Gravity in Hollow Shell: Nonadditivity and Relativistic Self-Interaction

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SUMMARY

The discussion centers on the nonadditivity of gravity in general relativity, contrasting it with classical gravity, which is additive. It highlights that classical gravity obeys Gauss' law, resulting in the absence of gravitational effects within a hollow, spherically symmetric shell. In general relativity, the gravity of a mass distribution is nonadditive, with the flux increasing inward. Birkhoff's theorem confirms that the interior metric of a non-rotating hollow shell remains Minkowski, while a rotating shell introduces the Lense-Thirring effect, marking a divergence from Newtonian predictions.

PREREQUISITES
  • Understanding of Gauss' law in classical gravity
  • Familiarity with Einstein's field equations
  • Knowledge of Birkhoff's theorem
  • Concept of the Lense-Thirring effect in general relativity
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  • Study the implications of Birkhoff's theorem in various gravitational scenarios
  • Explore the mathematical formulation of Einstein's field equations
  • Investigate the properties of black holes and their gravitational effects
  • Learn about frame dragging and its significance in rotating mass distributions
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Physicists, astrophysicists, and students of general relativity seeking to deepen their understanding of gravitational interactions and the implications of nonadditivity in different mass distributions.

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Classical gravity is additive.
Therefore classical gravity obeys Gauss´ law. One result is absence of gravity in any hollow, spherically symmetric shell.

In general relativity, gravity is not additive.
Simple example is a black hole.
The gravity of a classical point mass diverges to infinity at zero distance, and the field flux is conserved. The gravity of a black hole diverges to infinity at a nonzero distance, and the field flux also diverges to infinity.

But the gravity of any mass distribution is nonadditive and the flux increases inwards.

Now, how does the relativistic self-interaction of gravity field work inside a hollow shell (that is not massive enough to be a black hole)? Does the field still cancel inside?
 
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Yes. Birkhoff's theorem says that the only spherically symmetric vacuum solution to Einstein's field equations is Schwarzschild's. And that only depends on the enclosed mass.
 
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If the hollow shell is not moving then Ibix's answer applies - Birkhoff's theorem says the interior metric is Minkowski. If the hollow shell is rotating though you will get a Lense-Thirring effect (frame dragging). That's the level (for this scenario) at which GR would depart from Newtonian predictions.
 
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