Is energy conserved in an expanding universe?

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Discussion Overview

The discussion centers around the conservation of energy in the context of an expanding universe, particularly examining the implications of General Relativity (GR) and Quantum Mechanics (QM) on this topic. Participants explore whether the expansion of space affects vacuum energy and how this relates to the law of conservation of energy, while referencing cosmological models and interpretations of spacetime.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants argue that while space is expanding, it is not "empty space" that expands, but rather objects moving apart within it.
  • Others propose that the expansion of space could imply an increase in vacuum energy, raising questions about energy conservation in this context.
  • A participant mentions that energy conservation in GR is complex and depends on the definitions used, noting that it is not conserved in general for expanding cosmologies.
  • Some contributors assert that there are various cosmological models, with differing views on whether energy is conserved, not conserved, or even increasing.
  • There is a suggestion that the phrase "expanding space" is often used in popular literature but may not accurately reflect the complexities of GR.
  • Participants express uncertainty about the implications of energy conservation in the large-scale structure of the universe, referencing previous discussions without reaching a consensus.

Areas of Agreement / Disagreement

Participants generally disagree on the interpretation of energy conservation in an expanding universe, with multiple competing views presented. The discussion remains unresolved regarding the implications of these interpretations.

Contextual Notes

Limitations include the lack of consensus on the definitions of energy and conservation in the context of GR, as well as the dependence on specific cosmological models that may not be universally accepted or tested.

  • #31
Cosmic static and binding energies?

Thanks pervect.

pervect said:
You've definitely computed some sort of number. The physical significance of this number is somewhat questionable. You might want to question why you consider this number to represent any sort of "energy".

I understand that 'rest energy' in this context is problematic but why I considered 'this number to represent any sort of "energy"' is probably not so problematic. Since we know the co-moving size and the critical energy density of the observable universe, we can easily calculate a present 'static' energy component of 2.62E+71 Joule for the observable universe. Is it not reasonable to say that this number represents some valid component of the total energy?

OK, the frame dependence remains, but it may be valid in our 'observational frame', whatever that means. Anyway, the next step could be to calculate the negative gravitational binding energy from this value. You said:

pervect said:
Another thing missing from your formula for "energy" would be any concept of "gravitational binding energy". For instance, the Newtonian gravitational binding energy of a sphere of mass M depends on its radius, R, by the formula

E = -G M^2 / r

Based on this and the 2.62E+71 Joule (or 2.92E+54 kg) 'static energy' of the observable universe and taking the co-moving radius as 46 Gly, or 4.35E+26 m, I get a present binding energy of -1.30E+72 Joule.

If this is correct, can one then conclude that the positive energy of expansion (the 'kinetic' energy?) is 1.30E+72 Joule, so that the total (binding + expansion) energy of the observable universe is zero for the Omega=1 case?

If all the above make any sense, (which I doubt somehow) one can calculate the variable static and expansion energies over the history of the universe as per the attached graph. This is an "engineering approach", which I hope is not considered too "agricultural"!:wink:
 

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  • #32
Jorrie said:
OK, the frame dependence remains, but it may be valid in our 'observational frame', whatever that means. Anyway, the next step could be to calculate the negative gravitational binding energy from this value. You said:

If this is correct, can one then conclude that the positive energy of expansion (the 'kinetic' energy?) is 1.30E+72 Joule, so that the total (binding + expansion) energy of the observable universe is zero for the Omega=1 case?

If all the above make any sense, (which I doubt somehow) one can calculate the variable static and expansion energies over the history of the universe as per the attached graph. This is an "engineering approach", which I hope is not considered too "agricultural"!:wink:

How to put this: I would not recommend trying to get the above analysis published in a peer-reviewed journal :wink:

Note that the formula I gave for binding energy was a Newtonian formula - not a GR formula. As I have been trying to explain, a GR formula just doesn't exist, at least not for the case of the universe - there are many situations in which GR does define an energy, the universe as a whole happens not to be one of them.

So you're (slightly) better off not including the binding energy rather than applying a Newtonian formula in an area where you know it won't give the right answer. (It would be best if this were a conscious omission). But basically the whole approach is so badly flawed as to be not worth very much, and if you talk to anyone knowledgeable about GR about the "energy of the universe" you shouldn't be too surprised if you get negative reactions or "funny looks".
 
  • #33
pervect said:
So you're (slightly) better off not including the binding energy rather than applying a Newtonian formula in an area where you know it won't give the right answer. (It would be best if this were a conscious omission). But basically the whole approach is so badly flawed as to be not worth very much, and if you talk to anyone knowledgeable about GR about the "energy of the universe" you shouldn't be too surprised if you get negative reactions or "funny looks".

OK, thanks again, I expected something to this effect.

One final question: if I drop the 'observable universe' as a basis and just consider a large, finite region that is fairly homogeneous, would the [edit: 'evolution over time of the'] 'static energy' (including all forms) still be fundamentally flawed as a concept?
 
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