how you've quantised gravity.
I don't claim to have finished quantization of gravity.
Instead, my "to do" list contains "The connection between the SM ether model and the ether theory of gravity, which are metaphysically compatible but mathematically yet unrelated theories;" The SM ether model is already a quantum theory, but the theory of gravity not yet.
The claims "The ether approach
to gravity solves many quantization problems of GR quantization: The notorious
problem of time [10] simply disappears. Together with the black hole collapse
the related information loss problem [13] disappears too."
are sufficiently obvious even without finishing quantization if you know the mentioned problems, for more details see gr-qc/0205035.
Especially I quote a paper about the problem of time with "``... in quantum gravity, one response to the problem of time is to `blame' it on general relativity's
allowing arbitrary foliations of spacetime; and then to postulate a
preferred frame of spacetime with respect to which quantum theory
should be written.'' My ether theory obviously follows this way.
QUOTE
You have done nothing more than use the GR equations for a perfect fluid (which is, literally, the textbook way to derive the Einstein Field Equations in a simple system), without reference to your ether you outline in the first part of the paper. Everything in section 4 is just usual GR but you're claiming it's an aether, your aether.
Sorry, but that's simply false. The continuity and Euler equations, as I use them, are classical fluid equations, with partial instead of covariant derivatives, and have nothing to do with GR equations for some fluid on some curved background or so. It is certainly not the textbook way to derive the EFE, already because I do not derive the EFE. Instead I derive the EFE with some additional term.
The additional term is not "just usual GR", it prevent black hole and big bang singularities and enforces harmonic coordinates.
It holds for all ether theories which fulfill the axioms. If such a Lagrange formalism exists for the continuous limit of my SM model is an open question. I can hardly answer it without having found the general Lagrangian for the SM model. (Which requires symmetry breaking + continuous limit.)
QUOTE (->
| QUOTE |
| You have done nothing more than use the GR equations for a perfect fluid (which is, literally, the textbook way to derive the Einstein Field Equations in a simple system), without reference to your ether you outline in the first part of the paper. Everything in section 4 is just usual GR but you're claiming it's an aether, your aether. |
Sorry, but that's simply false. The continuity and Euler equations, as I use them, are classical fluid equations, with partial instead of covariant derivatives, and have nothing to do with GR equations for some fluid on some curved background or so. It is certainly not the textbook way to derive the EFE, already because I do not derive the EFE. Instead I derive the EFE with some additional term.
The additional term is not "just usual GR", it prevent black hole and big bang singularities and enforces harmonic coordinates.
It holds for all ether theories which fulfill the axioms. If such a Lagrange formalism exists for the continuous limit of my SM model is an open question. I can hardly answer it without having found the general Lagrangian for the SM model. (Which requires symmetry breaking + continuous limit.)
You certainly do not approach the issue of quantising it, you just work out some classical equations of motion
Indeed.
QUOTE
(or rather, you just state them)
I postulate classical continuity and Euler equations, and their connection with the Lagrange formalism (a form of the Noether theorem). What follows is a derivation of the most general Lagrangian.
QUOTE (->
| QUOTE |
| (or rather, you just state them) |
I postulate classical continuity and Euler equations, and their connection with the Lagrange formalism (a form of the Noether theorem). What follows is a derivation of the most general Lagrangian.
Previously you'd written out mode operators for the quantum fields, why don't you do this for gravity? You can't claim to have used your ideas to 'solve problems with quantising gravity' when you never address it!
Quantization of gravity consists of two parts: Defining a quantum theory, and to show that the classical continous limit of this theory is, in some limit, GR.
I have defined now the quantum theory. There are some open problems with the connection between the ether model and the continuous theory of gravity (I need a very special form of the Lagrange formalism for the continuous limit of my model), but, assume they can be solved on the classical level.
Then, there is no need for writing down quantum operators for gravity. It is already defined. The continuous limit of the quantum theory may be full of technical problems. But these are problems of derivation of continous limits of well-defined quantum theories, not problems of defining quantum gravity.
In gr-qc/0205035 I have addressed some quantization issues. And what I have done after this, working on my SM model, was the following point in that quantization program:
"Next, we have to find atoms, that means, to discretize the
problem. The density $\rho$ should be identified with the number of
nodes inside a region,..."
QUOTE
If you continue down the road you appear to be on, ie just rehashing mainstream work in a very naive way, you'll find that you're unable to quantise gravity because of renormalisation issues.
It may be, indeed, that the situation with various types of hierarchy problems (smallness of the cosmological constant) is not better in my approach. This is left to future research. But, even in the worst case, the result will be a well-defined theory with some fine-tuning problem. Or what else do you expect?
QUOTE (->
| QUOTE |
| If you continue down the road you appear to be on, ie just rehashing mainstream work in a very naive way, you'll find that you're unable to quantise gravity because of renormalisation issues. |
It may be, indeed, that the situation with various types of hierarchy problems (smallness of the cosmological constant) is not better in my approach. This is left to future research. But, even in the worst case, the result will be a well-defined theory with some fine-tuning problem. Or what else do you expect?
Even with the notion of a lattice to quantise on, it's not immediately trivial, since lattice methods are common place in mainstream QFT and they don't help with gravity.
I agree.
But note that a whole direction of research - LQG - want's much more, namely to derive the dimensionality of spacetime from some foam-like background-free lattice.
That's not what I have to do. In my approach, the background R^3 x R is already given from the start.
Note also that non-renormalizability is not an issue.
The only issue related with renormalization are various fine-tuning problems. I acknowledge their importance, but, nonetheless, having a well-defined unitary and so on theory with some fine tuning problems is much better than having no such theory at all.
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