Energy conservation in an expanding universe

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SUMMARY

The discussion centers on the conservation of energy in an expanding universe, emphasizing that the total amount of energy remains conserved even during rapid inflation, as explained by Alan Guth. However, this conservation is contingent upon defining "the total amount of energy" as a pseudotensor, which is not invariant and relies on specific coordinate choices. Most physicists in General Relativity argue that physical laws should be expressed in terms of invariants, rendering coordinate-dependent quantities meaningless. Additionally, the Hamiltonian constraint in General Relativity suggests that the total energy of the universe could be zero, complicating the traditional understanding of energy conservation.

PREREQUISITES
  • Understanding of General Relativity concepts
  • Familiarity with pseudotensors and their implications
  • Knowledge of inflationary cosmology and Alan Guth's contributions
  • Basic grasp of Hamiltonian mechanics in the context of physics
NEXT STEPS
  • Explore Alan Guth's lecture on inflationary cosmology
  • Read Sean Carroll's article on energy conservation in the universe
  • Investigate the implications of the Hamiltonian constraint in General Relativity
  • Study the differences between invariant quantities and pseudotensors in physics
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Physicists, cosmologists, and students of theoretical physics interested in the nuances of energy conservation in the context of an expanding universe and General Relativity.

elcaro
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TL;DR
In an universe with positive and constant energy density the total amount of energy seems not to be conserved. However, if one also considers the negative energy contained in the gravitaional potential, which can become arbitrarily negative, then total energy in the universe IS conserved.
The total amount of energy is still a conserved quantity, even in an expanding universe based on a positive and constant energy density, and even under the rapid exponential expansion during inflation, total amount of energy is conserved. For how this works, see this lecture by Alan Guth, the father of inflationary cosmology.
 
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elcaro said:
The total amount of energy is still a conserved quantity
Only if you define "the total amount of energy" to be a pseudotensor. But a pseudotensor is not an invariant; it depends on a particular choice of coordinates. The viewpoint of most physicists working in General Relativity is that all of the physics is contained in invariants, and coordinate-dependent quantities have no physical meaning.

For a different viewpoint than Guth's, see, for example, this article by Sean Carroll (which you will find referenced fairly frequently here on PF when this subject comes up):

https://www.preposterousuniverse.com/blog/2010/02/22/energy-is-not-conserved/
 
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elcaro said:
The total amount of energy is still a conserved quantity
Note, btw, that there is another possible interpretation of this statement besides the pseudotensor one, which might be being implicitly used (at least in part) in Slide 6 of the lecture slides corresponding to the video you gave:

https://ocw.mit.edu/courses/physics...all-2013/lecture-slides/MIT8_286F13_lec01.pdf

At the bottom of this slide, it says: "The TOTAL ENERGY of the universe may very well be zero." There is a quantity called the "Hamiltonian constraint" (IIRC) in GR, which is in fact identically zero for any spacetime that is a solution of the Einstein Field Equation. If we interpret this Hamiltonian as "the total energy" of the solution, then this means the total energy is zero.

However, in this formulation, there is no split in this "total energy" between "positive energy of material" and "negative potential energy in the gravitational field"; the total energy is just zero. To get the split described in the lecture between the "positive" and "negative" parts of the total energy, you need to pick a pseudotensor, which has the problem I described in my last post.
 
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