Quantum Gravity and Specific GR Tests

[inflector]

In another forum that I frequent, I have been having a discussion where the state of quantum gravity research came up. Another poster claimed that one of the first thing that any gravity scientist checks for the theory is the theory's prediction for the precession of Mercury's perihelion.

Now for cosmological extensions to GR like, MOND, TeVeS or STVG, I can see where this might make sense. But I can't see how this poster's claim holds for quantum-gravity theories that haven't been able to establish that they reproduce GR in the continuum limit.

So I feel like I'm either missing something important about quantum gravity theories, in general, or the poster's comment only applies to gravity modifications designed as an alternative to dark matter and not quantum gravity theories. Or perhaps a little of each.

How, for instance, would one compute the precession of Mercury's perihelion using CDT, or Rovelli et al.'s spin-foam version of LQG? It may be that the dynamics of any object are implied in the spacetime microstructure, I don't understand the math well enough yet to follow the implications to know if this is true. But how can you compute the orbit of a planet when you require mass and fermions in order to have a sun and a planet like Mercury?

I noted the recent paper Dec. 21 paper where the Marseille LQG group claims to incorporate Fermions, so my question applies to research prior to this event, not that going forward.

 

[marcus]

But how can you compute the orbit of a planet when you require mass and fermions in order to have a sun and a planet like Mercury?

I noted the recent paper Dec. 21 paper where the Marseille LQG group claims to incorporate Fermions, so my question applies to research prior to this event, not that going forward.

started trying to answer and got interrupted, have to go.
Present inclusion of fermions is preliminary. No definite way to include mass, very much just a start. No way to compute orbits yet, which would be a classical application anyway. Some years more development needed.

 

[Careful]

In another forum that I frequent, I have been having a discussion where the state of quantum gravity research came up. Another poster claimed that one of the first thing that any gravity scientist checks for the theory is the theory's prediction for the precession of Mercury's perihelion.

Now for cosmological extensions to GR like, MOND, TeVeS or STVG, I can see where this might make sense. But I can't see how this poster's claim holds for quantum-gravity theories that haven't been able to establish that they reproduce GR in the continuum limit.

So I feel like I'm either missing something important about quantum gravity theories, in general, or the poster's comment only applies to gravity modifications designed as an alternative to dark matter and not quantum gravity theories. Or perhaps a little of each.

How, for instance, would one compute the precession of Mercury's perihelion using CDT, or Rovelli et al.'s spin-foam version of LQG? It may be that the dynamics of any object are implied in the spacetime microstructure, I don't understand the math well enough yet to follow the implications to know if this is true. But how can you compute the orbit of a planet when you require mass and fermions in order to have a sun and a planet like Mercury?

I noted the recent paper Dec. 21 paper where the Marseille LQG group claims to incorporate Fermions, so my question applies to research prior to this event, not that going forward.

The only scheme which can do you want it to do and which is available at the moment is semiclassical quantum gravity.

Careful

 

[genneth]

In another forum that I frequent, I have been having a discussion where the state of quantum gravity research came up. Another poster claimed that one of the first thing that any gravity scientist checks for the theory is the theory's prediction for the precession of Mercury's perihelion.

Now for cosmological extensions to GR like, MOND, TeVeS or STVG, I can see where this might make sense. But I can't see how this poster's claim holds for quantum-gravity theories that haven't been able to establish that they reproduce GR in the continuum limit.

So I feel like I'm either missing something important about quantum gravity theories, in general, or the poster's comment only applies to gravity modifications designed as an alternative to dark matter and not quantum gravity theories. Or perhaps a little of each.

How, for instance, would one compute the precession of Mercury's perihelion using CDT, or Rovelli et al.'s spin-foam version of LQG? It may be that the dynamics of any object are implied in the spacetime microstructure, I don't understand the math well enough yet to follow the implications to know if this is true. But how can you compute the orbit of a planet when you require mass and fermions in order to have a sun and a planet like Mercury?

I noted the recent paper Dec. 21 paper where the Marseille LQG group claims to incorporate Fermions, so my question applies to research prior to this event, not that going forward.

I don't think you're missing anything ;-)

I would actually like to tack on a question of my own:

As you noted, the precession of Mercury's perihelion is not quantum at all --- it's a purely classical effect. Thus the check would be to reproduce GR in the classical limit. LQG can almost show this for pure gravity. Can string theory? As I understand it, there is something like a theorem which states that spin-2 particles have to be gravitons (?) so does that mean everything is okay in the perturbative/effective theory limit, or does it imply quite some more?

