Conservation of Energy on the Cosmological Scale

In summary, energy conservation in General Relativity is valid locally for all types of stress-energy, including dark energy. However, in a general curved spacetime, there is no global energy conservation law. This is due to the fact that spacetime becomes dynamical in GR, and can exchange energy with its constituents. This enables one to define energy conservation globally, but it requires certain symmetries that may not exist in cosmology. Therefore, the source of dark energy may not obey this principle, but this is not a question that falls within the definable scope of present-day cosmology.
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Islam Hassan
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Am I correct in understanding that locally, ie, with respect to circumscribable phenomena, conservation of energy is valid in the cosmos but that otherwise it is/may not be?

Otherwise said, the source of dark energy does/may not obey this principle? Or is this a question that does not fall within the definable scope of present-day cosmology?IH
 
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Conservation of energy in General Relativity means that the covariant divergence of the stress-energy tensor is zero. Physically, this means that stress-energy cannot be created or destroyed in any infinitesimal volume of spacetime. This is true for all types of stress-energy, including dark energy. This conservation law is local.

In a general curved spacetime, there is no global energy conservation law for stress-energy. Sean Carroll gives a good discussion of this here:

http://www.preposterousuniverse.com/blog/2010/02/22/energy-is-not-conserved/
 
  • #3
Islam Hassan said:
Am I correct in understanding that locally, ie, with respect to circumscribable phenomena, conservation of energy is valid in the cosmos but that otherwise it is/may not be?

Otherwise said, the source of dark energy does/may not obey this principle? Or is this a question that does not fall within the definable scope of present-day cosmology?IH
Energy conservation is subtle in GR. Without GR, we define energy as a conserved Noether current in a fixed spacetime. Spacetime is just a stage, doing nothing. However, in GR, spacetime becomes dynamical and can exchange energy with its constituents. But the subtlety is that locally, a gravitational field can always be interpreted as you accelerating. Globally this is not possible, because curvature manifests itself unambigously at a global scale. So this enables one to define energy conservation globally. For this however one needs, as in the not-GR case, symmetries. For cosmology one needs a so-called timelike Killing vector of a deSitter solution, and to my understanding such a Killing vector does not exist.

The subtlety in energy conservation already follows from the observation that in an expanding spacetime with constant energy density (the cosmological constant being interpreted as an energy density!) energy seems to be created out of nothing. However, this apparent "paradox" arises from not understanding energy conservation in dynamical spacetimes.

This is also Carroll's statement in Peter's link, I guess.
 
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Related to Conservation of Energy on the Cosmological Scale

1. What is the concept of conservation of energy on the cosmological scale?

The law of conservation of energy states that energy can neither be created nor destroyed, but can only be transformed from one form to another. This concept applies to the entire universe, including the cosmological scale, where energy is constantly being exchanged and transformed between different systems and objects.

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

The expansion of the universe is governed by the laws of thermodynamics, which include the conservation of energy. As the universe expands, the energy within it remains constant, but it may be transformed from one form to another, such as from potential energy to kinetic energy.

3. Can the conservation of energy be violated on the cosmological scale?

No, the conservation of energy is a fundamental law of physics and cannot be violated on any scale, including the cosmological scale. While energy may appear to be lost or gained in certain processes, it is simply being transformed into a different form.

4. How does dark energy fit into the concept of conservation of energy on the cosmological scale?

Dark energy, a mysterious force that is responsible for the accelerating expansion of the universe, is thought to be a form of energy that exists throughout space. While its exact nature is still not fully understood, it is believed to be consistent with the conservation of energy as it does not create or destroy energy, but rather acts as a driving force for the expansion of the universe.

5. Is the conservation of energy relevant to our understanding of the Big Bang theory?

Yes, the conservation of energy is a crucial concept in understanding the Big Bang theory. According to this theory, all the energy in the universe was present at the moment of the Big Bang and has been conserved and transformed throughout the history of the universe. This theory is supported by numerous observations and experiments, making the conservation of energy an essential principle in our understanding of the origins and evolution of the universe.

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