Unifying Gravity and EM

In summary, the conversation discusses a proposal for a unified field theory that combines gravity and electromagnetism into a single rank 1 field. The Lagrange density for this proposal is provided, along with a discussion of how the equations are generated and the physical implications of the theory. The proposal is consistent with both weak and strong field tests of gravity and there are no known physical experiments that contradict it.
  • #526
Maxwell and GEM derivation on YouTube

Hello:

I will be going to the New England APS/AAPT Meeting in New London, Connecticut on Saturday to give the talk "Using Quaternions for Lagrangians in EM and GEM." At just under 15 minutes, you will be able to see the Maxwell equations derived from its Lagrangian. Rarely will you see this much detail about this central part of physics. GEM is a small variation on the theme, where you can see the 12 of 24 terms flip signs, generating a relativistic cousin of Newton's field equations for gravity. Enjoy.

Doug

http://youtube.com/watch?v=P9TUqUXGgpE
 
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  • #527
Lawrence B. Crowell said:
Teleparallel connections are commutative for special cases of nongeodesic motion. Christopher Columbus sailed to the new World on a nearly teleparallel path.

I can see that the connections are symmetric for geodesics (force-free) motion. But are the generators of the translation group identified with the connections ? The connections are derivatives of the gauge field whose generators commute. I'm busking this, maybe you can set me straight.

Lut
 
  • #528
Connections in Standard EM

Hello Lut:

On my latest YouTube talk, I got asked a good question: what would the Maxwell and GEM derivations look like if I included all the connections? I know that because the EM field strength tensor uses an exterior derivative, I could just they that is why they drop out. I wish to see these drop in detail. I will make the same presumptions as happen in GR: the connection is metric compatible and torsion-free, so I can use Christoffel symbols of the second kind. These are not tensors and have 3 indexes. What I hope to learn is how exactly to play with Christoffel symbols in EM, so that they all happen to drop out. Seeing this work for the B field gives us a good place to start:

[tex]\nabla \times A = \frac{\partial A^u}{\partial x^v} - \Gamma_{\mu}^{v u} A^{\mu} - \frac{\partial A^v}{\partial x^u} + \Gamma_{\mu}^{u v} A^{\mu}[/tex]

[tex]= \frac{\partial A^u}{\partial x^v} - \frac{\partial A^v}{\partial x^u}\quad eq 1[/tex]

Because the Christoffel is symmetric in the indexes, the two gammas cancel. I figured a similar thing should happen with the E field, but I must be missing a sign:

[tex]E = -\frac{\partial A^u}{\partial t} + \Gamma_{\mu}^{0 u} A^{\mu} -\frac{\partial \phi}{\partial x^u} + \Gamma_{\mu}^{u 0} A^{\mu}\quad eq 2[/tex]

This time the gammas add. Oops. Where did I misstep?

Thanks,
Doug
 
  • #529
Losing connections

Hi Doug:
I'll try and repeat the calculations above later. The covariant derivatives cancel out in the field tensor.

[tex]F_{\mu\nu} = \nabla_{\mu}A_{\nu} - \nabla_{\nu}A_{\mu}[/tex]

where

[tex]\nabla_{\mu}A_{\nu} = \partial_{\mu}A_{\nu} - \Gamma^{k}_{\mu\nu}A_k[/tex]

and because of the symmetry in the lower indexes the Gamma factors cancel.

As I've pointed out many times, this does not happen with the symmetric field tensor, so you end up with terms containing A^2 in the lagrangian, as well as functions of the metric.

I just don't see how you can mix up a metric theory and a vector potential. Your field equations are four in number and your unknowns are 10 for the metric ( 40 connections) and 4 for the potential. How do you solve that ?

Lut
 
  • #530
Mistake in 529

Hello Lut:

It looks like my mistake in Eq. 2 of post #529 was on the first gamma, it should have been negative. For the E field, I need:

[tex]E = \nabla_{0}A_{u} - \nabla_{u}A_{0} = -\frac{\partial A_u}{\partial t} - \Gamma^{k}_{0 u}A_k - (\frac{\partial \phi}{\partial x^u} - \Gamma^{k}_{u 0}A_k)[/tex]


So the minus in the first term happens from the lower script for the Au which does not change the sign of the gamma. The minus on the second term does flip the switch on the second gamma, making it positive. Not difficult, but I need to get rock solid on how signs work in standard EM first, then out to GEM. Gammas are always negative unless one tosses a minus sign in front.

Doug
 
  • #531
Hi Doug:

with non-zero Christoffel symbols, raising and lowering indices is a nightmare -

[tex] A_{\mu} = g_{\mu\nu}A^{\nu} = A_{0}g^{\mu 0}+A_{1}g^{\mu 1}+A_{2}g^{\mu 2}+A_{3}g^{\mu 3}[/tex]

and this

[tex]\Gamma^{ bc}_{a} = g_{ka}g^{bm}g^{cn}\Gamma^{k}_{ mn}[/tex]

has 64 terms.

Note that most of the GEM calculations I did are with the Minkowski metric.

Lut
 
  • #532
3-vector versus 3-vector

Hello:

I am writing code to handle the Even representation of quaternions on the command line so I can make animations using them. In this context, quaternions are always 4 numbers that get piped from one program to another. It is not possible to know if a quaternion being fed into the next program in a chain of these programs was an Even or Hamilton quaternion.

When I got to the nuts and bolts of the programming, I noticed that this issue only matters for binary operations, and then only for that part of the binary operation that has the 2 3-vectors forming a product. In the Hamilton representation, the dot product gets a minus sign, the even dot product stays positive. In the Hamilton representation, the curl is the curl with half the terms positive, half minus. In the Even representation, all the same terms are all positive.

A few issues are missed by using tensors. One is the issue of knowing there is an inverse for both the Hamilton and Even representations of quaternions. I used to justify this on an issue of quantum field theory which is kind of obscure. A more apparent reason might have to do with the observation of the critical importance of group theory in physics. The definition of a group relies on there being both an identity and an inverse for every member of the group. Those are both there for these two representations of quaternions. Tensors don't have to have inverses.

Doug
 
  • #533
Complete analysis of vector current coupling

Hello:

I am preparing a talk for an APS meeting in St. Louis. One of the points I intend to make is that Feynman's analysis of the phase of the current coupling term is incomplete. The image really rocks, but I am unsure how to upload images here, so I'll have to get by with LaTeX.

The current coupling term is also known as the source term: [itex]-J^{\mu} A_{\mu}[/itex]. Take the Fourier transform of the potential to get J'/k2. Since the indices are the same, this term evaluates to the following scalar:

[tex]-J^{\mu} J'_{\mu}/k^2 = (-\rho \rho' ~+~ Ax Ax' ~+~ Ay Ay'~+~ Az Az')/k^2 \quad eq~1[/tex]

What Feynman does is consider a specific case of a current moving along the z axis. While it makes the algebra simpler, it made my slide longer, and not as general. Skip all the z-axis specific stuff, and just multiply these two together using the Hamilton representation of quaternions:

[tex]-J J'/k^2 = (-\rho \rho' ~+~ Ax Ax' ~+~ Ay Ay'~+~ Az Az', [/tex]

[tex]-\rho Ax' ~-~ Ax \rho' ~+~ Ay Az'~-~ Az Ay', [/tex]
[tex]-\rho Ay' ~-~ Ay \rho' ~+~ Az Ax'~-~ Ax Az', [/tex]
[tex]-\rho Az' ~-~ Az \rho' ~+~ Ax Ay'~-~ Ay Ax')/k^2 \quad eq~2[/tex]

The phase is the final 3 lines of eq 2. What Feynman calculated was part of the third line, [itex]Ax Ay'~-~ Ay Ax'[/itex]. These two terms do not add together, so it will take 2 pi to get back to the starting position, the sign of spin 1 symmetry. That is excellent, since these terms are the transverse modes of EM that need spin 1 symmetry so like charges repel.

Now look at the first two terms of the third line, [tex]-\rho Az' ~-~ Az \rho'[/itex]. These do work together, and will require only pi rotations to get back to the starting position. This is a property of spin 2 symmetry. Spin 2 particles are needed for systems where like charges attract. A complete analysis of the phase looks good to me.

Doug
 
  • #534
Mentz114 said:
I can see that the connections are symmetric for geodesics (force-free) motion. But are the generators of the translation group identified with the connections ? The connections are derivatives of the gauge field whose generators commute. I'm busking this, maybe you can set me straight.

Lut

I guess I missed this one. Non-geodesic motion involves some other force on the motion of a particle. Teleparallel connections have a number of meaning as I understand. One is that the geodesic motion is given by a horizontal bundle and the "force" by a vertical bundle. This is Finsler geometry. Another definition, related maybe, is where the motion is parallel or Euclidean-like (latitudinal lines on a globe) and where the force or vertical bundle terms act to sustain this flow. I think this can result in torsional gravity.

