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Why all these prejudices against a constant? ( dark energy is a fake probem) 
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#19
Mar2810, 09:14 AM

P: 5,632

Marcus: again, thanks for bringing another great paper to our attention....
and this regarding the coincidence argument: FRA I also think we are current missing much of what appears as an information based universe. 


#20
Mar2810, 09:19 AM

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#21
Mar2810, 10:36 AM

P: 2,799

1) stop worrying about the "mysterious lambda" or 2) START worrying about all mysterious "constants". In the generic sense "constant" could also apply to other things than numbers, for example "constant" symmetries, and thus "physical law" itself. Ie. the fact that it may be "just another constant" doesn't make it less mysterious. Maybe we rather just have more "clues" to this particular constant, than say the gravitational constant or plancks constant? /Fredrik 


#22
Mar2810, 11:22 AM

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#23
Mar2810, 12:26 PM

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P: 1,685

The CC is not a problem for GR (well except that it makes various cosmological solutions a little more ugly), but really a generic quantum problem.
It doesn't matter what side of the field equation you put it on, the problem is the same, namely an unnatural cancelation between two quantities that a priori have nothing to do with one another (read no known physical relation). In the full quantum theory, we are interested in the expectation value of the stress energy tensor <Tuv>, which in vacuum is proportional to < P > Guv by Lorentz invariance. By inspection of Einsteins field equations, this is equivalent to adding a term to the effective cosmological constant. lambda effective = lambda + 8piG <P>, where lambda is just the old simple (undetermined classical constant of integration) and <P> is the energy density of the quantum vacuum. Now (lambda effective/8piG) = Pv ~ 10^47 Gev^4 by experiment (WMAP say). The problem is that we know how to calculate <P>, generically it is simply summing up all the normal modes of the zero point energy of some field (or sets of fields), up to some cutoff. If we take the cutoff to be Mpl, <P> will be something like ~10^72 Gev^4 and then you notice that (lambda/8piG + <P>) in order to satisfy experimental bounds, must delicately conspire to cancel to something like 120 decimal places. The problem is that there is no obvious physical reason why lambda/8piG (a quantity arising from a classical equation) should have anything whatsoever to do with <P> (a quantum quantity). Now, if there was an unknown symmetry that related them, you might venture to guess that they could cancel exactly, but no such symmetry is known and worse they dont cancel exactly. I should point out that you can't get around this miracle trivially. Even if you completely ignore everything from the electroweak scale, all the way down to the Planck scale and instead only consider standard model physics, you would set the cutoff value to something like say the QCD scale, you still have about 40 orders of magnitude worth of decimal places to account for. Now you are of course free to simply set the constant term equal to the tree level or semiclassical contribution to <P> and set them equal to zero. The problem then is you still have to talk about the shift of the vacuum energy, by higher order terms induced by radiative corrections, and so you have to arrange it so that each constant appearing in front of the counterterms is finetuned order by order, such that the final sum approaches the experimental bound. It is this, more than anything else, that really is the crux of the problem. The thing we measure in our telescopes is necessarily the full theory (b/c quantum mechanics is part of the real world). And in this quantum theory, nothing protects the vacuum energy from radiative corrections. An analogous (though much less severe) problem occurs for instance, when you consider the smallness of the Neutrino mass relative to say the Higgs vev. If you naively proceed as above, you see that there is an unnatural cancellation that should take place. Of course there, we are rescued by a mechanism that forces the two terms involved in the cancellation to actually be close (this is called the seesaw mechanism). 


#24
Mar2810, 12:56 PM

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P: 1,685

Its worth pointing out how Supersymmetry almost solves the problem and how it elucidates the nature of the issue.
Assume that <P> appearing above, was for some reason identically zero, then indeed lambda effective would just be a constant of integration and everyone would be happy. No rhyme or reason why its small or big, or whatever. Who cares, its just a number that experiment happened to find. You could invoke the anthropic principle trivially if you really wanted too at that point and no one would mind. And indeed, in exact rigid supersymmetry it was noted long ago that fermion loops exactly cancel boson loops and the net vacuum contribution is zero (at least perturbatively). The problem is, exact supersymmetry is not the way the world works, and it must be broken. When you break rigid supersymmetry in this framework you induce terms that necessarily set <p> != 0 (and if you include gravity and make the susy local, the superpotential and the kahler potential will not in general exactly cancel!) and you are back to worrying about how weird it is for physical cancellations to take place of that magnitude (although now, the problem is cut in two on a log scale and may also be sensitive to exactly where the supersymmetry breaking scale is set) 