 

[Careful]

As you noted, the precession of Mercury's perihelion is not quantum at all --- it's a purely classical effect.

Isn't the world quantum mechanical ? So what do you mean by a classical effect?

Thus the check would be to reproduce GR in the classical limit. LQG can almost show this for pure gravity.

Could you please cite paper, date and author ?

 

[inflector]

I don't think you're missing anything ;-)

I didn't think so. It would have meant that I really had a deep hole in my understanding somewhere for this to have been true.

As you noted, the precession of Mercury's perihelion is not quantum at all --- it's a purely classical effect. Thus the check would be to reproduce GR in the classical limit. LQG can almost show this for pure gravity.

I tried to argue this specific point, that reproducing GR was the first check, and that once you could do that, you automatically get Mercury's perihelion computations. But this idea seemed to fall on deaf ears.

That's one of the problems with forums, especially when you are new. There can be members with lots of experience in the forum (posts and years) who don't know as much as they think, and there can be very smart experienced members—even professional scientists—who don't know as much as you do in a specific domain where you as a relative beginner have studied more than they have. It makes it hard when someone disagrees with you because you are in the process of learning yourself and can't really judge others' opinions objectively. At least here in Physics Forums, I know who tends to know what they are talking about for the topics of interest to me.

Thus the check would be to reproduce GR in the classical limit. LQG can almost show this for pure gravity. Can string theory? As I understand it, there is something like a theorem which states that spin-2 particles have to be gravitons (?) so does that mean everything is okay in the perturbative/effective theory limit, or does it imply quite some more?

Good question. It might be good to post a separate thread. My understanding of string theory is so limited that I can't even begin to answer your question adequately. From what I have read about the graviton-based reproduction of GR in string theory, they have only shown GR in Minkowski space without dipheomorphism invariance.

 

[Careful]

I tried to argue this specific point, that reproducing GR was the first check, and that once you could do that, you automatically get Mercury's perihelion computations. But this idea seemed to fall on deaf ears.

Please, could you define precisely what you mean by reproducing GR from a theory of quantum gravity. That might substiantially help any further discussion.

Careful

 

[genneth]

Please, could you define precisely what you mean by reproducing GR from a theory of quantum gravity. That might substiantially help any further discussion.

Careful

I think both I and the OP (who should correct me if otherwise) think of this as writing down an expansion of the theory, order by order, in \hbar. Now, such a procedure is probably not going to produce a convergent series (but maybe an asymptotic one?), but it would still be good if the zero-th order theory yields GR (or at least after taking some more limits, such as not-too-strong field, etc.)

As far as the state of the art in LQG, marcus should be the one to pipe up, but my personal favourite review at the moment: is http://arxiv.org/abs/1012.4707

I believe (from memory as opposed to quoting) that the state "LQG reproduces GR in the semiclassical limit" is more technically "using only 5-valent vertices in spin-foams, to zeroth order in \hbar, the action of LQG is that of Regge theory (a discretised GR, which has already been shown to give GR in the limit that lattice spacing goes to zero)". (Again, quotes are not literal quotes!)

 

[Careful]

I think both I and the OP (who should correct me if otherwise) think of this as writing down an expansion of the theory, order by order, in \hbar. Now, such a procedure is probably not going to produce a convergent series (but maybe an asymptotic one?), but it would still be good if the zero-th order theory yields GR (or at least after taking some more limits, such as not-too-strong field, etc.)

But the problem here is what background are you writing your expansion around ? If you take Minkowski, you would have to reproduce the Newtonian potential as a condensate of virtual gravitons. I haven't seen anybody doing that yet, all one does is to study S-matrices for graviton scattering at asymptotic infinity (where the Newtonian potential is switched off). The point being is that your background should also be dynamically determined and this is merely words in LQG so far. And what does such expansion mean ? The only thing you can study is correlation functions. How would this translate to a planet moving around the sun?

the action of LQG is that of Regge theory (a discretised GR, which has already been shown to give GR in the limit that lattice spacing goes to zero)". (Again, quotes are not literal quotes!)