Lawrence B. Crowell
 
  • #535
New article out that perhaps reads on this subject:

A Spatially-VSL Gravity Model with 1-PN Limit of GRT
Jan Broekaert
In the static field configuration, a spatially-Variable Speed of Light (VSL) scalar gravity model with Lorentz-Poincaré interpretation was shown to reproduce the phenomenology implied by the Schwarzschild metric. In the present development, we effectively cover configurations with source kinematics due to an induced sweep velocity field w. The scalar-vector model now provides a Hamiltonian description for particles and photons in full accordance with the first Post-Newtonian (1-PN) approximation of General Relativity Theory (GRT). This result requires the validity of Poincaré’s Principle of Relativity, i.e. the unobservability of ‘preferred’ frame movement. Poincaré’s principle fixes the amplitude of the sweep velocity field of the moving source, or equivalently the ‘vector potential’ ξ of GRT (e.g.; S. Weinberg, Gravitation and cosmology, [1972]), and provides the correct 1-PN limit of GRT. The implementation of this principle requires acceleration transformations derived from gravitationally modified Lorentz transformations. A comparison with the acceleration transformation in GRT is done. The present scope of the model is limited to weak-field gravitation without retardation and with gravitating test particles. In onclusion the model’s merits in terms of a simpler space, time and gravitation ontology—in terms of a Lorentz-Poincaré-type interpretation—are explained (e.g. for ‘frame dragging’, ‘harmonic coordinate condition’).
http://www.springerlink.com/content/b3758t680gj383j8/

Back on the first of the year, Foundations of Physics (the above journal) picked up a new editor, Gerardus 't Hooft, who writes:

During my first couple of months in this office, it became clear that fundamental questions in physics and philosophy also attract the interest of many laymen physicists.

We receive numerous submissions from people who venture to attack the most basic premises of theories such as Special Relativity, but instead only succeed in displaying a lack of professional insight in how a physical theory is constructed. I suspect that some of these people may have been working somewhere in an attic, deprived from daylight for decades, determined only to reemerge with a Theory of Everything in their hands. Even though they may be very sincere, we have to disappoint such authors. New insights are gained only by intense interactions with professionals all over the globe, and by solidly familiarizing oneself with their findings, and we must make a selection from only those papers whose authors have a solid understanding of the topics they are discussing.

Fortunately they also submit their work, and their clever inventiveness continues to surprise us.
...
I hope to receive your submissions. Acceptation of a paper may not necessarily mean that all referees agree with everything, but rather that the issues put forward by the author were considered to be of sufficient interest to our readership, and the exposition was clear enough that our readers, whom we assume to be competent enough, can judge for themselves.
...
http://www.springer.com/physics/journal/10701
 
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  • #536
Variable Speed of Light theory

Hello Carl:

The paper cost $32 to download, ouch. I know I have a bias against spatially-Variable Speed of Light theories. On my dinning room wall is a large artwork, The Speed of Light According to Rene Magritte. I think about c as time's relationship to space. Photons travel at the speed of light because time is space. It is hard to see how that statement can vary.

Any reasonable proposal for gravity must agree to the first parameterized Post-Newtonian accuracy, as these folks do. I am a bit surprised they didn't look at the second level of accuracy.

The "scalar-vector model" might have passing similarities to GEM, but I am skeptical.

The attitude of the editor parallels some of the motivations of the Independent Research section of Physics Forums. 't Hooft has a site, How to become a good theoretical physicist, I always recommend to people working alone in the attic.

Should I ever get satisfied with my draft paper, I would consider sending it there. A number of issues need to be addressed first. I need to shift the action from tensor notation to quaternions because the issue of gauge symmetry must be clearly addressed. Second, I still have to get the energy expression in order.

I am emailing from the April APS Meeting in Saint Louis. I heard a talk by someone who is trying to take EM up a level to use the tools similar to GR, basically the opposite direction I am traveling. That talk gave me a good overview of the various approaches to EM as a geometry phenomena. I asked the speaker to send me his slides.

The talks about dark matter and dark energy make me sad. They certainly don't sound like solid physics. In a question and answer section, I confirmed with the speaker that she knew of no large scale systems where Newtonian gravity produces the observed results. That is what I expect since I think an unusual effect of gravity, labeled the relativistic rocket effect, Vc dm/dR Vhat, is never put into their numerical integration systems. I will recall these talks when trying to approach my fears of doing the calculations (they look hard, and I know my limitations too well).

Doug
 
  • #537
Doug:
Jan Broekaert has several papers in the arXiv. Do a search in GR-QC for his name in authors. I'm having a look at one later, for diversion. Wiil report if it's interesting.

Carl:
I enjoyed the quote from t'Hooft.

Lut

[edit : this appears to be the very paper. Save $32 now !]

arXiv:gr-qc/0405015
 
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  • #538
CarlB said:
New article out that perhaps reads on this subject:

A Spatially-VSL Gravity Model with 1-PN Limit of GRT
Jan Broekaert
In the static field configuration, a spatially-Variable Speed of Light (VSL) scalar gravity model with Lorentz-Poincaré interpretation was shown to reproduce the phenomenology implied by the Schwarzschild metric.

These types of theories are curious, but as Doug pointed out c is just an invariant measure by which space and time are equivalent. The value of c in its particular comes from other units in nature associated with electromagnetism, e, [itex]\epsilon_0,~\mu[/itex] and so forth. If suspect that a variability in c or some energy dependence might come about near the Planck scale, but then again the Planck scale is defined according to c.

Lawrence B. Crowell
 
  • #539
Lawrence B. Crowell said:
These types of theories are curious, but as Doug pointed out c is just an invariant measure by which space and time are equivalent.

This is true only under the assumption that there is no preferred coordinate system. In that sense, the equivalence is logically circular. Any theory of gravity that is built on a flat underlying space has to have a variable speed of light. And in such a theory, the speed of light is well defined and variable.

My favorite such theory is the gauge theory of gravity by the Cambridge geometry group. The math it uses is based on the Clifford algebra of Dirac's gamma matrices (which they call "geometric algebra" following David Hestenes). Their theory is identical to GR (to all orders) outside of the event horizons but is built on a flat (well, Minkowski) underlying space or coordinates. I started a website supporting their theory here that includes links to the papers:
http://www.gaugegravity.com/
I'm planning on redoing the website to make it more informational soon. There are a lot of articles that use these ideas to model electrons and black holes, and I need to link those in.

When you have a flat gravity theory (and from my point of view, Sweetser's theory is flat), the first thing to do is to write down what the theory does for a singular mass, a black hole. This defines a preferred coordinate system, and that system defines the speed of light in the theory.

Since gauge gravity is identical to GR, the gravity you get from it is equivalent to GR written in a particular choice of coordinates. The stationary black hole becomes Painleve coordinates for the Schwarzschild solution. I created a java applet simulation that shows the relation of these to the usual Schwarzschild coordinates here:
http://www.gaugegravity.com/

Now the original name of the applet was "sweet" because I wanted to include Sweetser's gravity as well as Newton, and Einstein's in Schwarzschild and Painleve coordinates. However, I haven't figured out how to actually write down his equations, in the form of the acceleration felt by a test body, and so I haven't modeled it yet. I quit asking, but if he comes up with an equation, I'll type it up into java and add it to the simulation (hint hint).
 
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  • #540
oscillation can respond ?

(translation from french observation)

I think a new theory for source gravity. Maybe the origin of gravity is an oscillation of electrostatic wave. The oscillation of each particle is very very small compared an electron charge. Each particle send a wave, and each wave is accumulate to another wave. The charge of a particle is 0 but the wave is something around 0, one moment + and later - etc. So, each particle send + and - wave around it. It's possible to synchronize all wave because there is a difference between forces if you imagine two sinusoide waves face to face, there is two waves very close and two waves far, the force is with 1/d² so the difference can create a synchronism. This can explain deviation of light and redshift. The formula of perihelion precession of Mercury is the same with electrostatic forces integrate in the formula.

I have create a site for explain (in french for the moment) my ideas: 3w eisog dot com

Maybe this idea is not new, tell me ...

Ludovic
 
  • #541
The breaking of Lorentz symmetry has been proposed by some. I am not sure how I stand on this for certain --- leaning against the idea I suppose. One can work with all sort of pseudotensors and the like with this, though I am not sure if that is what Sweetser is doing.

Gauge gravity, or in a general form with the B-F or Plebanski Lagrangian, recovers Einstein's gravitation at least for weak [itex]\alpha^2~\sim~G[/itex], though corrections on this for stronger G and higher energy (also I suspect cosmological scales) probably lead to consequences beyond a naive breaking of Lorentz symmetry.

Lawrence B. Crowell
 
  • #542
All tensors

Hello Lawrence:

The GEM proposal does not appear to break Lorentz symmetry.

This issue of tensors and GEM remains a concern. We know that [itex]\nabla_{\mu} A_{\nu}[/itex] transforms like a tensor because that is why the machinery of a covariant derivative was built. We also know that the field strength tensor of EM transforms like a tensor, [itex]\nabla_{\mu} A_{\nu} ~-~ \nabla_{\nu} A_{\mu}[/itex]. Correct me if I am wrong, but I believe that the difference of two tensors of the same order is also a tensor. If that is the case, then:

[tex]\nabla_{\mu} A_{\nu} - \frac{1}{2}(\nabla_{\mu} A_{\nu} ~-~ \nabla_{\nu} A_{\mu})[/tex]

[tex]= \frac{1}{2}(\nabla_{\mu} A_{\nu} ~+~ \nabla_{\nu} A_{\mu})\quad eq ~1[/tex]

Is it fair to call this object with the plus sign a tensor? Sure would hope so. Yes all three have different properties, but they all look like they belong in the family of tensors, not pseudotensors.

