Loop Quantum Gravity and entropy

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Discussion Overview

The discussion revolves around Loop Quantum Gravity (LQG) and its implications for cosmology, particularly regarding the concepts of oscillation between big bang and big crunch scenarios, the nature of singularities, and the theory's ability to address entropy and black hole information loss. Participants explore theoretical frameworks, predictions, and the appeal of LQG compared to other models like string theory.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • One participant questions how LQG accounts for oscillations of the universe and whether energy decreases after multiple bounces, expressing uncertainty about LQG's premises.
  • Another participant asserts that LQG posits only one bounce, prompting further inquiry about the implications of this view and the nature of time before a singularity.
  • A response clarifies that while the one-bounce model is common, it does not address deeper existential questions or the origins of the universe, focusing instead on phenomena around the bounce.
  • Participants discuss the implications of LQG for inflation and observable signatures, noting that quantum effects may lead to repellent gravity during high-density phases, resulting in super-inflation.
  • One participant expresses skepticism about LQG's explanatory power, suggesting it lacks definitive predictions and may not provide insights into black hole interiors.
  • Another participant highlights the appeal of LQG due to its focus on unsolved problems and its growing research community, while also mentioning competing theories like Shape Dynamics.
  • Links to recent papers on geometric entropy and other topics in quantum gravity are shared, indicating ongoing research interests in the field.

Areas of Agreement / Disagreement

Participants express differing views on the number of oscillations in LQG, the theory's explanatory power, and its comparison to string theory. The discussion remains unresolved, with multiple competing perspectives on these topics.

Contextual Notes

Participants note that LQG does not provide a definitive account of phenomena inside black holes and that its predictions are still considered provisional. The discussion highlights the complexity of defining geometric entropy and the challenges of observational confirmation in the context of LQG.

Who May Find This Useful

Researchers and enthusiasts in quantum gravity, cosmology, and theoretical physics may find this discussion relevant, particularly those interested in the implications of LQG and its comparison to other models.

Digitalism
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How specifically does LQG explain how the universe can oscillate from big bang to big crunch ad infinitum? Wouldn't the total energy able to be used as work decrease after a couple of bounces? Am I simply misunderstanding or making a false assumption about what LQG's premises are? I've not been following physics closely for several years, but I am familiar enough that you probably don't have to use metaphors to explain so feel free to be detailed.
 
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There is just one bounce.
 
Are you serious? Doesn't that just push back the question of what happened "before" a singularity back one step? Also, how could you know -objectively- how many oscillations have occurred? Or are you saying it would be a time symmetric oscillation or something similar?
 
Digitalism said:
Are you serious? Doesn't that just push back the question of what happened "before" a singularity back one step? Also, how could you know -objectively- how many oscillations have occurred? Or are you saying it would be a time symmetric oscillation or something similar?

Nothing wrong with the one-bounce picture. That is the most common in the LQC research lit.
You can set it up, with zero cosmological curvature constant , so that it repeatedly bounces, but that is not the most common case to consider.

It seems to me that the theory does not address questions like "why does existence exist?" or "where did it all come from?". It studies what could have happened to geometry and matter right around the bounce. What implications for inflation? What features might carry over from prior collapsing region? What might be an OBSERVABLE signature of the bounce?

AFAIK it leaves completely open the question of where the prior collapsing phase could have come from!

You might say the attitude is first let's try to understand what really happened instead of that classical failure called "singularity". And let's try to TEST our model by determining its footprint on the CMB polarization map.

So it's very focused on what should replace the classical theory breakdown. When the classical theory is replaced by a quantum theory that recovers the classical shortly before and after its failure, they find that in the new version quantum effects at high density cause gravity to be repellent. The brief episode where gravity is repellent involves a period of faster than exponential growth called "super-inflation", which precedes the ordinary inflation era. Ordinary inflation has constant or slowly declining H, super-inflation has rapidly increasing H, driving H to around the Planck frequency. (H is Hubble growth rate, units of reciprocal time). Considerable inhomogeneity, or "structure" is wiped out during the period where quantum effects dominate and gravity is repellent instead of attractive.

there are some recent papers on the pre-inflationary period in LQC. In case you are interested I'll get some links. there's also the interesting question of geometric entropy. How do you define it? When gravity is attractive, structure tends to increase, clumping, inhomogeneity grows, when repellent, the reverse. Different equilibrium states. New paper by Clifton Ellis Tavakol on geometric entropy, still no universally accepted definition.

BTW you are quite right that it pushes the frontier back a step. that is how science works I guess.
Model and test, figure out what was actually going on at the start of expansion, and immediately before. then, if you can do that, you still have another problem:what came before that. But I wouldn't call that *merely* pushing one step back in time. I think it is potentially a valuable accomplishment and very worthwhile striving for. (Though it fails to explain why existence exists :biggrin: )
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Ok, thank you so much Marcus that helps a lot and I appreciate you addressing the questions in a forthright manner. I guess I am at a loss as to why LQG would be so much more attractive to those working on it/who are proponents of it compared with string theory etc? I know some string models have been dismissed because of recent experiments. I know the "why?"s can not be answered directly, but I thought part of the appeal of LQG was the ability to explain the inner workings/structure of black holes etc and to bypass the information loss problem that happens as masses crunch into singularities. I would most definitely appreciate those links if you have the time to post them!
 
