A change going on in theoretical physics

In summary, there has been a recent shift in theoretical physics where spacetime geometry has become the main driver of research, particularly in the areas of cosmology, black holes, and the early universe. This has led to a renewed interest in quantizing General Relativity, which has a different concept of space and time compared to other theories. The concept of backgroundlessness in GR has been a topic of discussion, with some struggling to understand the idea of fields being defined on top of themselves. However, this idea is not new as GR has always been diffeo-invariant and has worked well for almost 90 years. It is believed that background-independence will continue to be a major factor in theoretical physics and may even lead to the rebuilding
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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.
 

1. What is the current change happening in theoretical physics?

The current change going on in theoretical physics is the shift towards more holistic and unified theories, such as string theory and the search for a grand unified theory. This change is also characterized by a focus on understanding the fundamental building blocks of the universe and the laws that govern them.

2. How does this change impact our understanding of the universe?

This change in theoretical physics has the potential to greatly impact our understanding of the universe by providing a more comprehensive and cohesive framework for explaining the laws of nature. It also opens up new possibilities for technological advancements and practical applications.

3. What are the implications of this change for current theories in physics?

This change in theoretical physics may challenge some current theories and models, as it seeks to reconcile conflicting ideas and unify different branches of physics. However, it also has the potential to provide a more complete and accurate understanding of the universe.

4. How does this change affect the research being done in theoretical physics?

This change in theoretical physics has sparked new areas of research and collaboration among scientists, as they work towards finding a unified theory. It also requires a multidisciplinary approach, with physicists working alongside mathematicians and other scientists to tackle complex problems.

5. What are the potential benefits of this change for society?

The potential benefits of this change in theoretical physics for society are vast. It could lead to advancements in technology, medicine, and energy production, as well as a deeper understanding of the universe and our place in it. It also has the potential to inspire future generations of scientists and push the boundaries of human knowledge.

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