- #491
Lawrence B. Crowell
- 190
- 2
sweetser said:Hello Lawrence:
And just as seriously, I understand why this holds together so tightly from a logical perspective. I have even learned from you how odd it is to try and tack on something symmetric to this construction, which is not what I am trying to do. Every tight web of logic has an underlying assumption. What underlies this is the assumption that the Riemann curvature tensor is necessary to describe the physical force of gravity. GR does work that way, we have darn great data to say GR is correct. All vetted researchers try to recreate GR in a wider context, or do a technical variation on the rank 2 field theory theme. I hope to show that GR, as good as it is, is not good enough for a unified field theory, it will be a challenge to challenge. I heard no reply to the long standing energy problem which is well known and well ignored today. There is no trivial way around that problem. If the Riemann curvature tensor is not relevant to the way unified fields in Nature work, then the Bianchi identities - a property of the Riemann curvature tensor - are also not important, nor are the bundles built on top of it all.
You have fallen into the trap! There is no energy problem with general relativity, at least if you think about it correctly. What you see as a problem is in fact an astounding fact of cosmology which is vitally important! Here is what you think the problem is, which I will state in fairly precise terms. The deSitter spacetime, which our cosmology appears to be asymptoting towards, as the metric
[tex]
ds^2~=~-dt^2~+~e^{\beta t}(dr^2~+~r^2d\Omega^2)
[/tex]
The metric terms are time dependent and it is not possible to find a [itex]k_t[/itex] so that there is a stationary condition [itex]{\cal L}_{K_t}g~=~0[/itex] , for a Lie derivative [itex]{\cal L}_{K_t}~=~\kappa\partial/\partial t[/itex]. This Lie derivative is defined according to brackets so that
[tex]
{\cal L}_{k_t}g(X,~Y)~=~g([K_t,~X],~Y)~+~g(X,~[K_t,~Y]),
[/tex]
where the brackets [itex][K_t,~X][/itex] are not zero because the vectors X are functions of time. So there is no involutary system which defines a conservation of energy on the entire spacetime. The basis vectors for the deSitter cosmology are [itex]]X_i~=~exp(\sqrt{\Lambda/3}~t/2)[/itex] and so the above expression gives
[tex]
{\cal L}_{K_t}g_{\mu\nu}~=~\sqrt{\Lambda/3}g_{\mu\nu}
[/tex]
For the cosmological constant [itex]\Lambda~=~3H^2\Omega/c^2[/itex] this equation is an eigenvalued equation, and the nonvanishing of the Hubble constant is a measure of how [itex]k_t[/itex] fails to be a proper Killing vector.
[tex]
{\cal L}_{K_t}g_{\mu\nu}~=~Hg_{\mu\nu}
[/tex]
The Hubble constant defines a velocity-distance rule [itex]H~=~{\dot R}/R[/itex], for [itex]R(t)[/itex] a scale factor for the cosmology.
This gives a nonconservation of energy! There is no symmetry in general which defines a conservation of energy in a cosmology. This might for some be a horrible problem --- for me it is an astounding miracle! Now there is still the continuity equation [itex]\nabla_a T^{ab}~=~0[/itex], which is related to Bianchi identities etc, but the energy is the projection of a manifold basis vector on the momentum energy tensor
[tex]
E^a~=~\Big(\int_{V^3}~-~\int_{V'^3}\Big) e_bT^{ab}
[/tex]
which is defined in a region of four spacetime bounded by three bounding spatial surfaces. The generalized Stokes' law then tells us this is the same as the differential of the integrand evaluated on the enclosing four spacetime
[tex]
E^a~=~\int_{V^4}d(e_bT^{ab})
[/tex]
which can be expressed according to the covariant derivative. This will give a covariant derivative on the basis vector with [itex]de_a~=~{\underline\omega_a}^b e_b[/itex], and the differential one form is a connection form. This is coordinate dependent and so the energy can't be localized. In the above case with cosmology, this is a similar result, but here the energy can't be defined globally and conservation of energy is not a global law.
A cosmology with a nonzero cosmological constant, or what is likely a parameter set into a constant (or approximately constant) value by the inflaton or dilaton in a [itex]spin(4,2)~\sim~su(2,2)[/itex] model, is one where in general there is no unitarily equivalency between states in all regions of the cosmology. Even if the spatial surface is flat the accelerated expansion of the cosmology means that there is no such equivalency, and this comes about because there is no Killing vector K which when it acts on the energy KE = const. Without a Killing vector of this sort it means there is no isometry in the spacetime which maintains a constant energy on all paths in the cosmology. So the unitarity inequivalence of vacua in the earliest universe, where a vacua of unitary states is defined on a region [itex]\sim L_p[/itex] in a superposition of other such vacua on about the same scale, is frozen into the classical cosmology after inflation. In a more general setting the Coleman-Mandula theorem is then a local principle. This gives the maximal set of symmetries of the S-matrix as the [itex](0,~1/2)\oplus(1/2,~0)[/itex] spinorial Lorentz group for external symmetry, an internal symmetry [itex][A_i,~A_j]~=~c_{ijk}A_k[/itex], and the discrete CPT symmetry. The "maximal" extension on this is called supersymmetry. A cosmology with a non-zero cosmological constant necessarily means this is a local law, it does not apply globally. This is likely a source for what we call dark energy.
I will leave this at this point. This might sound odd, but this is a tremendous blessing. This is not something physicists should try to bury away, but embrace it. If thought about properly the consequences are astounding.
Lawrence B. Crowell