New paper about No Dark Matter

In summary, J.W. Moffat's paper discusses the effects of Einstein gravity coupled to a massive skew symmetric field and its implications for gravitational theory. Using non-perturbative renormalization group equations and observational input, special trajectories are characterized to allow for the running of the effective gravitational coupling and the coupling of the skew field to matter. These findings show an increase in Newton's constant at large galactic and cosmological distances, which can explain the flat rotation curves of galaxies without the need for exotic dark matter. The equations of motion for test particles also yield predictions that agree with observations. The paper also addresses the issue of gravitational lensing without dark matter and the possibility of a variable G that can explain the data without assuming the existence of
  • #1
marcus
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Gravitational Theory, Galaxy Rotation Curves and Cosmology without Dark Matter
J. W. Moffat
http://arxiv.org/abs/astro-ph/0412195

"Einstein gravity coupled to a massive skew symmetric field [tex]F_{\mu\nu\lambda}[/tex] leads to an acceleration law that modifies the Newtonian law of attraction between particles. We use a framework of non-perturbative renormalization group equations as well as observational input to characterize special renormalization group trajectories to allow for the running of the effective gravitational coupling G and the coupling of the skew field to matter. The latter lead to an increase of Newton's constant at large galactic and cosmological distances. For weak fields a fit to the flat rotation curves of galaxies is obtained in terms of the mass (mass-to-light ratio M/L) of galaxies. The fits assume that the galaxies are not dominated by exotic dark matter and that the effective gravitational constant G runs with distance scale. The equations of motion for test particles yield predictions for the solar system and the binary pulsar PSR 1913+16 that agree with the observations. The gravitational lensing of clusters of galaxies can be explained without exotic dark matter. An FLRW cosmological model with an effective G=G(t) running with time can lead to consistent fits to cosmological data without assuming the existence of exotic cold dark matter."

31 pages, 20 figures
many of the figures show galaxy rotation curve fits
 
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  • #2
I will turn you to the dark side of the force (polarized ZPE fields as the source of gravitation and inertia). :tongue2: I truly wish I had the math skills to express the effects I see in my thought experiments with this model. As a VERY crude analogy, imagine a bunch of little bar magnets thrown on a slippery table top. They will immediately clump in a way that represents the lowest potential energy state acheivable from that initial state. (less suspense, more closure, in a sociological analogy) I believe the ZPE fields do this as well, and the attraction expressed in the binding of the lowest potential energy state is what we call gravity.
 
  • #3
I'm not comfortable with Moffat's explanation. Unless I made an OOM error, the effects he describes would have measurable effects on planetary orbits within our solar system. Futhermore, I do not see how it addresses the resulting flatness problem of spacetime curvature.
 
  • #4
I cannot claim to understand this paper, but it appears that G=Go within the solar system but runs up to G=6Go at larger scales, so that planet trajectories are not affected, but the amount of dark matter is replaced by a variable G.

So it appears that the introduction of variability in distance and time to the gravitational constant plus non-symetric gravity theory can fit all observed phenomena including a flat spacetime curvature and gravitational lensing.

So my question is, what gives us the right to make G variable? Is it not possible that the variable G is just a curve fit to actual Dark Matter. Is there some other process that could make G variable. Is there some way to observe if that is true. Is the theory falsifiable or just a model?

I quess that Occums razor applies. Both invisible energy and matter, and a variable G, can explain the data. But invisibility is preferred to variability.

Richard
 
  • #5
Agreed yanniru. It does appear local solar system dynamics are not distinguishable from GR predictions under the NGT model. I'm curious why no mention was made of the pioneer anomaly. It was also unclear how combining GR with a skew symmetric rank 3 tensor field invoking a 'fifth force' coupling constant produces a simpler gravitational theory. The variance of G over time was intriguing, yet unexplained. G is initially low and remains constant for about 10,000 years, then suddenly climbs to the present, much higher value by the time the universe is 1,000,000 years old. The absence of an explanation for this phenomenon, it looks like hand tuning to get a .04 baryonic density in the primordial universe and a .24 baryonic density after 1,000,000 years. That was a bit hard to swallow.
 