#25
Mar2810, 02:17 PM

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P: 5,451

Haelfix,
I think you agree with Rovelli, but I am not sure. He does not deny that the smallness of lambda is no problem, but e says that one must distinguish between 1) a small classical (tree level) lambda which stays small even if you calculate quantum corrections and 2) zero classical lambda where the nonzero part is purely quantum mechanical. So acording to Rovelli the problem is why lambda stays small even if it is subject to quantum corrections, not how quantum corrections create lambda which zero classically. Compare it to the Higgs mass. It is unclear how the Higgs mass is protected against quantum corrections pushing it to the Planck scale. But these effects (or their absence) seems to have nothing to do whith the creation of teh Higgs mass at all. The same applies to all other parameters in the SM. It is a puzzle where they are coming from, but it is fairly well understood how they behave under quantum corrections (the Higgs mass is an exception). What you are saying about SUSY is the core of the problem. Zero lambda would be fine, but tiny lambda including quantum corrections from broken SUSY is a riddle. But if you look at all other classical field theories they perfectly make sense w/o quantum corrections in a certain regime. If you restrict yourself to tis regime there is no problem with the constants at all. 


#26
Mar2810, 02:58 PM

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P: 1,685

I don't quite follow.
The way I read the paper was that it wasn't anything new to the standard story I told above, it just restated it differently. To simplify the terminology, and with total abuse of notation and disregard for constants, i'll just state the above equation again: Lambda total = lambda classical + lambda quantum. Lambda total is fixed by experiment. You are free to set lt = lc but then you have to explain why lq is zero (this is what I think he wants us to do). You can set lc = 0 but then you have to explain why lq is however many orders of magnitude different than a qft calculation tells us it should be. Or you can insist that there is some sort of mechanism that relates lc and lq such that they are extremely close and the finetuning becomes natural. The problem is the same in all three cases, its just basically a relabeling of words what you want to call things. 


#27
Mar2910, 12:32 AM

P: 2,799

QM and Relativity did away with some realism, but not all of it. Both are somehow attempts at acknowledging the incompleteness and relativit of nature, without abandoning the incompletness and relativity of physical law. There is an ambigousness there IMO, becase _information about physical law_ are not treated on the same footing as _information about the initial state_ of a system, when it IMO should. /Fredrik 


#28
Mar2910, 01:44 AM

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P: 5,451

Let's try a different approach: for many constants in nature one expects that they are scaledependent. If they aren't one has to find a mechanism why they are protected. What we measure are not the bare nor the treelevel values but always the "dressed" values where all quantum corrections are already taken into account. Now we split the constants in a tree level and a quantum correction part (I do not know if this is really a good idea :) I think one can state the problem as follows: 1) if we believe in this classical part + quantum correction part story, then we have to solve the two problems what causes the classical part? and why should it be protected against scaling? 2) if we do not believe in this split, we have to solve the problem what causes the cc at all?. I think what Rovelli is saying is that it's not clear to him why the mechanism which causes the existence of the cc at all should be the same as the mechanism that causes it's scaling. (example: we understand the mechanism which scales a massterm in QFT, but we do not understand where this mass term comes from; if we use the Higgs, again we understand the scaling of the Yukawacoupling, but we do not understand why it is there at all) 


#29
Mar2910, 11:49 PM

PF Gold
P: 1,961

Just one question here: why all this quible here if Marcus himself support assymptotic safety? The small value of the cosmological constant is just a consequence of the non trivial fixed point of G x /\ space due to renormalizable non perturbative nature of the Einstein Hilbert action.



#30
Mar3010, 12:32 AM

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P: 5,451

This means that lambda is a term on the left hand side and is somehow protected against UV corrections. Is would solve the problem for its smallness, not for its existence.
What is the current status of asymptotic safety? 


#31
Mar3010, 11:24 PM

PF Gold
P: 1,961

Well, asymptotic safety doesn`t work withou lambda...



#32
Sep1511, 08:13 AM

Astronomy
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PF Gold
P: 23,233

Here's an alternative take on the CC problem:
http://arxiv.org/abs/1103.4841 The cosmological constant: a lesson from BoseEinstein condensates Stefano Finazzi, Stefano Liberati, Lorenzo Sindoni (Submitted on 24 Mar 2011) The cosmological constant is one of the most pressing problems in modern physics. In this Letter, we address the issue of its nature and computation using an analogue gravity standpoint as a toy model for an emergent gravity scenario. Even if it is well known that phonons in some condense matter systems propagate like a quantum field on a curved spacetime, only recently it has been shown that the dynamics of the analogue metric in a BoseEinstein condensate can be described by a Poissonlike equation with a vacuum source term reminiscent of a cosmological constant. Here we directly compute this term and confront it with the other energy scales of the system. On the gravity side of the analogy, this model suggests that in emergent gravity scenarios it is natural for the cosmological constant to be much smaller than its naif value computed as the zeropoint energy of the emergent effective field theory. The striking outcome of our investigation is that the value of this constant cannot be easily predicted by just looking at the ground state energy of the microscopic system from which spacetime and its dynamics should emerge. A proper computation would require the knowledge of both the full microscopic quantum theory and a detailed understanding about how Einstein equations emerge from such a fundamental theory. In this light, the cosmological constant appears even more a decisive test bench for any quantum/emergent gravity scenario. 5 pages, 1 figures 


#33
Sep1511, 09:40 AM

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P: 8,657

Nima gives it in http://www.cornell.edu/video/?videoID=909 at 13:57, explains that there is no problem in principle at 15:35, and further explains why the solution is considered fine tuned.