I'm not an expert, or active researcher, I simply follow research in QG and cosmology with interest. So this is FWIW, just opinion.
I tend to think that LQG does not explain ANYTHING until it has made some predictions about, say, features of ancient light (CMB) that are then found. And a small preliminary confirmation would even so still be very iffy and provisional.

I can't think how observational astrophysicists would ever confirm what LQG says about *inside* Black Holes. Maybe they might see some signature in Gammaray Bursts (GRB). I'm don't think the theory has a definitive account of the BH *inside*, although there have been several proposals. That would look to a researcher, I imagine, like an attractive area where there are interesting *unsolved* problems.

I get the impression that you want to better understand what attracts researchers to LQG and to Loop cosmology in particular. I imagine that what attracts young researchers, in general, is when a field has interesting *unsolved* problems, which are accessible and which are probably solvable, and which if solved, the solution might turn out to be important or consequential in some way. It's been a growing field, fast developing, for 7 or 8 years now, probably because of these factors.
Right now I think I see a significant rival competing for attention from young researchers: this is called Shape Dynamics. SD burst on the scene in 2011 when the Loops 2011 conference organizers devoted a day to it. The first day of the weeklong conference as I recall. Now in 2013 it will probably make a strong showing at Loops 2013. It is different from LQG but the Loop people have generally had their conferences be open to other background independent approaches (QG where you don't have a fixed geometric setup to start with).
They have hosted CDT (causal dynam. triang.) and AS (asymp. safety) QG in the past. Also have invited string theorists to give talks. I don't know how well SD will thrive in the longer run.

For some papers you could look down the list for the FIRST QUARTER 2013 MIP POLL.
https://www.physicsforums.com/showthread.php?t=681598
It's not all Loop but it has a bunch of interesting recent QG papers.
I'll get some links too, later today.
 
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Digitalism, this was a really nice question! After thinking for a while about it "LQG and entropy" I decided I would just give you the list of links to the top papers in the first quarter QG poll! That way it comes not just from me alone but from 14 of us who participated. It turned out that the top paper was about geometric ENTROPY and not specifically about LQG. I don't recommend reading it or any of these in particular, could be way too technical. This list is more to get an idea of what topics interest the nonstring qg researchers these days. An overview of the qg "research scene". Any paper you want to look at, just click the link. But the main thing is to kind of scan the lay of the land.

Six votes
http://arxiv.org/abs/1303.5612
A Gravitational Entropy Proposal
Timothy Clifton, George F R Ellis, Reza Tavakol

four votes
http://arxiv.org/abs/1302.0724
Death and resurrection of the zeroth principle of thermodynamics
Hal M. Haggard, Carlo Rovelli

http://arxiv.org/abs/1301.1264
Inflation as a prediction of loop quantum cosmology
Linda Linsefors, Aurelien Barrau

three votes
http://arxiv.org/abs/1303.7139
Symmetry and Evolution in Quantum Gravity
Sean Gryb, Karim Thebault

http://arxiv.org/abs/1303.2773
BTZ Black Hole Entropy in Loop Quantum Gravity and in Spin Foam Models
J.Manuel Garcia-Islas

http://arxiv.org/abs/1302.5265
The loop quantum gravity black hole
Rodolfo Gambini, Jorge Pullin

http://arxiv.org/abs/1301.5859
Hamiltonian spinfoam gravity
Wolfgang M. Wieland

Two votes
http://arxiv.org/abs/1303.6157
Loop quantum dynamics of the gravitational collapse
Yaser Tavakoli, Joao Marto, Andrea Dapor

http://arxiv.org/abs/1303.4989
Loop Quantum Gravity and the The Planck Regime of Cosmology
Abhay Ashtekar

http://arxiv.org/abs/1302.7142
Holonomy Operator and Quantization Ambiguities on Spinor Space
Etera R. Livine

http://arxiv.org/abs/1302.0254
The pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations
Ivan Agullo, Abhay Ashtekar, William Nelson

http://arxiv.org/abs/1301.6210
Embedding loop quantum cosmology without piecewise linearity
Jonathan Engle

http://arxiv.org/abs/1301.3480
Gauge networks in noncommutative geometry
Matilde Marcolli, Walter D. van Suijlekom

Thanks to everybody who participated: Atyy, Chemist@, Chronos, Devils, Jason_0, John, Martin, Nonlinearity, Nullius, Sam, Skydive, Tom and Vasu. It really gives a clarified 3D vision to have all our various viewpoints blended in, instead of just one person's.
 
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Is there any relation between LQC's bounce and the end of an Aeon, from Penrose?
 
ok, thank you so much marcus! I will definitely peruse the links as time permits.
 

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