Could gravity be an emergent property of nature?

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Sorry if this question is naive. It is just a curiosity that I have.

Are there theoretical or experimental reasons why gravity should not be an emergent property of nature?

Assume a standard model view of the world in the very small. Is it possible that gravity only applies to systems with a scale large enough to encompass very large numbers of particles as an emergent property?

After all: the standard model works very well without gravity; general relativity (and gravity in general) has only been measured at distances on the millimeter scale.

How could gravity emerge? For example, it could be that space-time only gets curved by systems which have measurable properties, or only gets curved by average values. In other words that the stress-energy tensor has a minimum scale by which it varies.

Edit to explain a bit better what I'm thinking of.

1. We would not have a proper quantum gravity as such. I.e. no unified theory that contains QM and GR at the same time.
2. We could have a "small" (possibly semi-classical) glue theory that only needs to explain how the two theories cross over:
• the conditions and mechanism of wave packet reduction (or the other corresponding phenomena in other QM interpretations, like universe branching or decoherence or whatnot)
• how this is correlated to curvature - how GM phenomena arise at this transition point.

Are there theoretical or experimental reasons why such a reasoning is fundamentally incorrect?

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Sklivvz
What do you mean by "scale"? If it is about spatial dimensions, then I believe what you are saying implies singularities should not have gravitation. Or do you mean a certain amount of mass is required to generate gravity?

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Cem
What I think my example implies is that there would be no singularities, but some other phenomena which are very similar. They would behave effectively like singularities above a certain scale (i.e. have the same metric outside of, say, a ball around the would-be singularity)

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Sklivvz
I don't know what "scale" means exactly. My question is not "here's a crackpot theory, please shoot holes in it", it's a more general question and the answer might well be: "no, it's not possible because it's impossible to define a scale"

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Sklivvz
I'm "curious" how you define emergent. At some level, all physical laws of nature are "emergent"!

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Noldorin
@Noldorin, what I mean in the question is if it is compatible with experiment to theorize a universe where spacetime is flat at the quantum level, and only gets curved in correspondence to "measurement", the assumption being that the Standard Model lives well without GR and vice versa.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Sklivvz
@Noldorin I read "emergent" often in pysics blogs and popular books. (Written by experts). I'll google a bit on that.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Georg
@Noldorin, there is an article in wikipedia on emergence. 50 Years ago, when I studied, that was called "cooperative phenomenon" (eg ferromagetic behaviour), that was much more telling and precise.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Georg

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Despite all I wrote in my other answer, there's a very interesting attempt by Xiao-Gang Wen to come up with emergent models of gravity starting from quantum lattice models with no gravity, and only nearest neighbor interactions. His work can be found at gr-qc/0606100 and arXiv:0907.1203. He managed to show that quasiparticles with no energy gap and a helicity of $\pm 2$ can emerge without being accompanied by helicity $\pm 1$ or $0$ quasiparticles. Whether or not this model can be considered a model of gravity though is another matter.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user QGR
answered Jan 9, 2011 by (250 points)
+1 for mentioning Wen's work in this regard.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user user346
Thanks for mentioning our work. After 6 years and many journals (Science, PRL, PRB, NJP, JHEP, NPB), one of our papers finally get published in NPB. The referee reports and our replies represent detailed discussions between two different points of view on quantum gravity: emergence vs geometry/gauge points of view. The exchange of opinions is important and helpful for the development of quantum gravity. So I like to share those exchanges which are related to the question raised here

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Xiao-Gang Wen
Regarding to "Whether or not these models can be considered a model of gravity?", it is very good question. Our models do produce linearized quantum gravity, and they may be the first models to produce linearized quantum gravity (correct me if I am wrong and also see my question). So the next problem is how non-linear quantum gravity can emerge from some lattice models. In any case, our results do favor an emergent origin of gravity.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Xiao-Gang Wen
c.also. physics.stackexchange.com/review/suggested-edits/1493

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Dimensio1n0
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I'm not an expert in gravity, however, this is what I know.