#34
Sep1511, 11:44 AM

Astronomy
Sci Advisor
PF Gold
P: 23,233

The FinazziLiberatiSindoni (FLS) paper could be something of a gamechanger, so I want to back up and reconsider what I was saying. Here is an excerpt from their conclusions:
==quote FLS http://arxiv.org/abs/1103.4841 == ...The implications for gravity are twofold. First, there could be no a priori reason why the cosmological constant should be computed as the zeropoint energy of the system. More properly, its computation must inevitably pass through the derivation of Einstein equations emerging from the underlying microscopic system. Second, the energy scale of Λ can be several orders of magnitude smaller than all the other energy scales for the presence of a very small number, nonperturbative in origin, which cannot be computed within the framework of an effective field theory dealing only with the emergent degrees of freedom (i.e. semiclassical gravity). The model discussed in this Letter shows all this explicitly. Furthermore, it strongly supports a picture where gravity is a collective phenomenon in a pregeometric theory. In fact, the cosmological constant puzzle is elegantly solved in those scenarios. From an emergent gravity approach, the low energy effective action (and its renormalization group flow) is obviously computed within a framework that has nothing to do with quantum field theories in curved spacetime. Indeed, if we interpreted the cosmological constant as a coupling constant controlling some selfinteraction of the gravitational field, rather than as a vacuum energy, it would straightforwardly follow that the explanation of its value (and of its properties under renormalization) would naturally sit outside the domain of semiclassical gravity. For instance, in a group field theory scenario (a generalization to higher dimensions of matrix models for two dimensional quantum gravity [19]), it is transparent that the origin of the gravitational coupling constants has nothing to do with ideas like “vacuum energy” or statements like “energy gravitates”, because energy itself is an emergent concept. Rather, the value of Λ is determined by the microphysics, and, most importantly, by the procedure to approach the continuum semiclassical limit. In this respect, it is conceivable that the very notion of cosmological constant as a form of energy intrinsic to the vacuum is ultimately misleading. To date, little is known about the macroscopic regime of models like group field theories, even though some preliminary steps have been recently done [20]. Nonetheless, analogue models elucidate in simple ways what is expected to happen and can suggest how to further develop investigations in quantum gravity models. In this respect, the reasoning of this Letter sheds a totally different light on the cosmological constant problem, turning it from a failure of effective field theory to a question about the emergence of the spacetime. ==endquote== This is a brief paper (besides references, only 4 pages!) with potentially farreaching implications, it seems to me. I don't recall our discussing itany comments? 


#35
Nov611, 01:45 PM

Astronomy
Sci Advisor
PF Gold
P: 23,233

More reasons to mistrust the "dark energy" interpretation of the cosmological constant (and the touted bafflement about its size) can be found in a review article for the special SIGMA issue on Loop gravity and cosmology, written by Larry Sindoni of AEI Potsdam.
http://arxiv.org/abs/1110.0686 Emergent models for gravity: an overview L. Sindoni (Submitted on 4 Oct 2011) We give a critical overview of various attempts to describe gravity as an emergent phenomenon, starting from examples of condensed matter physics, to arrive to more sophisticated pregeometric models. The common line of thought is to view the graviton as a composite particle/collective mode. However, we will describe many different ways in which this idea is realized in practice. 54 pages. Invited review for SIGMA Special Issue "Loop Quantum Gravity and Cosmology". I tend now to expect this Sindoni review of Emergent Gravity will become a basic wellcited paper, and that the SIGMA special LQG/C issue will constitute the next big Loop gravity book. Many of its chapters have now been posted as arxiv preprints. It's clearly going to be a valuable collection. Lorenzo Sindoni gave a seminar in December 2008 on Emer. and Analog Grav. that is on video http://pirsa.org/08120049/. Stefano Liberati at SISSA was his advisor, PhD in 2009 if I remember right. 


#36
Nov611, 07:48 PM

P: 124

Marcus, I believe I'm interested in the subject of your last three postings but it’s a little beyond me. Do you have the patience to explain it one more time in a simpler way? Thanks



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