Think of it this way. -iLog(i) when i is zero. Quantum noise is a bit high.
When the phase elements of the vacuum start deviating from their natural sample rate, they beat against each other, they are stuck with their relaxation moments, the packed nulls fall apart, and the system converts to free space until the sample rates are realigned to the Plank integer.
Derivation of Einstein's field equations
Suppose that the full action of the theory is given by the Einstein–Hilbert term plus a term
describing any matter fields appearing in the theory.![S = \int \left[ {1 \over 2\kappa} \, R + \mathcal{L}_\mathrm{M} \right] \sqrt{-g} \, \mathrm{d}^4 x](https://lh3.googleusercontent.com/blogger_img_proxy/AEn0k_tHyU2r4VC_CCJkd1aaChjOJCxbninF0D6aoarOc1XCPo-OvE6BBiuA3zARUtjjVff3BLIhLy9DPIAPFkzx8_ApLqJQGu6WgsRI7iwg9ZKLykbxXD4AVpBYWdAZFSk4mdlR9sstTRdTFYRHncWYBg=s0-d)
![\begin{align}
0 & = \delta S \\
& = \int
\left[
{1 \over 2\kappa} \frac{\delta (\sqrt{-g}R)}{\delta g^{\mu\nu}} +
\frac{\delta (\sqrt{-g} \mathcal{L}_\mathrm{M})}{\delta g^{\mu\nu}}
\right] \delta g^{\mu\nu}\mathrm{d}^4x \\
& = \int
\left[
{1 \over 2\kappa} \left( \frac{\delta R}{\delta g^{\mu\nu}} +
\frac{R}{\sqrt{-g}} \frac{\delta \sqrt{-g}}{\delta g^{\mu\nu} }
\right) +
\frac{1}{\sqrt{-g}} \frac{\delta (\sqrt{-g} \mathcal{L}_\mathrm{M})}{\delta g^{\mu\nu}}
\right] \delta g^{\mu\nu} \sqrt{-g}\, \mathrm{d}^4x.
\end{align}](https://lh3.googleusercontent.com/blogger_img_proxy/AEn0k_vR73adnVkiKrjAh9CCrDS4TKP_q29mDmq6H5np8W0wTijNtI9hzllrb8bwUuo6GKd3_fNXK2gL7S2K7zujgvlItWOkbmIbn4NbYxbUHyLPOVJJTbX_XfHxZM_DbdDZ1cenvP26TfADcDqg1CMG=s0-d)
How to plot?
Anyway, this is a moment to bring up the issue of plotting. I need to write out scaled up version of the complete sequence to a file and use a stronger plotting package. We should be able to run the quantizer to its limit and actually zero in on the fine details of the periodic table, for example. That is where I am.
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