There's a hypothesis about gravity being an entropic property. The paper from Verlinde is available at arXiv. That said, I would be surprised for this to be true. The reason is simple. As you probably know, entropy is an emergent property out of statistical probability. If you have non-interacting, adimensional particles into one half of a box, with the other half empty and separated by a valve, it's probability, thus entropy, that drives the transformation. If you look at it from the energetic point of view, the energy is exactly the same before and after the transformation. This works nicely for statistical distribution, but when you have to explain why things are attracted to each other statistically, it's much harder. From the probabilistic point of view, it would be the opposite: the more degrees of freedom your particles have, the more entropy they have. A clump has less degrees of freedom, hence has less entropy, meaning that, in a closed system, the existence of gravity is baffling. This is out of my speculation, and I think I am wrong. The paper seems to be a pleasure to read, but I haven't had the chance to go through it.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Stefano Borini
answered Nov 22, 2010 by (40 points)
Verlinde's paper is basically a confusing, badly composed rewrite of a paper made by Ted Jacobson in 1995: arxiv.org/abs/gr-qc/9504004

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user lurscher
Gravity increases entropy. In other words, a clump must have more entropy than a cloud of the same particles. Otherwise gravity would violate the laws of thermodynamics! The point here is that as matter clumps, it must lose energy. The energy is lost as some form of high entropy radiation. What is interesting is that both gravity and entropy have an asymmetrical direction: gravity is only attractive, entropy increases in the same direction of time.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Sklivvz
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You might want to look up the Weinberg-Witten theorem which shows that's not possible given certain assumptions. If the original model from which quantum gravity is supposed to emerge is an ordinary Poincaré covariant quantum field theory over flat nondynamical Minkowski space, they showed it's not possible for massless helicity $\pm 2$ particles to emerge. As a theory of quantum gravity ought to contain gravitons, this appears to rule out such models. Of course, these assumptions are questionable. For instance, the theory from which gravity emerges might not be a quantum field theory. This is the case for superstring theory.

Another possibility might be the "fundamental" model isn't Lorentz covariant. However, we still need the low energy effective theory to be approximately Lorentz covariant. In typical condensed matter analog models, different quasiparticles couple to different metrics, and there is no universality to the gravitational couplings, or the speed of light. Unless all the quasiparticles co-emerge together, I don't see any way around this problem.

It might be a bit hard to come up with the positive energy theorem in an emergent theory of gravity. The positive energy theorem states that the ADM energy of an asymptotically flat spacetime always has to be nonnegative. In an emergent theory, the ADM energy could just as easily be negative for some states. To see this, note first that the ADM energy can be defined locally as the limit as we go to spatial infinity of a locally defined integral over an enclosing spatial surface with one spatial and one time codimension. If we assume the "fundamental" theory is local, this means the now emergent ADM flux also has to be defined locally in terms of the more fundamental fields. As the enclosing boundary becomes larger and larger, its extrinsic curvature becomes closer and closer to zero. If we have a positive ADM flux passing through a plane — as defined with respect to a choice of normal vector orientation — a reflection by the plane will give us another state where this ADM flux is now negative. So, we can certainly imagine performing some sort of approximate reflection about the enclosing submanifold on a local patchwork basis, at least for the regions at or around the enclosing surface. We then need to find an interpolation of the resulting state far into the interior, which of course, might not look anything like a reflection at all. But if the fundamental theory also satisfies local independence, that ought to be possible. But the end result of all this construction is a state with negative emergent ADM energy. I know this argument is very handwavy and nonrigorous, but it sounds plausible. But there might be some loopholes. For instance, the fundamental theory might be local, but the emergent large scale excitations — and hence emergent spacetime — might be delocalized with respect to the underlying background spacetime. Or the underlying fundamental theory might be inherently nonlocal.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user QGR
answered Dec 31, 2010 by (250 points)
@Jason, could you elaborate in what sense the Weinberg-Witten theorem forbids emergent gravity? Your second point is a good one with a few caveats. In an emergent theory, quite generally speaking, one would have to sum over states of a microscopic ensemble of spin-networks (or strings) in order to obtain a semi-classical geometry. States in this ensemble could have negative energy w.r.t the quantum operator corresponding to the classical ADM observable. However, one would hope that some "natural" restrictions would disallow such states from contributing to physical observables.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user user346
@space_cadet: My comment doesn't apply to loop quantum gravity, or another other theory with Hamiltonian constraints. But Sklivvz appears to be asking about the emergence of quantum gravity from a quantum field theory, which can't admit Hamiltonian constraints.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user QGR
@QGR #1. all I'm saying is that any "emergent" model will ultimately yield GR in some limit. Whether you speak of the resulting GR in the Hamiltonian or the action (covariant) formulation, the physics will be the same. #2. Just to clarify - are you saying that a QFT cannot admit a constrained formulation?