Doug
 
  • #543
Lawrence B. Crowell said:
Gauge gravity, or in a general form with the B-F or Plebanski Lagrangian, recovers Einstein's gravitation at least for weak [itex]\alpha^2~\sim~G[/itex], though corrections on this for stronger G and higher energy (also I suspect cosmological scales) probably lead to consequences beyond a naive breaking of Lorentz symmetry.

This is a different gauge gravity than that of the Cambridge geometry group. I guess "gauge" is a cool word to use to describe a theory. The Cambridge version is identical to GR to all orders, at least locally. Where it differs is in that you can't do weird topological things like wormholes. Here's how David Hestenes puts it:

The specialization of GA [i.e. Geometric Algebra] to Minkowski spacetime is called Spacetime Algebra (STA). As explained below, STA clarifies the geometric significance of the Dirac Algebra and thereby extends its range of application to the whole of physics. In particular, STA provides the essential mathematical framework for the new Gauge Theory Gravity (GTG).

The foundations of GTG are fully expounded in a seminal paper, so we can concentrate
on highlights of its unique features. GTG is a gauge theory on Minkowski spacetime, but locally it is equivalent to General Relativity (GR), so it can be regarded as an alternative formulation of GR.8 However, GTG reformulates (or one might say, replaces) Einstein’s vague principles of equivalence and general relativity with sharp gauge principles that have clear physical consequences (Section IV). These gauge principles are more than mere rephrasing of Einstein’s ideas. They lead to intrinsic mathematical methods that simplify modeling and calculation in GR and clarify physical meaning of terms at every stage. In particular, they provide clean separation between gauge transformations and coordinate transformations, thus resolving a point of longstanding confusion in GR. Moreover, GTG simplifies and clarifies the analysis of singularities, for example, in assignment of time direction to a black hole horizon. Finally, since tensors and spinors are fully integrated in STA, GTG unifies classical GR and relativistic quantum mechanics with a common system of gauge principles. Besides facilitating the application of quantum mechanics to astrophysics, this opens up new possibilities for a grand unification of gravitation and electroweak theories, as explained in Section V.
http://modelingnts.la.asu.edu/pdf/procGTG-RQM.pdf

So far, GR has only been verified to 1-PN. I don't think that it will make 3-PN. What I like about Sweetser's gravity is that it seems natural to do as the consequences of a particle theory. The problem I see in doing this is that to end up with a variable speed of light type gravity theory requires that the force of gravity be carried by superluminal particles.

In other words, just as Maxwell's equations end up being a force mediated by a speed of light particle, a theory which produces a variable speed of light needs to be mediated by something that moves at some higher speed. Comments from Doug?
 
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  • #544
Geometric Algebra and Quaternions

Hello Carl:

Your email inspired me to go make another effort to wrap my head around geometric algebra. David Hestenes will be giving a keynote address at the conference in Brazil. Both Clifford algebras and geometric algebra fans view there tools as more general that quaternions, since quaternions are just Cl(0, 2) or a 0,2-multivector.

There is not much difference between these three approaches, but there is some. I think of the basis vectors differently, due to looking at this with my physics glasses on. A quaternion is described as a 0,2 multivector, which means a scalar for the first part, and three bivectors, e2/\e3, e3/\e1, and e2/\e1 for the 3-vector.

There are two issues the physicists in me objects. First, the main message of special relativity is to bring the scalar in with the 3-vector on equal footing. I look at quaternons at being 4 scalars with 4 basis vectors: (a0 e0, a1 e1, a2 e2, a3 e3). The GA folks like the wedge because it explains the minus signs. I find that claim hollow since is merely shift where the minus comes into the wedge itself. In my view of quaternions, the four parts look like equals.

The second objection comes from my view of gravity. In GEM, gravity can be about the potential, the basis vectors, or a combination of both. When it is about the basis vectors, then I want to be able to shift e0, e1, e2, and e3. For the exponential metric, e0 = exp(-2 GM/c^2 R) and e0 e1 = e0 e2 = e0 e3 = 1. I don't see how I could make similar statements with the GA formalism.

In the cited paper, Hestene explains how to do the Dirac algebra using geometric algebra. The details are different from how I do that with quaternions as triple products (all sixteen possibilities for e_u Q e_v make up the action of the gamma matrices).

My guess is the GA crowd will not be happy with the even representation of quaternions. I will get to find out, since that will lead off my 25 minute talk in Brazil.

The Cambridge geometry group looks like it is trying to recreate general relativity, with some more polite features. The GEM work is in line with a long tradition of directly confronting the dominant idea of the day, saying it is good up to 1-PN, but not 2-PN. One of those binary pulsar guys was at the APS meeting. I asked him if it is correct to take the equations developed for super-weak perihelion precession and apply it to a strong, dynamic system. If he writes back, I'll commmunicate to this thread.

I stay away from "faster than light". Using quaternions for everything is radical enough!

Doug
 
  • #545
CarlB said:
This is a different gauge gravity than that of the Cambridge geometry group. I guess "gauge" is a cool word to use to describe a theory. The Cambridge version is identical to GR to all orders, at least locally. Where it differs is in that you can't do weird topological things like wormholes. Here's how David Hestenes puts it:

The specialization of GA [i.e. Geometric Algebra] to Minkowski spacetime is called Spacetime Algebra (STA). As explained below, STA clarifies the geometric significance of the Dirac Algebra and thereby extends its range of application to the whole of physics. In particular, STA provides the essential mathematical framework for the new Gauge Theory Gravity (GTG).

Spinor algebra can reproduce general relativity in a pretty straightforward manner. The Dirac matrices [itex]\gamma_\mu[/itex] define the metric as

[tex]
\gamma_\mu\gamma_\nu~=~\frac{1}{4}g_{\mu\nu}
[/tex]

and so if the representation of the spinor basis is local or chart dependent one can pretty easily reproduce GR with the Dirac operator. A gauge invariant form of the Dirac operator would then be

[tex]
\partial_\mu(\gamma^\mu\psi)~=~\gamma^\mu D_\mu\psi~=~\gamma^\mu(\partial_\mu~+~A_\mu)\psi,
[/tex]

for [itex]A_\mu[/itex] a gauge term for GR.

For higher Clifford basis elements or with vierbiens extended GR theories can be derived. I suspect these are related in some ways to the string theory for GR which obtains for scales larger than the string length, but has deviations for scales approaching the string length. Of course there are some conformal invariance abuses with the string theoretic approach to GR as a bimetric form of theory. Yet string theory as a form of math-method does have some suggestive elements to it.

It is my sense that GR will survive to very high PN orders. I think deviations from GR obtain on two complementary scales: one scale near the Planck scale or say [itex]\le~10^3\sqrt{G\hbar/c^3}[/itex], and the other is on the cosmological scale where time translation invariance is "deformed" and there are inequivalent vacua states on scales across the cosmological event horizon. The verdict on this will likely come from gravity wave detection, such as LIGO, and the connection between these measurements with astrophysical events.

Lawrence B. Crowell
 
  • #546
Doug, I'm swamped right now with correspondence and I don't have internet connectivity at home so let me postpone writing more about what you've said here until later. But here's a link on another exponential gravitation theory. Can you talk about how this differs from your own?

[Uh, read down to the end of the article]
http://www.insidegnss.com/node/451

Carl
 
  • #547
lba7 said:
(translation from french observation)

This can explain deviation of light and redshift. The formula of perihelion precession of Mercury is the same with electrostatic forces integrate in the formula.

I have create a site for explain (in french for the moment) my ideas: 3w eisog dot com

Maybe this idea is not new, tell me ...

Ludovic

What is possible is that the spin quantum Hall effect might result in deviations from the equivalence principle. A circularly polarized photon as the superposition of two polarization states might be split by the effective index of refraction due to a gravity field. This would mean that gravitation has a Berry phase or a topological index associated with the spin of particles. This would be a possible deviation from classical general relativity.

An Einstein lens might provide the way to detect this. A radio telescope that detects photons from a lensed source will for a very narrow band pass filter measure quantum effect for entangled photons in this cosmic beam splitter. In principle the Wheeler Delayed Choice experiment could be performed this way. Also there might be for the two arms of this cosmic beam splitter a spin dependency in how the photons are split.

Lawrence B. Crowell
 
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  • #548
Making Everything Manifestly Covariant

Hello:

I can finally write about the New England American Physical Society Meeting on Saturday, April 5. Lut can skip this post since it involves the personal stories. The three posts that follow in quick succession will be technical calculations.

My hopes were not high for this local meeting at the Coast Guard Academy. It was held at a military facility, with an official entry gate. People were marching around all dressed to the military nines at 8 am. One positive aspect of the military is they get to wear sharp hats to work, hats that indicate one's station.

The usual cast of characters where at this APS meeting. There were a dozen people in the room, half of whom I was familiar with. The session started off with a familiar fringe guy. As far as I can tell, he claims that everything is in motion. As a skeptic, I attempt to see what notions I need to stretch to see some grain of truth in his near incomprehensible riffs. He claimed that everything was in motion. What I would say is everything moves in spacetime, mostly as time, as things continue to persist. He does make fun of himself a little which helps, otherwise his talks are tragic.

Larry Gold gave his "Let's doubt global warming". It reminds me of Fox News in the US which claims to be unbiased, then makes every effort to selectively sample data needed to support its position.