Regge theory is a classical theory and it is indeed well defined. The question is whether it's quantum ancestors like CDT/LQG are in the same category.

 

[marcus]

...

As far as the state of the art in LQG, marcus should be the one to pipe up, but my personal favourite review at the moment: is http://arxiv.org/abs/1012.4707

Mine too. The "December 4707" is a good review article, with history, motivation, intuition, and lots of citations to recent papers.

I believe (from memory as opposed to quoting) that the state "LQG reproduces GR in the semiclassical limit" is more technically "using only 5-valent vertices in spin-foams, to zeroth order in \hbar, the action of LQG is that of Regge theory (a discretised GR, which has already been shown to give GR in the limit that lattice spacing goes to zero)". (Again, quotes are not literal quotes!)

I think the "LQG reproduces GR" result is a beast gradually crawling up out of the mud of confusion. I see how it's going, even though I don't yet see the final result clean and clear.

 

[Careful]

Mine too. The "December 4707" is a good review article, with history, motivation, intuition, and lots of citations to recent papers.

Of course, it means everything that 25 years of ''progress'' can be summarized on 24 pages, that is 0,96 useful pages/year

 

[genneth]

Of course, it means everything that 25 years of ''progress'' can be summarized on 24 pages, that is 0,96 useful pages/year

Better than my batting average in research...? (Can I claim to have even written one useful page? I doubt it...)

 

[genneth]

But the problem here is what background are you writing your expansion around ? If you take Minkowski, you would have to reproduce the Newtonian potential as a condensate of virtual gravitons. I haven't seen anybody doing that yet, all one does is to study S-matrices for graviton scattering at asymptotic infinity (where the Newtonian potential is switched off). The point being is that your background should also be dynamically determined and this is merely words in LQG so far. And what does such expansion mean ? The only thing you can study is correlation functions. How would this translate to a planet moving around the sun?


Regge theory is a classical theory and it is indeed well defined. The question is whether it's quantum ancestors like CDT/LQG are in the same category.

Isn't the Regge action also independent of background? Isn't GR? I don't see why you have to expand around a fixed background at all. Classical GR is not a theory of scattering, and no background is necessary.

 

[MathematicalPhysicist]

Of course, it means everything that 25 years of ''progress'' can be summarized on 24 pages, that is 0,96 useful pages/year

It's almost 1 useful pages/year, what more can you ask for?!

 

[marcus]

One thing I get from Inflector's posts is an interest in testing. This could become more important than the gradual progress one sees being made on the "reproduce GR" front.

Someone to watch in this regard is Wen Zhao (Cardiff). In a recent paper of his he had two co-authors at the KICC---Kavili Institute for Cosmology Cambridge.
Yin-Zhe Ma and Michael Brown

The way I see it, interest and credibility in the eyes of young unknown astro-phenomenology postdocs at a place like KICC has an almost "make or break" significance. These are people I have never heard of, in a first-rate place, who either are or are not willing to invest career-time in seeing how to test an early universe QG model. Who may or may not take the LQG picture seriously. Who are not biased either way as to the outcome.

So we'll see.

Here are some Wen Zhao papers. This is exactly the sort of person you want to be interested in whether there was a bounce:

2. arXiv:1009.5243 [pdf, ps, other]
Relic gravitational waves: latest revisions and preparations for new data
Wen Zhao, L. P. Grishchuk
Comments: 11 pages, 4 figures, 3 tables; v.2: modifications, improvements, additional references; accepted for publication in Phys. Rev. D
Subjects: Cosmology and Extragalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)

4. arXiv:1009.0206 [pdf, ps, other]
Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
W. Zhao, C. Van Den Broeck, D. Baskaran, T.G.F. Li
Comments: 28 pages, 5 figures, 5 tables; v.2: modifications, improvements, additional references; accepted for publication in Phys. Rev. D
Subjects: Cosmology and Extragalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)

5. arXiv:1007.2396 [pdf, ps, other]
Constraints on standard and non-standard early Universe models from CMB B-mode polarization
Yin-Zhe Ma, Wen Zhao, Michael L. Brown
Comments: 41 pages, 23 figures, JCAP in Press
Journal-ref: JCAP 10 (2010) 007
Subjects: Cosmology and Extragalactic Astrophysics (astro-ph.CO)

