Conservation of Energy on the Cosmological Scale

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SUMMARY

In the context of General Relativity (GR), conservation of energy is locally valid, meaning that within circumscribable phenomena, the covariant divergence of the stress-energy tensor is zero. However, globally, energy conservation does not hold due to the dynamical nature of spacetime, which can exchange energy with its constituents. This leads to complexities, particularly regarding dark energy, where the lack of a timelike Killing vector in de Sitter solutions prevents a global conservation law. The discussion references Sean Carroll's insights on the subtleties of energy conservation in expanding spacetimes.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with the stress-energy tensor
  • Knowledge of cosmological constants and dark energy
  • Concept of Killing vectors in differential geometry
NEXT STEPS
  • Study Sean Carroll's blog on energy conservation in cosmology
  • Explore the implications of the cosmological constant in GR
  • Learn about the role of Killing vectors in curved spacetime
  • Investigate the relationship between energy density and expanding spacetimes
USEFUL FOR

Astronomers, physicists, and cosmologists interested in the implications of General Relativity on energy conservation and the nature of dark energy.

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/
 
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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