My talks was titled: "Using Quaternions for Lagrangians in EM and GEM Unified Field Theory." For an audience this tiny and quirky, I could not expect them to know about Lagrangians, or how to use them to derive field equations. I had thought about doing all the equations in LaTeX, but decided to use a fountain pen, good old black ink written by hand, to indicated that despite the complications, this sort of calculation can be done by a person. These sheets of paper packed full of partial differential equations are prized possessions. It looks so hard core. Two of these sheets - a derivation of the Maxwell equations from the Lagrangian, and a derivation of the gravity part of GEM - were at the core of the talk (the rest being a setup for the heavy duty math).

The talk had one technical glitch. My connecting wire is flaky so everything was yellow. Otherwise, the speech went according to plan. My talks often do not elicit questions, but this time someone started asking about the symmetric curl. It was like he was channeling Lawrence. He was wondering why I had all these coordinate dependent equations. After the session broke up, I asked him some more questions, trying to see what he found unsettling.

It certainly is my intension to write coordinate-independent equations that are valid in flat or curved spacetime. When I write a quaternion as "q", it could be in any coordinate system. When I write [itex]\nabla q[/itex], that is a covariant derivative, the same whether spacetime is flat or curved, independent of coordinates.

When I went to write out the derivative by its component parts, I invariably wrote things in terms of Cartesian coordinates, the rectilinear t, x, y, and z. The progression of symbols for derivatives goes something like this:

[tex]\frac{d}{dt} \rightarrow \frac{\partial}{\partial t} \rightarrow \nabla_0 \quad eq~1[/tex]

Only the last symbol is independent of coordinates, valid in flat or curved spacetime. I had never seen the Maxwell equations derived in a coordinate-free manifestly covariant way, so it was natural for me to just use partial derivatives with respect to t, x, y, and z.

Based on this criticism, I will be changing how I write component expressions. I will only use subscripts 0-3, not t-z. This way, equations that I think of as being manifestly covariant will have the notation required to be manifestly covariant.

For the record, I will repeat the quaternion operator derivations for the Maxwell equations, the gravity part of GEM, and the GEM unified field equations using the covariant notation in the next three posts.

Doug

Stills:
http://picasaweb.google.com/dougsweetser/MaxwellFieldEquations

The talk:
 
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  • #549
Hello:

In this post I will derive the Maxwell field equations using quaternion operators in a manifestly covariant notation.

Notice that the quaternion differential operator acting on a 4-potential creates a scalar gauge field, the -E and B fields:

[tex]\nabla A = (\nabla_0 \phi ~-~ \nabla \cdot A, \nabla_0 A ~+~ \nabla_u \phi ~+~ \nabla \times A) = (g, -E ~+~ B)\quad eq ~1[/tex]

The starting point for the derivation of the Maxwell equations is the Lagrangian which can be viewed as the difference between the scalars of B squared and E squared. This can be achieved by changing the order of the covariant differential operator with respect to the 4-potential, which flips the sign of the curl (B), but not the time derivative of A or gradient of phi which make up E. The scalar gauge field can be subtracted away:

[tex]-\frac{1}{8}(\nabla A ~-~ (\nabla A)^*)(A \nabla ~-~ (A \nabla)^*)[/tex]

[tex]=\frac{1}{8}(0, -\nabla_0 A ~-~ \nabla_u \phi ~-~ \nabla \times A)(0, \nabla_0 A ~+~ \nabla_u \phi ~-~ \nabla \times A)[/tex]

[tex]=\frac{1}{2}(0, E ~-~ B)(0, -E ~-~ B) = \frac{1}{2}(E^2 ~-~ B^2, -2 E \times B)\quad eq ~2[/tex]

Any expression derived from this one will be invariant under a scalar gauge transformation which uses the terms [itex]\nabla_0 \phi, \nabla \cdot A[/itex] because they have been explicitly subtracted away at this early stage. It is also of interest to know the 3-vector part of this expression is the Poynting vector, a conserved quantity in EM.

Write out the Lagrange density - the scalar part of eq 2 - in terms of its components, including the vector coupling, [itex]-\frac{1}{2 c}(J A + (J A)^*)[/itex]:


[tex]\mathcal{L}_{EB} = \frac{1}{2}(-(\nabla_1 \phi)^2 ~-~(\nabla_2 \phi)^2 ~-~(\nabla_3 \phi)^2 ~-~ (\nabla_0 A_1)^2 ~-~ (\nabla_0 A_2)^2 ~-~ (\nabla_0 A_3)^2[/tex]
[tex]~+~ (\nabla_3 A_2)^2 ~+~ (\nabla_2 A_3)^2 ~+~ (\nabla_1 A_3)^2 ~+~ (\nabla_3 A_1)^2 ~+~ (\nabla_2 A_1)^2 ~+~ (\nabla_1 A_2)^2)[/tex]
[tex]~-~ (\nabla_3 A_2)(\nabla_2 A_3) ~-~ (\nabla_1 A_3)(\nabla_3 A_1) ~-~ (\nabla_1 A_2)(\nabla_2 A_1) ~-~ (\nabla_1 \phi)(\nabla_0 A_1) ~-~ (\nabla_2 \phi)(\nabla_0 A_2) ~-~ (\nabla_3 \phi)(\nabla_0 A_3)[/tex]
[tex]-\rho \phi ~+~ J_1 A_1 ~+~ J_2 A_2 ~+~ J_3 A_3 \quad eq ~3[/tex]

Apply the Euler-Lagrange equation to this Lagrangian, treating the 4-potential as the variable:

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} \phi)}) = -\nabla_1^2 \phi ~-~ \nabla_2^2 \phi ~-~ \nabla_3^2 \phi ~-~ \nabla_0 \nabla_1 A_1 ~-~ \nabla_0 \nabla_2 A_2 ~-~ \nabla_0 \nabla_3 A_3 ~-~ \rho[/tex]
[tex]= \nabla \cdot E - \rho = 0 \quad eq ~4[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} A_1)}) = -\nabla_0^2 A_1 ~+~ \nabla_3^2 A_1 ~+~ \nabla_2^2 A_1 ~-~ \nabla_1 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_2 ~-~ \nabla_0 \nabla_1 \phi ~+~ J_1[/tex]
[tex]= \nabla_0 E_1 - (\nabla \times B)_1 + J_1 = 0 \quad eq ~5[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} A_2)}) = -\nabla_0^2 A_2 ~+~ \nabla_3^2 A_2 ~+~ \nabla_1^2 A_2 ~-~ \nabla_2 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_1 ~-~ \nabla_0 \nabla_2 \phi ~+~ J_2[/tex]
[tex]= \nabla_0 E_2 - (\nabla \times B)_2 + J_2 = 0 \quad eq ~6[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} A_3)}) = -\nabla_0^2 A_3 ~+~ \nabla_2^2 A_3 ~+~ \nabla_1^2 A_3 ~-~ \nabla_2 \nabla_3 A_2 ~-~ \nabla_1 \nabla_3 A_1 ~-~ \nabla_0 \nabla_3 \phi ~+~ J_3[/tex]
[tex]= \nabla_0 E_3 - (\nabla \times B)_3 + J_3 = 0 \quad eq ~7[/tex]

This work can be summarized with the Maxwell source equations:

[tex]\nabla \cdot E = \rho \quad eq 8[/tex]

[tex]\nabla \times B ~-~ \nabla_0 E = J[/tex]

This has been a manifestly covariant derivation of the Maxwell equations. This derivation remains the same in flat or curved spacetime, in Cartesian or spherical coordinates. Once you get used to keeping track of all these terms, it is kind of fun, honest!

Doug

Stills:
http://picasaweb.google.com/dougsweetser/MaxwellFieldEquations

The talk:
 
Last edited by a moderator:
  • #550
Covariat gravity field equation deivation

Hello:

In this post I will derive the Maxwell field equations using quaternion operators in a manifestly covariant notation.

Notice that the quaternion differential operator acting on a 4-potential creates a scalar gauge field, the -E and B fields:

[tex]\nabla A = (\nabla_0 \phi ~-~ \nabla \cdot A, \nabla_0 A ~+~ \nabla_u \phi ~+~ \nabla \times A) = (g, -E ~+~ B)\quad eq ~1[/tex]

The starting point for the derivation of the Maxwell equations is the Lagrangian which can be viewed as the difference between the scalars of B squared and E squared. This can be achieved by changing the order of the covariant differential operator with respect to the 4-potential, which flips the sign of the curl (B), but not the time derivative of A or gradient of phi which make up E. The scalar gauge field can be subtracted away:

[tex]-\frac{1}{8}(\nabla A ~-~ (\nabla A)^*)(A \nabla ~-~ (A \nabla)^*)[/tex]

[tex]=\frac{1}{8}(0, -\nabla_0 A ~-~ \nabla_u \phi ~-~ \nabla \times A)(0, \nabla_0 A ~+~ \nabla_u \phi ~-~ \nabla \times A)[/tex]

[tex]=\frac{1}{2}(0, E ~-~ B)(0, -E ~-~ B) = \frac{1}{2}(E^2 ~-~ B^2, -2 E \times B)\quad eq ~2[/tex]

Any expression derived from this one will be invariant under a scalar gauge transformation which uses the terms [itex]\nabla_0 \phi, \nabla \cdot A[/itex] because they have been explicitly subtracted away at this early stage. It is also of interest to know the 3-vector part of this expression is the Poynting vector, a conserved quantity in EM.

