Gravity/conservation of energy?

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SUMMARY

The discussion centers on the complexities of energy conservation in the context of General Relativity (GR), particularly regarding gravitational fields and potential energy. It highlights that while energy conservation holds in flat spacetime, the situation becomes intricate in curved spacetimes, where the equivalence of differential and integral formulations of energy conservation breaks down. Key references include the textbook "Gravitation" by Misner, Thorne, and Wheeler (MTW) and a FAQ on gravitational energy by John Baez. Understanding these concepts requires careful consideration of the definitions of energy and conservation in GR.

PREREQUISITES
  • Understanding of General Relativity (GR) principles
  • Familiarity with gravitational potential energy concepts
  • Knowledge of differential and integral equations
  • Basic grasp of spacetime curvature
NEXT STEPS
  • Read "Gravitation" by Misner, Thorne, and Wheeler for in-depth understanding of energy in GR
  • Explore John Baez's FAQ on gravitational energy for layperson-friendly explanations
  • Study the differences between energy conservation in flat and curved spacetimes
  • Investigate the mathematical formulations of energy conservation in differential and integral forms
USEFUL FOR

Students of physics, researchers in gravitational theory, and anyone seeking to understand the nuances of energy conservation in General Relativity.

navonoD
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If gravity is warped space time, and potential/kenetic energy can be derived from gravities effect on mass, apparently without exhausting any energy, how can conservation of energy hold true?
I'm not arguing in any sense, i just really don't get it... NEone?
 
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This is a FAQ, asked on average every week here.

Localization of gravitational field energy, and "gravitational potential energy", are very tricky concepts in gtr, for mathematical reasons. See the discussion in MTW, Gravitation or other good textbooks.
 
The usual FAQ oriented towards the layperson is at http://math.ucr.edu/home/baez/physics/Relativity/GR/energy_gr.html

Here's a very short quote from the introduction:

Is Energy Conserved in General Relativity?

In special cases, yes. In general -- it depends on what you mean by "energy", and what you mean by "conserved".

In flat spacetime (the backdrop for special relativity) you can phrase energy conservation in two ways: as a differential equation, or as an equation involving integrals (gory details below). The two formulations are mathematically equivalent. But when you try to generalize this to curved spacetimes (the arena for general relativity) this equivalence breaks down. The differential form extends with nary a hiccup; not so the integral form.

I'll encourage interested people to read the original in its entirety (due to copyright and other reasons, it's not appropriate to repost it, but to rerfer people to the original).
 

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