A change going on in theoretical physics

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SUMMARY

The ongoing shift in theoretical physics emphasizes the significance of spacetime geometry and the urgent need to quantize General Relativity (GR). This transition is primarily driven by advancements in cosmology, including concepts such as dark energy and black holes, which necessitate a re-evaluation of traditional physics frameworks. The notion of a backgroundless spacetime, where matter is defined relative to gravitational fields rather than fixed geometries, is central to this discussion. The recent focus on diffeo-invariant theories and polymer-like networks as excitations of space marks a pivotal evolution in understanding the relationship between matter and geometry, indicating a potential reconstruction of the standard model in a background-independent manner.

PREREQUISITES
  • General Relativity (GR) concepts
  • Understanding of diffeo-invariance in theoretical physics
  • Familiarity with cosmological phenomena such as dark energy and black holes
  • Knowledge of quantum gravity and polymer-like networks
NEXT STEPS
  • Research the implications of quantizing General Relativity
  • Explore the concept of diffeo-invariance in theoretical frameworks
  • Study the role of polymer-like networks in quantum gravity
  • Investigate the impact of background independence on the standard model of particle physics
USEFUL FOR

Theoretical physicists, cosmologists, and researchers interested in the foundations of quantum gravity and the evolution of spacetime concepts will benefit from this discussion.

marcus
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a shift in theoretical physics

GR has a different concept of space and time from the one in String Theory and habitually used in the rest of physics. This is being realized more now because of a shift in factors driving research.

Spacetime geometry has taken over the job of driving development in theoretical physics. Cosmology, big bang, inflation, dark energy, dark matter, constants over cosmological time, dispersion relations in gammaray bursts, black holes, and so on---this is where the questions are coming from, not (as was the case in the 1970s) from accelerator event-counts.

GR is the framework within which these things are defined, which is one reason for the increased concern with quantizing it. GR is used to calculate the interesting numbers (e.g. about early universe as related to what can be observed now in CMB, particle and element abundances, structure etc.) and perhaps partly because of this it now seems more urgent to quantize GR.

With GR comes different ideas of space and time. Rovelli's recently posted "Dialog on quantum gravity" is basically about the difficulty HEP theorists have with the "backgroundless"--ness of General Relativity.

In GR the spacetime manifold has no physical meaning--its points are not realworld events. The manifold is just a convenience to get you started, and it has no set geometry. The thing with physical meaning is the gravitational field itself, things (matter) are located within the field. space is relational not absolute and matter is located relative to other matter and the curvaceous field itself. This sounds hard and it is but Relativists have been working with backgroundlessness (no fixed prior geometric setup) since 1915. If a branch of physics has coped with this for almost 90 years it can't be an intellectual impossibility.

Still you get, in "Dialog on quantum gravity", the pitiful cry of Professor Simp "What are the fields defined ON?"

It's worth anybody's time trying to understand, in my opinion. In the quantum theory factoring out smooth deformations of the manifold leads to cataloging the quantum states of geometry by polymer-like networks

matter fields have to be defined on these polymeric "excitations" of space. It is a Rovelli proverb that "matter cannot exist where geometry is not excited"

it is the excitations that give area and volume to surfaces and regions. if there is no polymer somewhere then it is nowhere and matter cannot be nowhere

In the dialog, the grad student Sal tells Professor Simp that the fields are defined on top of themselves. This is what happens with a diffeo-invarient theory----smooth deformation is "gauge" and gets factored out-----when the physically meaningless and arbitrariness (the "gauge") has been squeezed out of the picture what is left is the field (or the graph-like quantum excitations of the field) allowing essential relationships among things to be expressed.

The joke is that this isn't new. General Relativity has always been diffeo-invariant, backgroundless, whatever you want to call it, since its 1915 inception and it has worked fine. The manifold you start with has always been just a convenience for getting started defining stuff, points in it have always been known to be physically meaningless. Motion location rotation and all that good stuff has always, in GR, meant "relative to the field".

Nice thing about Einstein is that he agonized between 1912 and 1915 over whether to have the theory diffeo-invariant because he realized how radical it was. Not to be embarrassed if the GR concept of spacetime seems strange---to you, to me, to Professor Simp.

Note, this is not Special Relativity stuff, which is the 1905 theory and has time dilation and space contraction and the speed-of-light speedlimit and moving observers Anne and Bob in their rocketships and all that. We are not talking about 1905 Special stuff. The 1915 step was REALLY different, with a really radically new idea of space and time, and maybe we should discuss it some.

I think standard model physics will probably be rebuilt in a background-independent fashion. selfAdjoint said something like that in a thumbnail sketch of "Rovelli's vision" in another thread
 
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I think the idea of background-independence is here to stay, and it will be a driving factor in theoretical physics for many years to come.
 
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The shift in theoretical physics towards a focus on spacetime geometry and the need to quantize GR is a significant development in the field. This change is being driven by the increasing relevance of cosmology and the need to understand the fundamental nature of the universe. The concept of spacetime in GR is vastly different from that in other theories, and this has led to a deeper understanding of the relationship between matter and the gravitational field. The idea of a backgroundless spacetime, where matter is located relative to other matter and the gravitational field, challenges traditional notions of space and time. However, this concept has been successfully utilized in GR since its inception in 1915. The recent emphasis on diffeo-invariant theories and the concept of polymer-like networks as excitations of space reveals a deeper understanding of the relationship between matter and geometry. This shift in theoretical physics is a testament to the ongoing evolution of our understanding of the universe and the importance of constantly questioning and challenging our existing theories. It will be interesting to see how this shift will impact our understanding of the standard model and how it will shape the future of theoretical physics.
 
"Supernovae evidence for foundational change to cosmological models" https://arxiv.org/pdf/2412.15143 The paper claims: We compare the standard homogeneous cosmological model, i.e., spatially flat ΛCDM, and the timescape cosmology which invokes backreaction of inhomogeneities. Timescape, while statistically homogeneous and isotropic, departs from average Friedmann-Lemaître-Robertson-Walker evolution, and replaces dark energy by kinetic gravitational energy and its gradients, in explaining...

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