Write out the Lagrange density - the scalar part of eq 2 - in terms of its components, including the vector coupling, [itex]-\frac{1}{2 c}(J A + (J A)^*)[/itex]:

[tex]\mathcal{L}_{EB} = \frac{1}{2}(-(\nabla_1 \phi)^2 ~-~(\nabla_2 \phi)^2 ~-~(\nabla_3 \phi)^2 ~-~ (\nabla_0 A_1)^2 ~-~ (\nabla_0 A_2)^2 ~-~ (\nabla_0 A_3)^2[/tex]
[tex]~+~ (\nabla_3 A_2)^2 ~+~ (\nabla_2 A_3)^2 ~+~ (\nabla_1 A_3)^2 ~+~ (\nabla_3 A_1)^2 ~+~ (\nabla_2 A_1)^2 ~+~ (\nabla_1 A_2)^2)[/tex]
[tex]~-~ (\nabla_3 A_2)(\nabla_2 A_3) ~-~ (\nabla_1 A_3)(\nabla_3 A_1) ~-~ (\nabla_1 A_2)(\nabla_2 A_1) ~-~ (\nabla_1 \phi)(\nabla_0 A_1) ~-~ (\nabla_2 \phi)(\nabla_0 A_2) ~-~ (\nabla_3 \phi)(\nabla_0 A_3)[/tex]
[tex]-\rho \phi ~+~ J_1 A_1 ~+~ J_2 A_2 ~+~ J_3 A_3 \quad eq ~3[/tex]

Apply the Euler-Lagrange equation to this Lagrangian, treating the 4-potential as the variable:

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} \phi)}) = -\nabla_1^2 \phi ~-~ \nabla_2^2 \phi ~-~ \nabla_3^2 \phi ~-~ \nabla_0 \nabla_1 A_1 ~-~ \nabla_0 \nabla_2 A_2 ~-~ \nabla_0 \nabla_3 A_3 ~-~ \rho[/tex]
[tex]= \nabla \cdot E - \rho = 0 \quad eq ~4[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} A_1)}) = -\nabla_0^2 A_1 ~+~ \nabla_3^2 A_1 ~+~ \nabla_2^2 A_1 ~-~ \nabla_1 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_2 ~-~ \nabla_0 \nabla_1 \phi ~+~ J_1[/tex]
[tex]= \nabla_0 E_1 - (\nabla \times B)_1 + J_1 = 0 \quad eq ~5[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} A_2)}) = -\nabla_0^2 A_2 ~+~ \nabla_3^2 A_2 ~+~ \nabla_1^2 A_2 ~-~ \nabla_2 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_1 ~-~ \nabla_0 \nabla_2 \phi ~+~ J_2[/tex]
[tex]= \nabla_0 E_2 - (\nabla \times B)_2 + J_2 = 0 \quad eq ~6[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EB}}{\partial (\nabla_{\mu} A_3)}) = -\nabla_0^2 A_3 ~+~ \nabla_2^2 A_3 ~+~ \nabla_1^2 A_3 ~-~ \nabla_2 \nabla_3 A_2 ~-~ \nabla_1 \nabla_3 A_1 ~-~ \nabla_0 \nabla_3 \phi ~+~ J_3[/tex]
[tex]= \nabla_0 E_3 - (\nabla \times B)_3 + J_3 = 0 \quad eq ~7[/tex]

This work can be summarized with the Maxwell source equations:

[tex]\nabla \cdot E = \rho \quad eq ~8[/tex]

[tex]\nabla \times B ~-~ \nabla_0 E = J \quad eq ~9[/tex]

This has been a manifestly covariant derivation of the Maxwell equations. This derivation remains the same in flat or curved spacetime, in Cartesian or spherical coordinates. Once you get used to keeping track of all these terms, it is kind of fun, honest!

Doug

Stills:
http://picasaweb.google.com/dougsweetser/MaxwellFieldEquations

The talk:
 
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  • #551
Covariant GEM field equations

Hello:

<Preamble>
This post is very similar to the last two. This time I have few of the set of the last two, but unify gravity and EM in the process. Nice.
</Preamble>

In this post I will derive gravity and the Maxweill field equations using quaternion operators in a manifestly covariant notation.

The Hamilton representation will be used for the Maxwell field equations. The even representation of quaternions - where all signs are the same, and the Eivenvalues ore excluded so the quaternion can be inverted - will be used in the first phase of this derivation. What the even representation does is flip the relative signs of the E and B signs, so now the e filed has two signs, and the b field has one, like so:

[tex]E = -\nabla_0 A ~-~ \nabla_u \phi[/tex]
[tex]e = \nabla_0 A2 ~-~ \nabla_u \phi[/tex]

[tex]B_w = \nabla_u A_v ~-~\nabla_v A_u = \nabla \times A[/tex]
[tex]b_w = -\nabla_u A2_v ~-~\nabla_v A2_u = \nabla \Join A2 \quad eq ~0[/tex]

The fifth play is the term that makes up the gauge field:

[tex]g = \nabla_0 \phi ~-~ \nabla \cdot A[/tex]

None of these transform like tensors, but together they do from [itex]\nabla A[/itex].

Let's generate all 5 fields:

[tex]\nabla A = (\nabla_0 \phi ~-~ \nabla \cdot A2, \nabla_0 A2 ~+~ \nabla_u \phi ~+~ \nabla \times A) = (g, -E ~+~ B)[/tex]
[tex]\nabla^* A2 = (\nabla_0 \phi ~-~ \nabla \cdot A2, -\nabla_0 A2 ~+~ \nabla_u \phi ~-~ \nabla \Join A2) = (g, -e ~+~ b)\quad eq ~1[/tex]

The starting point for the derivation of the unified GEM equations is the Lagrangian which can be viewed as the difference between the scalars of E,b squared and B,e squared. This can be achieved by using the first set of quaternion operators used in the previous posts:

[tex]\frac{1}{8}((\nabla A)(A \nabla) ~-~(\nabla^* A2)(\nabla A2^*))[/tex]

[tex]=\frac{1}{8}(\nabla_0 \phi ~-~ \nabla \cdot A, \nabla_0 A ~+~ \nabla_u \phi ~+~ \nabla \times A)(\nabla_0 \phi ~-~ \nabla \cdot A, \nabla_0 A ~+~ \nabla_u \phi ~-~ \nabla \times A)[/tex]
[tex]-(\nabla_0 \phi ~-~ \nabla \cdot A, \nabla_0 A ~-~ \nabla_u \phi ~-~ \nabla \Join A)(\nabla_0 \phi ~-~ \nabla \cdot A, -\nabla_0 A ~+~ \nabla_u \phi ~-~ \nabla \Join A)[/tex]

[tex]=\frac{1}{2}(g, -E ~+~ B)(g, -E ~-~ B) ~-~ (g, e ~+~ b)(g, -e ~+~ b) = \frac{1}{2}(B^2 ~-~ E^2 ~-~ b^2 ~+~ e^2, 2 E \times B ~-~ b \Join b ~+~ e \Join e)\quad eq ~2[/tex]

Any expression derived from this one will be invariant under a scalar gauge transformation which uses the terms [itex]\nabla_0 \phi, \nabla \cdot A[/itex] because they have miraculously been cancelled!

Write out the Lagrange density - the scalar part of eq 2 - in terms of its components, including the vector coupling whose phase has spin 1 and spin 2 symmetry[/itex]:

[tex]\mathcal{L}_{EBeb} = -~(\nabla_3 A_2)(\nabla_2 A_3) ~-~ (\nabla_1 A_3)(\nabla_3 A_1) ~-~ (\nabla_1 A_2)(\nabla_2 A_1) ~-~ (\nabla_1 \phi)(\nabla_0 A_1) ~-~ (\nabla_2 \phi)(\nabla_0 A_2) ~-~ (\nabla_3 \phi)(\nabla_0 A_3)[/tex]
[tex]-\rho \phi ~+~ J_1 A_1 ~+~ J_2 A_2 ~+~ J_3 A_3 \quad eq ~3[/tex]

[sidebar: The assertion that the current coupling term has both spin 1 and spin 2 symmetry for all terms in the phase requires a small calculation. I decided to leave that as a problem. My guess is that until someone starts confirming these by hand, I'll be the only one to see that even these cool details work out.[/sidebar]

Apply the Euler-Lagrange equation to this Lagrangian, treating the 4-potential as the variable:

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EBeb}}{\partial (\nabla_{\mu} \phi)}) = - \nabla_0 \nabla_1 A_1 ~-~ \nabla_0 \nabla_2 A_2 ~-~ \nabla_0 \nabla_3 A_3 ~-~ \rho[/tex]
[tex]= -\frac{1}{2}\nabla \cdot (E ~-~ e) - \rho = 0 \quad eq ~4[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EBeb}}{\partial (\nabla_{\mu} A_1)}) = -~ \nabla_1 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_2 ~-~ \nabla_0 \nabla_1 \phi ~+~ J_1[/tex]
[tex]= \frac{1}{2}(\nabla_0 (E_1 ~+~ e_1) - (\nabla \times B)_1 - (\nabla \Join b)_1) + J_1 = 0 \quad eq ~5[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EBeb}}{\partial (\nabla_{\mu} A_2)}) = - \nabla_2 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_1 ~-~ \nabla_0 \nabla_2 \phi ~+~ J_2[/tex]
[tex]= \frac{1}{2}(\nabla_0 (E_2 ~+~ e_2) - (\nabla \times B)_2 - (\nabla \Join b)_2) + J_2 = 0 \quad eq ~6[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{EBeb}}{\partial (\nabla_{\mu} A_3)}) = - \nabla_2 \nabla_3 A_2 ~-~ \nabla_1 \nabla_3 A_1 ~-~ \nabla_0 \nabla_3 \phi ~+~ J_3[/tex]
[tex]= \frac{1}{2}(\nabla_0 (E_3 ~+~ e_3) - (\nabla \times B)_3 - (\nabla \Join b)_3) + J_3 = 0 \quad eq ~7[/tex]

This work can be summarized with the GEM gravity source equations:

[tex]\frac{1}{2} \nabla \cdot (E ~-~ e) = \rho \quad eq ~8[/tex]

[tex]\frac{1}{2}(\nabla \times B ~+~ \nabla \Join b - \nabla_0 (E ~+~ e)) = J \quad eq ~9[/tex]

This has been a manifestly covariant derivation. This derivation remains the same in flat or curved spacetime, in Cartesian or spherical coordinates.

