Poisson brackets in general relativity

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SUMMARY

The discussion focuses on the application of Poisson brackets in the context of general relativity, specifically concerning the fundamental variables of the three-dimensional metric tensor g_{ij}(\vec{x}) and its conjugate momentum \pi^{ij}(\vec{x}). The Poisson bracket for these variables is defined as \{F,G\} = \int_\mathcal{M}\left( \frac{\delta F}{\delta g_{ij}}\frac{\delta G}{\delta \pi^{ij}} - \frac{\delta F}{\delta\pi^{ij}}\frac{\delta G}{\delta g_{ij}}\right). A key question raised is the functional derivative \frac{\delta g_{ij}}{\delta g_{kl}}, which is determined to be \frac{1}{2}(\delta^k_i\delta^l_j + \delta^l_i\delta^k_j), reflecting the symmetry of the metric tensor.

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shoehorn
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Hi. I've been wondering about the following and haven't made much progress on it. To set the scene, consider the following. Suppose that we have some sort of discrete theory in which the phase space variables are q^i and p_i. If we have some functions F(q,p) and G(q,p) we can define their Poisson bracket as

\{F,G\} = \sum_i\left( \frac{\partial F}{\partial q^i}\frac{\partial G}{\partial p_i} - \frac{\partial F}{\partial p_i}\frac{\partial G}{\partial q^i}\right)<br />

Then, for example, we have the following fundamental Poisson brackets

<br /> \{q^i,p_j\} = \delta^i_{\phantom{i}j},<br /> \{q^i,q^j\} = \{p_i,p_j\} = 0.<br />

Now suppose that we go to a field theory in which the fundamental `variables' are the position-dependent q^i(\vec{x}) and \pi_j(\vec{x}). The Poisson brackets of two functionals F(q,\pi) and G(q,\pi) are then

\{F,G\} \equiv \sum_i \int_\mathcal{M} dv \left( \frac{\delta F}{\delta q^i}\frac{\delta G}{\delta \pi_i} - \frac{\delta F}{\delta \pi_i}\frac{\delta G}{\delta q^i}\right).

With this definition we obtain

\{q^i(\vec{x}),\pi_j(\vec{x}&#039;)\} = \delta^i_{\phantom{i}j}\delta(\vec{x}-\vec{x}&#039;),<br /> \{q^i(\vec{x}),q^j(\vec{x}&#039;)\} = \{\pi_i(\vec{x}),\pi_j(\vec{x}&#039;)\} = 0.

That's all fine and good. But, in the Hamiltonian version of general relativity the fundamental variables are actually the three-dimensional metric g_{ij}(\vec{x}) and \pi^{ij}(\vec{x}), both of which are symmetric tensors. I can define the Poisson brackets for these variables easily as

<br /> \{F,G\} \equiv \int_\mathcal{M}\left( \frac{\delta F}{\delta g_{ij}}\frac{\delta G}{\delta \pi^{ij}} - \frac{\delta F}{\delta\pi^{ij}}\frac{\delta G}{\delta g_{ij}}\right).<br />

My question is this: what exactly is

\frac{\delta g_{ij}}{\delta g_{kl}}?

I assume that it's not something simple like \delta^i_k\delta^j_l and that it has to reflect the symmetry of the metric tensor, but I can't seem to figure it out. Since I can't figure it out, neither can I work out explicitly what the fundamental Poisson brackets for GR should be.

Can anyone shed some light on this? An immediate extension that springs to mind is the general case of the above, i.e., if T^{a_1\ldots a_r} is some arbitrary (r,0) tensor then what is

\frac{\delta T^{a_1\ldots a_r}}{\delta T^{b_1\ldots b_r}}?
 
Last edited:
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shoehorn said:
My question is this: what exactly is

\frac{\delta g_{ij}}{\delta g_{kl}}?

\frac{1}{2}(\delta^k_i\delta^l_j + \delta^l_i\delta^k_j)


sam
 

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