6. arXiv:1005.4549 [pdf, ps, other]
Relic gravitational waves in the light of 7-year Wilkinson Microwave Anisotropy Probe data and improved prospects for the Planck mission
W. Zhao, D. Baskaran, L. P. Grishchuk
Comments: 27 pages, 12 (colour) figures. Published in Phys. Rev. D. V.3: modifications made to reflect the published version
Journal-ref: Phys.Rev.D82:043003,2010
Subjects: General Relativity and Quantum Cosmology (gr-qc); Cosmology and Extragalactic Astrophysics (astro-ph.CO); High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)

7. arXiv:1005.1201 [pdf, ps, other]
Separating E and B types of polarization on an incomplete sky
Wen Zhao, Deepak Baskaran
Comments: 43 pages, 15 figures, 1 table. The finial version, will appear in PRD
Journal-ref: Phys.Rev.D 82, 023001 (2010)
Subjects: Cosmology and Extragalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)

8. arXiv:1004.0804 [pdf, ps, other]
Primordial Gravitational Waves and Cosmic Microwave Background Radiation
D. Baskaran, L. P. Grishchuk, W. Zhao
Comments: A summary of presentations delivered at the OC1 parallel session "Primordial Gravitational Waves and the CMB" of the 12th Marcel Grossmann Meeting on General Relativity (Paris, 12-18 July 2009). To be published in the Proceedings of the MG12. 18 pages, 8 (colour) figures.
Subjects: General Relativity and Quantum Cosmology (gr-qc); Cosmology and Extragalactic Astrophysics (astro-ph.CO); High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)

 

[Careful]

Isn't the Regge action also independent of background? Isn't GR? I don't see why you have to expand around a fixed background at all. Classical GR is not a theory of scattering, and no background is necessary.

Well, Regge action still requires a nice piecewise linear manifold with fixed topology, a background if you want to. GR has the same kind of background dependence. LQG has not. I don't know if you are aware, but all kind of observables we use in relativity are gauge dependent. When we calculate perihelion shift of Mercury we assume a flat Minkowski background, when we speak about orbits of planets we do the same... Dirac observables are almost never ever computed in GR and doing so in quantum gravity would be ''almost'' impossible.

Moreover, if you want to define perturbation series in $\hbar$, you always have to split the system in free part and interaction and the linearization of the system always depends upon the background metric. Equivalently, in LQG, you will have to import a preferred basis which is not related to the total Hamiltonian, otherwise you won't be able to set up a perturbation series.

Careful

 

[Careful]

It's almost 1 useful pages/year, what more can you ask for?!

Indeed, from such intellectual giants

 

[marcus]

Well, Regge action still requires a nice piecewise linear manifold with fixed topology, a background if you want to. GR has the same kind of background dependence. LQG has not...

?

In the LQG community "background independence" refers to to theories where the development does not require a background metric--a pre-arranged geometry.

Regge GR and the original formulation of LQG are more or less on the same footing. They all assumed a manifold at the start. Indeed with LQG there is a fixed topology, as in other cases.

The manifold simply did not have a background metric defined on it at the start. The metric arises dynamically. Traditionally this is what the relevant researchers have always meant by "background independence".

So what you said there was potentially confusing.

 

[Careful]

?

In the LQG community "background independence" refers to to theories where the development does not require a background metric--a pre-arranged geometry.

Regge GR and the original formulation of LQG are more or less on the same footing. They all assumed a manifold at the start. Indeed with LQG there is a fixed topology, as in other cases.

That was the case in the original formulation and required to give meaning to things like knotting of spin networks. But things have evolved now, and people start to think more in the causal set way. This is another example of a fact I once mentioned to you, LQG says A and not A, and it's practitioners demand I can only use classical logic

The manifold simply did not have a background metric defined on it at the start. The metric arises dynamically. Traditionally this is what the relevant researchers have always meant by "background independence".

So what you said there was potentially confusing.

No, it was not, certainly not in the modern way of thinking about it.

Careful

 

[marcus]

That was the case in the original formulation and required to give meaning to things like knotting of spin networks. But things have evolved now, and people start to think more in the causal set way. This is another example of a fact I once mentioned to you, LQG says A and not A, and it's practitioners demand I can only use classical logic


No, it was not, certainly not in the modern way of thinking about it.

Careful

Heh heh, now you are getting even more confusing. The meaning of "background independence" has not changed. It still means the theory does not use a prearranged background metric.