I have spent the day trying get all the signs and factors right. If there are any questions, send me a private note, and I will recheck it. If needed, we can put up a new post.

Doug

Stills:
http://picasaweb.google.com/dougsweetser/MaxwellFieldEquations

The talk:

(this derivation was not part of the talk)
 
Last edited by a moderator:
  • #552
Covariant gravity field equations

Hello:

<Preamble>Looks like two of my posts were identical, sorry. The software here doesn't appear to like this much LaTeX.

This post is very similar to the last. I am starting out the draft by cutting and pasting the text, as all the same terms are the same. used in the same locations of the same equations. What changes are a few signs. The E field is made of two parts, [itex]-\nabla A_0[/itex] and [itex]-\nabla \phi[/itex]. These happen to have the same sign. In this post, the case where these have opposite signs will be explored. A similar thing will be done for the magnetic field, where the two terms [itex]\nabla_u A_v[/itex] and [itex]\nabla_v A_u[/itex] have the same sign.

Those readers concerned about how these objects transform can rest easy. We know that [itex]\nabla A[/itex] transforms like a rank 2 tensor - it was the justification behind developing the covariant tensor [itex]\nabla[/tex] in the first place. We also know that the EM field strength tensor, [itex]\frac{1}{2}(\nabla_u A_v - \nabla_v A_u)[/itex], transforms like a tensor. The difference between these two tensors which is [itex]\frac{1}{2}(\nabla_u A_v + \nabla_v A_u)[/itex], also transforms like a tensor since the difference of two tensors remains a tensor.
</Preamble>

In this post I will derive the gravity part of the GEM proposal using quaternion operators in a manifestly covariant notation.

The even representation of quaternions - where all signs are the same, and the Eivenvalues ore excluded so the quaternion can be inverted - will be used in the first phase of this derivation. What the even representation does is flip the relative signs of the E and B signs, so now the e filed has two signs, and the b field has one, like so:

[tex]E = -\nabla_0 A ~-~ \nabla_u \phi[/tex]
[tex]e = \nabla_0 A2 ~-~ \nabla_u \phi[/tex]

[tex]B_w = \nabla_u A_v ~-~\nabla_v A_u = \nabla \times A[/tex]
[tex]b_w = -\nabla_u A2_v ~-~\nabla_v A2_u = \nabla \Join A2 \quad eq ~0[/tex]

None of these transform like tensors, but together they do from [itex]\nabla A[/itex].

Notice that the quaternion differential operator acting on a 4-potential creates a scalar gauge field, and two fields the -e and b fields:

[tex]\nabla^* A2 = (\nabla_0 \phi ~-~ \nabla \cdot A2, \nabla_0 A2 ~-~ \nabla_u \phi ~-~ \nabla \Join A2) = (g, e ~+~ b)\quad eq ~1[/tex]

The starting point for the derivation of the GEM gravity equations is the Lagrangian which can be viewed as the difference between the scalars of b squared and e squared. This can be achieved by changing the order of the conjugation operator with respect to the 4-potential, which flips the sign of the time derivative of A and gradient of phi which make up e, but not the symmetric curl b. The scalar gauge field can be subtracted away:

[tex]\frac{1}{8}(\nabla^* A2 ~-~ (\nabla^* A2)^*)(\nabla A2^* ~-~ (\nabla A2^*)^*)[/tex]

[tex]=\frac{1}{8}(0, \nabla_0 A ~-~ \nabla_u \phi ~-~ \nabla \Join A)(0, -\nabla_0 A ~+~ \nabla_u \phi ~-~ \nabla \Join A)[/tex]

[tex]=\frac{1}{2}(0, e ~+~ b)(0, e ~-~ b) = \frac{1}{2}(b^2 ~-~ e^2, b \Join b ~-~ e \Join e)\quad eq ~2[/tex]

Any expression derived from this one will be invariant under a scalar gauge transformation which uses the terms [itex]\nabla_0 \phi, \nabla \cdot A[/itex] because they have been explicitly subtracted away at this early stage. It is also of interest to think about the properties of the 3-vector, since in the EM case it was the Poynting vector.

Write out the Lagrange density - the scalar part of eq 2 - in terms of its components, including the vector coupling, [itex]-\frac{1}{2 c}(J A2* + (J A2^*)^*)[/itex]:

[tex]\mathcal{L}_{eb} = \frac{1}{2}((\nabla_1 \phi)^2 ~+~(\nabla_2 \phi)^2 ~+~(\nabla_3 \phi)^2 ~+~ (\nabla_0 A_1)^2 ~+~ (\nabla_0 A_2)^2 ~+~ (\nabla_0 A_3)^2[/tex]
[tex]~-~ (\nabla_3 A_2)^2 ~-~ (\nabla_2 A_3)^2 ~-~ (\nabla_1 A_3)^2 ~-~ (\nabla_3 A_1)^2 ~-~ (\nabla_2 A_1)^2 ~-~ (\nabla_1 A_2)^2)[/tex]
[tex]~-~ (\nabla_3 A_2)(\nabla_2 A_3) ~-~ (\nabla_1 A_3)(\nabla_3 A_1) ~-~ (\nabla_1 A_2)(\nabla_2 A_1) ~-~ (\nabla_1 \phi)(\nabla_0 A_1) ~-~ (\nabla_2 \phi)(\nabla_0 A_2) ~-~ (\nabla_3 \phi)(\nabla_0 A_3)[/tex]
[tex]-\rho \phi ~+~ J_1 A_1 ~+~ J_2 A_2 ~+~ J_3 A_3 \quad eq ~3[/tex]

Apply the Euler-Lagrange equation to this Lagrangian, treating the 4-potential as the variable:

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{eb}}{\partial (\nabla_{\mu} \phi)}) = \nabla_1^2 \phi ~+~ \nabla_2^2 \phi ~+~ \nabla_3^2 \phi ~-~ \nabla_0 \nabla_1 A_1 ~-~ \nabla_0 \nabla_2 A_2 ~-~ \nabla_0 \nabla_3 A_3 ~-~ \rho[/tex]
[tex]= -\nabla \cdot e - \rho = 0 \quad eq ~4[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{eb}}{\partial (\nabla_{\mu} A_1)}) = \nabla_0^2 A_1 ~-~ \nabla_3^2 A_1 ~-~ \nabla_2^2 A_1 ~-~ \nabla_1 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_2 ~-~ \nabla_0 \nabla_1 \phi ~+~ J_1[/tex]
[tex]= \nabla_0 e_1 - (\nabla \Join b)_1 + J_1 = 0 \quad eq ~5[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{eb}}{\partial (\nabla_{\mu} A_2)}) = \nabla_0^2 A_2 ~-~ \nabla_3^2 A_2 ~-~ \nabla_1^2 A_2 ~-~ \nabla_2 \nabla_3 A_3 ~-~ \nabla_1 \nabla_2 A_1 ~-~ \nabla_0 \nabla_2 \phi ~+~ J_2[/tex]
[tex]= \nabla_0 e_2 - (\nabla \Join b)_2 + J_2 = 0 \quad eq ~6[/tex]

[tex]\nabla_{\mu}(\frac{\partial \mathcal{L}_{eb}}{\partial (\nabla_{\mu} A_3)}) = \nabla_0^2 A_3 ~-~ \nabla_2^2 A_3 ~-~ \nabla_1^2 A_3 ~-~ \nabla_2 \nabla_3 A_2 ~-~ \nabla_1 \nabla_3 A_1 ~-~ \nabla_0 \nabla_3 \phi ~+~ J_3[/tex]
[tex]= \nabla_0 e_3 - (\nabla \Join b)_3 + J_3 = 0 \quad eq ~7[/tex]

This work can be summarized with the GEM gravity source equations:

[tex]-\nabla \cdot e = \rho \quad eq ~8[/tex]
[tex]\nabla \Join b - \nabla_0 e = J \quad eq ~9[/tex]

This has been a manifestly covariant derivation. This derivation remains the same in flat or curved spacetime, in Cartesian or spherical coordinates. Once you get used to keeping track of all these terms, it is kind of fun, honest!

Doug

Stills:
http://picasaweb.google.com/dougsweetser/MaxwellFieldEquations

The talk:
 
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  • #553
Hatch's work on an exponential force equation

Hello Carl:

Ronald Hatch sent me his paper which has an exponential in the force equation. For me as a member of the ultra-conservative fringe, it was not a happy read. He did not define a Lagrangian, so the proposal felt ad hoc. The way to get the force equation is to vary the Lagrangian with respect to velocity.