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user user346
@space_cadet: A quantum field theory can admit Gauss gauge constraints, but not Hamiltonian constraints.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user QGR
@QGR - a QFT with a Hamiltonian constraint, i.e. $H |\Psi>$ for all physical states $|\Psi>$, has no local degrees of freedom. But it can have topological (non-local roughly speaking) d.o.f. This is known as a TQFT. An example is Chern-Simons theory.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user user346
AdS/CFT circumvents the Weinberg-Witten theorem by producing gravity in d+1 dimensions from a field theory in d dimensions.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user pho
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Isn't the answer to the question of the title widely believed to be "yes"?

If you believe that searching for what high-energy theorists call a "theory of everything" is a valuable and worthwhile enterprise, then you probably also believe that gravity as we currently understand it (General Relativity, say) "emerges" from some deeper theory (in the effective field theory sense) which unifies it with all other known fundamental forces.

Of course nobody yet knows for sure what that theory is, but I'm told certain flavors of string theory are the most viable candidates as of 2010. You can find some indication towards how gravity emerges from string theory in the first few sentences of this answer by Eric Zaslow.

Perhaps Eric Zaslow or some other expert can give more details at the level of saying, for instance, how Einstein's equations arise from string theory (I would ask this as a question on this site, except that I know I could find the answer in any book on string theory if I cared enough to look). I'm told that it has something to do with the renormalization group equations of the conformal field theory on the worldsheet, but I'm afraid I can't reproduce or explain that argument any further for you here.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user j.c.
answered Nov 23, 2010 by (260 points)
By my question I mean if it is possible that there is actually NO quantized gravity force field at all. Gravity would only exist classically.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Sklivvz
I'm afraid I don't quite understand what that means. Quantum mechanics can't only apply to some of the phenomena in the universe; if it did, there would be a ton of contradictions.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user j.c.
j.c. all of the flavors of string theory are actually the same thing expressed differently mathematically, as shown by Ed Witten.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Cem
@Cem: as conjectured by Ed Witten, you mean

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user j.c.
Right, sorry for an absolute tone. I was not aware there was a controversy about that.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user Cem
Well, I wouldn't say there's any controversy. What Ed Witten has done is generally accepted, but even he would say that it doesn't yet give a full understanding of M-theory.

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user j.c.
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In December, Carlo Rovelli summarized the last twenty years of the research agenda of a group of researchers in Loop Quantum Gravity theory. In a nutshell, LQG argues that gravity is a property of space-time rather than a quantum field theory mediated by a boson, and that space-time is fundamentally discrete with point-like locations in space-time connected by a network of connections to each other. In this approach, described by three main equations, the number of dimensions in space-time itself is emergent and neither locality nor the number of dimensions of space-time are well defined concepts at the most fine grained level. You are at point A and connected to points B, C and D, related by the equations, which when repeated ad infinitum are well approximated by a continuous, four dimensions space that may satisfy the properties of GR in classical approximation. As he sums up the research agenda:

"There is substantial circumstantial evidence that the large distance limit of the theory is correctly general relativity, from asymptotic analysis and from large distance calculations of n-point functions and in spinfoam cosmology; and there are open directions of investigations to reinforce this evidence. The degrees of freedom are correct and the theory is generally covariant: the low-energy limit is not likely to be much else than general relativity. But there is no solid proof yet."

This post imported from StackExchange Physics at 2014-04-04 15:42 (UCT), posted by SE-user user2592
answered Mar 17, 2011 by anonymous

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