Research on conservation of spacetime curvature

In summary, the conversation is about the properties that are transferred by different types of bosons in quantum physics. The first 4 properties (electric charge, color charge, weak isospin, and a combination of weak isospin and weak hypercharge) are conserved. The question then arises if spacetime curvature, which is a tensor and not a conserved quantity in general relativity, could also be conserved. There is a discussion about this on a physics forum, but it is mentioned that discussing personal research or speculations is not the purpose of the forum. The conversation ends with the thread being closed.
  • #1
Structure seeker
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TL;DR Summary
Is there any research done on conservation of (integrated over all spacetime) spacetime curvature?
After trying to kinda get a picture of the field of play in quantum physics according to the standard model, a question came up. I tried to formulate the known bosons each as a particle transferring some property.

1. Photons transfer electric charge: the electromagnetic force gives attraction between positive and negative charges so an electronic current
2. Gluons transfer color charge
3. The 3 weak bosons transfer weak isospin
4. The Higgs mechanism transfers a combination of weak isospin and weak hypercharge
5. Gravitons, if they exist, transfer spacetime curvature?

The first 4 properties transferred are conserved (by quantum conservation laws). My question is: has any research been done on whether spacetime curvature (integrated over all of it) could be conserved? I'm especially interested in loop quantum gravity views on this matter (hope I can sort of understand that but OK)

The only thing I found on internet is a physics stackexchange question https://physics.stackexchange.com/questions/130379/conservation-in-space-time-curvature where the question is waved away with the observation that the universe at large is not curved, so what curvature? But IMO that might be in fact an indication that every negative curvature induces an equal opposite positive curvature somehow.
 
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  • #2
Structure seeker said:
has any research been done on whether spacetime curvature (integrated over all of it) could be conserved?
"Spacetime curvature" is not even a number; it's a tensor. In GR it is not a conserved quantity.

Structure seeker said:
the question is waved away with the observation that the universe at large is not curved
This answer confuses spacetime curvature with spatial curvature in our best current model of our universe. They're not the same.
 
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  • #3
I'm not a physicist but more a hobbyist in the area of mathematical physics, so whether it matches GR or not is outside my area of expertise.

Regardless, taking the analysis I made seriously could lead to interesting viewpoints or directions to new theories. It's clear this analysis got no critique, so the observations I made are somewhat peer-reviewed now. But no wild speculation here please.
 
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  • #4
Structure seeker said:
It's clear this analysis got no critique
...apart from Peter pointing out that curvature is a tensor, not a number, which renders questions about a "total curvature" meaningless, even before you get to questions about conservation.
 
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  • #7
Structure seeker said:
It's clear this analysis got no critique, so the observations I made are somewhat peer-reviewed now.
If by this you mean that you think the fact that nobody has given you a detailed refutation implies that we think there is some value in your speculations, you are wrong.

Structure seeker said:
taking the analysis I made seriously could lead to interesting viewpoints or directions to new theories.
That is not what PF is for. PF is not for discussion of personal research or personal speculations. It is to help people understand physics that is already mainstream. If you think there is something useful in the speculations you are making, get a peer-reviewed paper published.

Thread closed.
 
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FAQ: Research on conservation of spacetime curvature

What is the conservation of spacetime curvature?

The conservation of spacetime curvature refers to the principle that the curvature of spacetime, as described by General Relativity, remains consistent and is governed by the Einstein field equations. These equations relate the distribution of matter and energy to the curvature of spacetime, ensuring that the overall geometry is conserved in a way that aligns with physical laws.

How does the conservation of spacetime curvature relate to General Relativity?

In General Relativity, the conservation of spacetime curvature is a direct consequence of the Einstein field equations. These equations dictate how matter and energy influence the curvature of spacetime. The conservation principles ensure that the total curvature is balanced by the presence of matter and energy, maintaining the consistency of the spacetime fabric.

What are the practical implications of studying spacetime curvature conservation?

Studying the conservation of spacetime curvature has profound implications for our understanding of the universe. It helps in predicting the behavior of celestial bodies, understanding black holes, gravitational waves, and the expansion of the universe. This research can also lead to advancements in technologies like GPS, which relies on precise measurements of spacetime curvature.

Can the curvature of spacetime be directly measured?

While we cannot directly measure the curvature of spacetime, we can observe its effects. For example, the bending of light around massive objects (gravitational lensing), the orbit of planets, and the behavior of galaxies all provide indirect evidence of spacetime curvature. Instruments like the Laser Interferometer Gravitational-Wave Observatory (LIGO) detect gravitational waves, which are ripples in spacetime curvature.

What challenges do scientists face in researching spacetime curvature conservation?

One of the main challenges is the extreme conditions under which significant curvature effects occur, such as near black holes or during the early moments of the universe. These environments are difficult to replicate or observe directly. Additionally, the mathematical complexity of the Einstein field equations makes it challenging to find exact solutions or to model scenarios accurately. Advanced computational methods and innovative observational techniques are essential to overcome these challenges.

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