He thinks there is an absolute ether which strikes me as wrong.

He wants to give up the equivalence principle. His logic for this struck me as muddled. The discussion of mass was particular confusing. It looked like he had the classic self-taught blindspot vis-a-vis E=mc2, that the real relation is between the invariant m2 c4 and the square of the covariant 4-momentum, E2 - P2 c2. One of his equations looked like a trivial rearrangement of terms, a rearrangement he took seriously.

The precession of the perihelion of Mercury is a tough calculation. He wanted to add a second order effect in as if it was a first order effect.

By a strict application of the rules for the Independent Research area of Physics Forums, I don't think his work would be accepted. I forwarded my concerns to him directly, but he said I needed to think about things more carefully. The paper is published in Physics Essays.

Doug
 
  • #554
Seeing spin 1 and spin 2 symmetry

Hello:

I exchanged a dozen emails with Steve Carlip over the coupling current [itex]J^{\mu} A_{\mu}[/itex]. The discussion started this way: "I have thought about Feynman's analysis of the spin of the vector current coupling." This post represents the back story, what I got from looking at chapter 3, pages 29-39 for about three to four weeks.

The first thing I did was work on my speed of going through the algebra in section 3.2, "Amplitudes and polarizations in electrodynamics, our typical field theory". You can only motor if you are confident about all the steps, just like in video games. The logic runs like this:

1. Start with the current-potential contraction.
2. Take the Fourier transformation of the 4-potential to get a current.
3. Simplify the current-current interaction along one axis, z.
4. Write out the contraction in terms of its components.
5. Use charge conservation to eliminate one term.
6. One term is the standard Coulomb interaction, the others are the relativistic corrections.

Then Feynman wants to know what that correction term is. This is were it gets a little odd. He talks about plane polarized light, and how looking at that you can see the angular momentum projections. I admit, I never quite saw those. What I did instead was try to strip away all the physics-speak, and just find the kernel of math underlying the operation. Looking back, that is what took the time: reducing the physics to a simple math expression. The Rosetta stone was a line on page 39:
Feynman said:
...we know that [itex](x ~\pm ~ i y)(x ~\pm~ i y)[/itex] are evidently of spin 2 and projection [itex]\pm 2[/itex]; these products are [itex](xx ~-~ yy ~\pm~ 2 i xy)[/itex], which have the same structure as our terms (3.4.1)

This is the pure math way to spot a system with spin 2: start with the product of two complex numbers, and check that the imaginary part has a 2ixy. This will require a change in x of pi radians to get back to the start point since there is an multiplier of 2. To speak like Feynman, I should talk up the projection operators, but I like to keep the math kernel free of that jargon.

Looking back on an earlier calculation, I was able to transcribe an earlier bit of algebra into a similar set of complex numbers:

[tex](x ~\pm ~ i y)(x' ~\pm~ i y')^* = (xx' ~+~ yy' ~+~ (yx' ~-~ xy') i \quad eq~1[/tex]

This is a system which has spin 1 projection operators, to use physics-speak. In math terms, the xy' does not help out the yx', there are no factors of 2 or 1/2, so this would take 2 pi radians to get the imaginary part of this back to where it was.

In terms of the math, the difference between a spin 1 system (eq 1) and a spin 2 system (see the quote) is no more complicated than looking at the imaginary part of a complex product.

Doug
 
  • #555
Feynman, Steve Carlip, and I

Hello:

I have the exchange of emails between Prof. Steve Carlip and myself up on the screen. It is not easy for me to read. Steve is a professional, I am not. On occasion, I babble. Babbling is a form of exploring, a process used to learn how to speak a language like a native. Studies have shown that deaf children do so learning sign language, and that baby birds do so before they can sing exactly like adults do. Recognizing this process, I have great patience for others that babble physics. Steve probably is that way in the right context, but in this email exchange, I got the book tossed at my head.

The discussion began with a http://picasaweb.google.com/dougsweetser/SpinAndPhaseOfCurrentCoupling/photo#5196141258835741330 . I went by the book, section 3.2 of Feynman's lectures, for three of four steps:

1. Start with the coupling term, [itex]J^{\mu} A_{\mu}[/itex].

2. Take the Fourier transformation, [itex]J^{\mu} A_{\mu} = -\frac{1}{K^2} J^{\mu} J'_{\mu} \quad eq~3.2.2[/itex]

3. Write out 2 in terms of the components:
[tex]J^{\mu} A_{\mu} = -\frac{1}{K^2}(\rho \rho' - J_1 J'_1 - J_2 J'_2 - J_3 J'_3 ) \quad eq~3.2.5[/tex]

[Note on imprecise notation: in the slide I use x, y, and z which imply a coordinate choice. I should have used numbers for subscripts. I also didn't toss in the minus sign as Feynman does for the Fourier transformation step.]

Up to this point, I have exactly walked down the path Feynman wrote about. When it came to writing up the slides, I initially put in a further step Feynman used: he imagines picking a coordinate system such that all the current goes along one direction (the 3 axis). Everyone is accustom to this step. Yet it bothered me. I would have to rewrite the derivation if someone chose the 2 axis instead. A more general position would involve choosing no axis, yet spotting the symmetries of the spin in the phase anyway. I decided to work with that as a goal.

4. Multiply out the two currents as quaternions:

-J J' = (-rho rho' + J1 J'1 + J2 J'2 + J3 J'3,

-rho J'1 - J1 rho' - J2 J'3 + J3 J'2,

-rho J'2 - J2 rho' - J3 J'1 + J1 J'3,

-rho J'3 - J3 rho' - J1 J'2 + J2 J'1)The terms in italics are equation 3.2.5, the underlined terms are in an expression about spin 2 symmetry on page 39, and the terms in bold are in 3.2.10 in a discussion of spin 1 symmetry.

Steve had no idea what I was doing, none. Communication was broken by step 4. I was at work, trying to do my job, or appear to be doing my job, and quickly come up with a response to someone with far more intellectual precision. It did not work out so well. The worse thing I did was about equation 3.2.10 concerning circularly polarized light. Feynman writes out the currents for two circularly polarized light whose imaginary parts cancel. I got a sign wrong, so they didn't cancel, and I got to look stupid.

Both Steve and Feynman talked about projection operators, the relevant machinery from quantum field theory. I did not talk about projection operators at all. I am not going to do so now since I would probably just babble about them. I understand why the well-trained would say that if I don't discuss projection operators intelligently, then this has nothing to do with the spin of particles. Nothing. For me, projection operators are a patina on the underlying algebra (patina def.: the sheen on the surface of an old object, caused by age and much handling).

Steve left the discussion convinced I didn't even understand the basics of spin in physics. He won the word game, but the algebra in step 4 still stands consistent with what Feynman wrote. At the end of the day, algebra trumps words.

Doug
 
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  • #556
Three new bits of math

Hello:

Preparing for my talk in Brazil, I had an interesting insight. The thesis behind "Doing Physics with Quaternions" at quaternions.com is that physics describes patterns of events in spacetime using quaternions up to an isomorphism. Most of physics works great without quaternions because the quaternion expression would not provide new information.

My epiphany was this: new quaternion math equals new physics. Here in this thread, the new math is the Even representation for quaternions (a reinvention of Clyde Daven's hypercomplex numbers). The current coupling J2 A2 has the spin 2 symmetry in the phase, and the field strength tensor [itex]\nabla A2[/itex] contains the symmetric curl needed for the symmetric field b.

I have also mentioned here the work in animating quaternions which lead to an understanding why the groups U(1), SU(2), SU(3) and Diff(M) must be all that makes up the symmetry forces of Nature. With the visual perspective, the forces are more tightly linked algebraically. The standard model is written as U(1)xSU(2)xSU(3), which would have 1+3+8=12 generators for its Lie algebra. One mystery of the standard approach is why the electro and weak forces should team up to form the electroweak force. Another mystery is why should confinement exist for the strong force SU(3)? These phenomena are suggesting something more like [U(1)xSU(2)]xSU(3) than three equal players. That is what happens with the quaternion representation of the symmetry of forces:

[tex]A^* B = (\frac{A}{|A|} exp (A - A^*))^* (\frac{B}{|B|} exp (B - B^*))\quad eq~1[/tex]

which is (U(1) SU(2))*(U(1) SU(2)). The Lie algebra only has 8 generators. This smaller model has a chance to provide a cause for the confinement of quarks.

The third quaternion math innovation I do not talk about much because I have yet to see how it impacts a calculation, although it helps with a big riddle, a "why" question, in physics. Many who work with quaternion derivatives accept the idea of a left handed versus right handed derivative. This comes from the limit definition, putting the differential on the left or right. This definition is ineffective since one cannot show that a function as simple as f(q)=q2 is analytic in q. For me that indicates the definition has no utility. What I did was steal a move from L'Hospital's rule and use a dual limit process. Let the pesky 3-vector with its three imaginary basis vectors go to zero first, leaving only the real number which commutes with all. Effectively this is a directional derivative along the real axis. Things work out great for proofs using this definition (if one is good at doing proofs, which I am not). All events are ordered by the real scalar. If this definition is applied to events in spacetime, the scalar is time, and thus all the events are order in time like a movie.

