Energy conservation in an expanding universe

In summary, Alan Guth's lecture states that the total amount of energy is still conserved, even in an expanding universe based on a positive and constant energy density. However, this statement is only true if you define the "total amount of energy" to be a pseudotensor.
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elcaro
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TL;DR Summary
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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FAQ: Energy conservation in an expanding universe

What is energy conservation in an expanding universe?

Energy conservation in an expanding universe refers to the idea that the total energy of the universe remains constant as it expands. This means that while the distribution of energy may change, the overall amount of energy in the universe does not.

How does energy conservation apply to the expansion of the universe?

According to the first law of thermodynamics, energy can neither be created nor destroyed, only converted from one form to another. This means that as the universe expands, the energy within it may be transformed into different forms, but the total amount of energy remains the same.

What evidence supports the concept of energy conservation in an expanding universe?

One major piece of evidence is the cosmic microwave background radiation, which is a remnant of the hot, dense early universe. This radiation is evenly distributed throughout the universe, indicating that the total energy of the universe has remained constant throughout its expansion.

How does dark energy affect energy conservation in an expanding universe?

Dark energy is a mysterious force that is thought to be responsible for the accelerating expansion of the universe. While it may seem like this would violate the principle of energy conservation, it is believed that dark energy is a form of energy that is inherent to the fabric of space itself and does not violate the laws of thermodynamics.

What are the implications of energy conservation in an expanding universe for the future of the universe?

If energy conservation holds true, it suggests that the universe will continue to expand indefinitely, with the total energy remaining constant. This could have implications for the ultimate fate of the universe, as well as the potential for the existence of other universes beyond our own.

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