or known only locally), how do I proceed with boundary conditions and stress-energy tensor?

Consider the following simple problem: two point masses m_1, m_2 are separated by distance a. Obviously T_{\mu\nu} is a sum of two delta functions. Suppose the first mass is at the origin but where then is the second mass? Should I write \delta(x^1 - a) or \delta(\sqrt{(x^1)^2 + x^1 x^2} - a) or ...? You may say - OK, choose the coordinates in such a way that \delta(x^1 - a) would be valid. But there are only 4 possible coordinate transformations, what if I had thousands of point masses?

So it seems that in general a statement of a problem in GR is interconnected with its very solution, which is confusing: are all problems solvable? uniquely? what would a "real mccoy" equation look like?

As starting point:

http://en.wikipedia.org/wiki/ADM_fo...Numerical_Solutions_of_the_Einstein_Equations

Read here about the ADM formalism in general, then its use for initial value problems in numerical relativity. Of course, start with wikipedia with a grain of salt, and study the references.
 
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