What happens when the limit processes are reversed, and the pesky 3-vector goes to zero after the scalar gets frozen? All one can do in this case is to determine the norm of the derivative. Although not well known, there is a branch of math that studies norms of derivatives. I think this is the domain of quantum mechanics. We cannot order things in time, but we can tell on average how much change is going to happen after making many measurements.

Now to make the slides...
Doug
 
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  • #557
but when doing the product of quaternions if Q is a quaternion then where you put [tex] Q.Q=Q^{2} [/tex] it should read [tex] Q.Q^{*} [/tex] , for example for Minkowsky metric

[tex] dQ=dt-idx-jdy-kdz [/tex] then [tex] ds^{2}=(dQ).(dQ^{*})=dt^{2}-dx^{2}- dy^{2}-dz^{2} [/tex]

and as i pointed in other part of the forum, you have the problem of non-commutativity so

[tex] ij(dx.dy)=-ji (dy.dx) [/tex],

anyway the idea seems very interesting
 
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  • #558
The Even representation

Hello mhill:

In the standard Hamilton representation, for a quaternion dQ = (c dt, dx, dy, dz) we have the product:

[tex]dQ dQ = (c^2 dt^2 ~-~ dx^2 ~-~ dy^2 ~-~ dz^2, 2 c ~dt~ dx, 2 c~ dt~ dy, 2 c ~dt~ dz)\quad eq~1[/tex]

When one uses tensors, the Einstein summation convention ignores the three other terms. That is a mistake in my opinion. One thing I have noticed about the GEM proposal: the 3-vector (2 dt dx, 2 c dt dy, 2 c dt dz) is an invariant in the presence of a gravitational source. That is really cool because special relativity is about the invariant scalar, and for GEM, gravity is about the invariance of the 3-vector.

If we look at the product of two quaternions that are nearby each other, a dQ and dQ', we get a similar result with a cross product:

[tex]dQ dQ' = (c^2~ dt~ dt' ~-~ dx~ dx' ~-~ dy~ dy' ~-~ dz ~dz',[/tex]
[tex]c~ dt ~dx' ~+~ c ~dx~ dt' ~+~ dy ~dz' ~-~ dz~ dy',[/tex]
[tex]c ~dt ~dy' ~+~ c ~dy ~dt' ~+~ dz ~dx' ~-~ dx ~dz',[/tex]
[tex]c ~dt ~dz' ~+~ c ~dz ~dt' ~+~ dx ~dy' ~-~ dy ~dx')\quad eq~2[/tex]

Hamilton could have done that one, so this is not new math. For the Even representation of quaternions, the rules are easy to remember: everything is sunny and positive in California, and so it goes for the Even representation:

[tex]i^2 = j^2 = k^2 = ijk = 1\quad eq~3[/tex]

[tex]ij = ji = k \quad eq~4[/tex]

[tex]ik = ki = j \quad eq~5[/tex]

[tex]jk = kj = i \quad eq~6[/tex]

There is not a minus sign to write. This will be a division algebra if and only if the eigenvalues of the real 4x4 matrix representation are excluded from the set of quaternions.

There will be math wonks who insist that the name "quaternions" is reserved for non-commutative 4D division algebras. Historically, that has been the use. Doing new math can cause conflict, so be it. The non-commutative aspect is a result of an arbitrary choice in how to represent a 4D division algebra. I have chosen a different representation. It still is a division algebra, but one where multiplication commutes. Clyde Daven did this first and called them hypercomplex numbers. That makes them sound like a separate animal, and I don't think it is. This is representation theory in practice, applied to quaternions.

To indicate the Even representation is being used, I toss in a "2" every now and then. Repeat eq. 1 with the even representation:

[tex]dQ2^* dQ2 = (c^2 ~dt^2 ~-~ dx^2 ~-~ dy^2 ~-~ dz^2, - 2~ dy ~dz, - 2 ~dx ~dz, - 2 ~dx ~dy)\quad eq~7[/tex]

The scalar is the same, but the 3-vector has changed. Instead of rescaling the (dx, dy, dz) by a 2 dt factor, this time it is all about the symmetric curl. The dt factor does not make it into the 3-vector.

Repeat the dQ2 dQ2' in the Even representation:

[tex]dQ2^* dQ2' = (c^2 ~dt ~dt' ~-~ dx ~dx' ~-~ dy ~dy' ~-~ dz ~dz',[/tex]
[tex]c ~dt ~dx' ~-~ c ~dx ~dt' ~-~ dy ~dz' ~-~ dz ~dy',[/tex]
[tex]c ~dt ~dy' ~-~ c ~dy ~dt' ~-~ dz ~dx' ~-~ dx ~dz',[/tex]
[tex]c ~dt ~dz' ~-~ c ~dz ~dt' ~-~ dx ~dy' ~-~ dy ~dx')\quad eq~8[/tex]

If dQ2' where to get acted on by the conjugate operator instead of dQ2, then the only terms to flip signs involve dt dR.

What makes the Even representation interesting is it gives a more complete way of viewing a quaternion product. In the Hamilton representation, the rescaling (dt dR) was unaltered by changing the order of multiplication, while the cross product flipped signs. In the Even representation, the symmetric curl is unaltered by changing the order of conjugation, while the rescaling flips signs. The scalar remains steady no matter what. That sounds like a more complete survey of the product of two sets of four numbers.

Doug
 
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  • #559
Pitching the program

Hello:

I spend time and effort pitching this research project to both the upper elite and the technical masses. I took off a Wednesday from work to see a talk by Nobel Laureate Sheldon Glashow, who got one in the 70s for the electroweak theory. I told him I had an animation for U(1)xSU(2) on my MacBook Pro. He was too busy to look right then, but I could send him an email, which I did.

Later that evening, Michio Kaku was doing book promo work. He agreed to sign his latest book, "Physics of the Impossible", which is doing well on the New York Times Best Seller list. I got in line late, and the book was sold out by the time I got there. I bought a different book, and had him sign "Maxwell is the best!" I also dropped off a version of my proposal where I derive the Maxwell equations first - to established I am much better than your average crank - and with a variation get equations for a metric approach to gravity. He thanked me as he went on to sign another book.

Max Tegmark gave a talk on the Physics of Super Heroes, along with a screening of Superman. He is a big survey astronomer by day, so it was fun to cruise through the known Universe with his software. He knew me from a previous outreach program he did, and had traded a few stories back then about quaternions. I told him of the quaternion animation project, how it could be found on YouTube with a search for "Quaternions Standard Model". I gave him a business card with the search instructions after my 20 second pitch.

Low odds on getting a reply from these busy folks, but I need to try, so I do.

There are many more folks who read a high traffic site such as slashdot.com They had an article on Lectures On the Frontiers of Physics Online. Buch of big names in physics have videos up there:
Neil Turok's 'What Banged?,' John Ellis with 'The Large Hadron Collider,' Nima Arkani-Hamed with 'Fundamental Physics in 2010,' Paul Steinhardt with 'Impossible Crystals,' Edward Witten with 'The Quest for Supersymmetry,' Seth Lloyd with 'Programming the Universe,' Anton Zeilinger with 'From Einstein to Quantum Information,' Raymond Laflamme with 'Harnessing the Quantum World,'

You might be able to see the site in a day or two here, http://perimeterinstitute.ca/index.html

So I posted a note there which reflects my current thoughts:


Title: Maxwell Trumps General Relativity

General Relativity rocks. It is elegant in its minimialism. All efforts to add a little extra have failed, usually by allowing a dipole gravity wave mode of emission which has been ruled out by binary pulsar data.

The only field theory that is manifestly better than GR is the Maxwell field equations. Every time we have added to it in the name of symmetry, the theory has done more. James did it himself by tacking on the Ampere current. Einstein looked to get rid of a duplicate law, and so special relativity was born. With the huge supply of new particles coming out of atom smashers, the gauge symmetry in EM (U(1)) was expanded to SU(2) for the weak force, and SU(3) for the strong.

None of those smart cats listed in the initial post will be talking about the Maxwell equations. Too bad, the history of physics is clear: expand Maxwell, you win.

Max depends on the field strength tensor d_u A_v - d_v A_u. There is a subtraction in there, a great thing (called an exterior derivative). But in the name of symmetry, we need to work with the rest of it, d_u A_v + d_v A_u. Do that right, and you get a unified field theory that Einstein failed to find by looking for workable extensions of GR. Extend Max, not GR.

If anyone here wants to see the nuts and bolts of deriving the Maxwell equations using the Euler-Lagrange equations, search for "GEM action" on YouTube. A small variation - two minus signs - on the Maxwell equations leads to equations for gravity. Yes, I show that there is a metric solution (the Rosen metric if you are up on your GR jargon, a bunch of exponentials if not). Yes I know there is an issue of spin 1 and spin 2 which can be addressed if you get what the phase of current coupling really is.

YouTube can survive being slashdotted.

Doug
 
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  • #560
Brazil Talk Video

Hello:

I am about to power down the laptop and get it ready for a trip to a foreign land. I will be giving this Thursday, May 29, in Campinas, Brazil at 5:30 pm. Stop by if you are in town. Since I figure about zero of you can do that, I just uploaded a video of the talk to YouTube. The video is 41 minutes long, but I only have a 25 minute slot, so I will have to be more efficient. As always, critiques are appreciated.

I really like the central thesis: that only by doing new math can I do new physics. Will report back on if I can get others excited by this work.

Doug
 

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