Lqg, including the most recent formulation, shares this property with GR and Regge etc.

 

[Careful]

Heh heh, now you are getting even more confusing. The meaning of "background independence" has not changed. It still means the theory does not use a prearranged background metric.

Lqg, including the most recent formulation, shares this property with GR and Regge etc.

Sure it has been. If you want to, I will even cite a paper of SMOLIN proving that it has been so ! Smolin has been taking about many different kinds of background independence going from kinematical objects such as the manifold, the differentiable structure, the dimension to objects we think of as dynamical such as the metric.

Careful

 

[Careful]

For example, see http://arxiv.org/PS_cache/hep-th/pdf/0507/0507235v1.pdf page 20, third bullet. Other references needed ?

Careful

 

[marcus]

I thought you might try to cite Smolin's "The case for background independence."

Smolin is not a representative LQG researcher---more of an outlier. That was a 2005 paper where he tried to expand the discussion, and generalize on B.I. It did not catch on. For most of the LQG community, B.I. just means B.I. That one 2005 paper did not change how 50 other Loop researchers talk.

Smolin's paper explicitly argued that it would be fruitful to talk about degrees of background independence, put it on a scale, so you could say something was more or less background independent. The term has a special meaning within the context of the paper.

 

[atyy]

But Smolin is the one who started all the fuss with his popular anti-string book.

And how can Rovell's "relational" arguments in his QG book make sense if there is a background metric? Do you think Rovelli meant only no background 4D spacetime metric - ie. not everything is relational?

Did you think LQG researchers understand "background independence" to mean "no background 4D spacetime metric" or "no background metric"?

 

[atyy]

Maybe Weinberg would say that the fewer pages per year the better - isn't the dream of of a TOE to have everything on 1 line?

genneth is a condensed matter guy, I think, so his aim would be different?

 

[marcus]

But Smolin is the one who started all the fuss with his popular anti-string book.
...

Atyy I suspect you are just joking. There are serious issues involving QG and "tests" as mentioned by the O.P. Inflector---issues involving the background independence of GR and newer theories (e.g. Witten papers on B.I. going back to 1992, 1993 as I recall.)

Whether or not there was some "fuss" is largely irrelevant to the substantive issues that we care about.

Also the "fuss" I think you refer to was already in full cry in 2003! on Usenet sci.physics.research. I was particularly struck by the posts of Motl and Baez but there were many others. I don't remember much from Lee Smolin at the time. And his book did not appear until Fall of 2006! Back in 2003 there was this Usenet thread called "String theory crack up?" and all this stuff was hotly debated. Susskind had come out with the "anthropic string landscape" in summer 2003.

In some sense none of this matters. GR is still background independent---in the usual sense of having dimension and topology specified, but no background metric (no prior geometry). GR is still general covariant--thus no physical meaning to points in space. Manifold used in formulation but ultimately modded out---solutions are equivalence classes belonging to no particular manifold.

So either the rest of physics needs to catch up with GR, and reach a general covariant formulation (continuum does not physically exist) or it has to find some reason not to take the principles of GR seriously---some crucial flaw or limitation.

It doesn't matter if there is fuss or no-fuss. These issues persist on the agenda.

And how can Rovell's "relational" arguments in his QG book make sense if there is a background metric? Do you think Rovelli meant only no background 4D spacetime metric - ie. not everything is relational?

Did you think LQG researchers understand "background independence" to mean "no background 4D spacetime metric" or "no background metric"?

Unfortunately I don't understand the questions. You could elaborate and explain why you think the questions are important.

I think it is assumed that there is no background metric, and so the premise of your question "how can...make sense?" does not seem to hold.

In case you want to look into them here are some Witten papers on B.I.---I don't know what he meant by B.I. back in 1992-1993, exactly, but here they are for what it's worth:3. arXiv:hep-th/9306122 [pdf, ps, other]
Quantum Background Independence In String Theory
Edward Witten
Comments: 20 pp
Subjects: High Energy Physics - Theory (hep-th)

4. arXiv:hep-th/9210065 [pdf, ps, other]
Some Computations in Background Independent Open-String Field Theory
Edward Witten
Comments: 14 pp
Journal-ref: Phys.Rev.D47:3405-3410,1993
Subjects: High Energy Physics - Theory (hep-th)

5. arXiv:hep-th/9208027 [pdf, ps, other]
On Background Independent Open-String Field Theory
Edward Witten
Comments: 18 pp
Journal-ref: Phys.Rev.D46:5467-5473,1992
Subjects: High Energy Physics - Theory (hep-th)

 

[marcus]

Maybe Weinberg would say that the fewer pages per year the better - isn't the dream of of a TOE to have everything on 1 line?

genneth is a condensed matter guy, I think, so his aim would be different?