  • #6
When the current theory has issues, everything is on the table.

Invisible matter in and of itself, isn't much of a theoretical stretch. Requiring 80%+ of all matter in the universe to be non-baryonic, despite the fact that there is not yet a single direct observation of non-baryonic matter, is a stretch. If the stuff makes up so much of all matter, one needs a pretty good reason for explaining why no one has ever come across a chunk of the stuff.

Moffat, Mannheim, and Milgrom-Bekenstein all illustate that it is possible to devise modifications of GR and more specifically of gravity, which eliminate the vast majority of the implication of dark matter. Indeed, there are at least three similar, but not identical ways, to do so.

Moreover, these M^3 scholars also illustrate an additional limitation on any viable CDM theory. Not only must it find non-baryonic matter not yet observed to account for the vast majority of the matter in the universe, it most also explain why the distribution of that matter is so tightly fine tuned to the visible light in the galaxies observed, so as to fit M^3 predictions. In a CDM context, this has to be done more or less entirely through the galaxy formation process, as CDM interacts only through standard GR gravity. A satisfactory and coherent theory to explain the incredible coincidence of galaxy formation that distributed CDM in this way has not emerged to my knowledge.

A G constant that runs with time is certainly the most worrisome aspect of the Moffat approach, but there is a very well documented phenomena out there and CDM as a solution has serious issues.
 
  • #7
ohwilleke said:
Moreover, these M^3 scholars also illustrate an additional limitation on any viable CDM theory. Not only must it find non-baryonic matter not yet observed to account for the vast majority of the matter in the universe, it most also explain why the distribution of that matter is so tightly fine tuned to the visible light in the galaxies observed, so as to fit M^3 predictions. In a CDM context, this has to be done more or less entirely through the galaxy formation process, as CDM interacts only through standard GR gravity. A satisfactory and coherent theory to explain the incredible coincidence of galaxy formation that distributed CDM in this way has not emerged to my knowledge.
This is where my ZPE model shines. There is no need to invoke special distributions of CDM. The visible matter, gas and dust that we observe (plus any dark baryonic matter that we can't sense easily) are sufficient to cause the gravitational effects that we see, like cluster binding and lensing. Masses polarize the ZPE EM fields, and the local interaction of masses with the polarized vacuum fields is gravitation. Space-time in this model is flat, and gravitational lensing is a purely optical effect of EM waves propagating through densified polarized EM vacuum fields. The concept of photons following geodesics in space-time is eliminated. GR's space-time curvature is a great mathematical approximation of gravitation in simple systems, like our solar system, but it breaks down on galactic scales, which is why CDM has to be invoked to keep the standard model chugging along.
 

1. What is the main finding of the new paper about No Dark Matter?

The main finding of the paper is that the observed gravitational effects in galaxies can be explained by the laws of gravity rather than the existence of dark matter.

2. How does this new paper challenge the current understanding of dark matter?

This paper challenges the current understanding of dark matter by proposing an alternative explanation for the observed gravitational effects in galaxies, without the need for dark matter particles.

3. What evidence does the new paper provide for its claims?

The new paper provides evidence from computer simulations and observations of galaxies that support the idea that the laws of gravity alone can explain the observed gravitational effects.

4. Does this mean that the concept of dark matter is no longer relevant?

No, this paper does not completely dismiss the concept of dark matter. It simply presents a different perspective and proposes that the observed phenomena can be explained without the need for dark matter particles.

5. What are the implications of this new research for future studies on dark matter?

This new paper opens up new avenues for research and encourages scientists to continue exploring alternative explanations for the observed gravitational effects in galaxies. It also highlights the need for further studies and observations to fully understand the nature of dark matter.

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