Yes I agree! Some of the great landmark papers in physics have been just a couple of pages, or a halfdozen, or so I'm told. It's sometimes a good sign when something is so concise.

Why do you think Genneth specialty is condensed matter? I have that impression too but don't remember where I got it. Did he say something to that effect in another thread?

In any case it is refreshing to meet someone with lively interest in some field (like QG) but no stake in this or that approach

 

[genneth]

All this speculation about me is a bit embarrassing... I am a condensed matter theorist by training, but have now almost left physics entirely for biology. Ironically, this has perhaps led me to really think about where theoretical physics sits in the grand scheme of things, especially with respect to experiments.

Back to the topic at hand, I find Careful's words intriguing. I'm not 100% certain I understand what his point was, but my interpretation is that he is asking about what the "background" is, rather in the style of the Smolin article Marcus linked to. This I believe is a perfectly good question. However, I think the answer is that in LQG the system under study actually allows *greater* change than GR proper. In GR, the topology is fixed, and only the metric is allowed to vary. Similarly, in Regge theory we build a combinatoric structure of flat 4-simplices glued together, and this structure is fixed, but the "creases" at the gluing edges are allowed to vary. In LQG, we actually sum over all combinations of the combinatorial structure; in principle there is no limit (unless I have not understood the papers correctly --- always possible, even likely) to what the underlying graph actually is. I expect that we would find topologically non-trivial configurations to simply be massively unfavourable in the sum-over-spin-foams, but nevertheless be represented. Perhaps someone who actually does these computations can weigh in and answer in detail? There's only so much information an amateur can bring to the table...

 

[atyy]

Yes, a viable theory of quantum gravity should have GR as its classical limit, and thus have no prior 4D spacetime geometry in that limit. However, I don't see the relationship between that and Rovellian LQG's tremendous stress on general covariance and relational physics.

One can have generally covariant flat spacetime theories, so Rovellian LQG's concentration on general covariance may have nothing to do with no prior 4D spacetime geometry.

If Rovellian LQG's insistence that all physics should be relational means that there is no background metric, it is wrong. There can be a background metric which does not have the meaning of spacetime, so that the emergent classical spacetime is still dynamical.

 

[genneth]

Yes, a viable theory of quantum gravity should have GR as its classical limit, and thus have no prior 4D spacetime geometry in that limit. However, I don't see the relationship between that and Rovellian LQG's tremendous stress on general covariance and relational physics.

One can have generally covariant flat spacetime theories, so Rovellian LQG's concentration on general covariance may have nothing to do with no prior 4D spacetime geometry.

If Rovellian LQG's insistence that all physics should be relational means that there is no background metric, it is wrong. There can be a background metric which does not have the meaning of spacetime, so that the emergent classical spacetime is still dynamical.

I think it's important to separate Rovelli the philosopher from the LQG theorist. The former will make strong statements about relational views on quantum mechanics and the importance of general covariance. The latter produces concrete, novel physical theories which are scrutinised to the usual level of rigour. Of course, the former may have guided the latter, and the latter occasionally extols the virtues of LQG with the moral viewpoint of the former, but we can still take the physics and leave the interpretation up to personal preference. *IF* it turns out that LQG really does reduce (at zero-th order in \hbar) to Regge theory then it doesn't really matter how and why the philosophy works --- we should indeed rebuild the philosophical understanding after the fact.

All this current discussion was based around my original assertion (why may have been worded too strongly) that LQG does indeed reduce to Regge theory (kinda --- I had already clarified to what extent I believe this to be true (belief here meaning what I understand, rather than what I personally believe...)). The question I asked still stands: to what extent can a similar program be achieved with the state of the art in string theory? I have no doubt that string theory can produce sensible scattering amplitudes in the perturbative regime --- but that was the case some 15/20 years ago --- what's the status now? (Review papers would be excellent, but I don't know the literature in the same way as I do for LQG).