Gravity in Hollow Shell: Nonadditivity and Relativistic Self-Interaction

In summary, classical gravity obeys Gauss' law and does not exhibit gravity in a hollow, spherically symmetric shell. However, in general relativity, gravity is not additive and can be seen in the example of a black hole where the field flux diverges to infinity at a nonzero distance. The gravity of any mass distribution is also nonadditive, leading to an increase in flux inwards. Birkhoff's theorem states that the only spherically symmetric vacuum solution in general relativity is Schwarzschild's, which depends on the enclosed mass. Therefore, in a non-moving hollow shell, the interior metric is Minkowski. However, if the hollow shell is rotating, there may be a Lense-Thirring effect
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snorkack
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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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  • #2
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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  • #3
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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1. What is the significance of "nonadditivity" in the context of gravity in a hollow shell?

Nonadditivity refers to the fact that the total gravitational force experienced by an object inside a hollow shell is not equal to the sum of the forces exerted by each individual mass element of the shell. This is a consequence of the shell theorem, which states that the gravitational force inside a hollow spherical shell is zero.

2. How does relativistic self-interaction affect the behavior of gravity in a hollow shell?

Relativistic self-interaction refers to the fact that the motion of a mass element in a hollow shell is affected by the gravitational pull of other mass elements in the shell. This self-interaction leads to a nonadditive behavior of gravity in the shell, as described by the nonadditivity factor in the formula for the gravitational force.

3. Can you explain the concept of "gravity in a hollow shell" in layman's terms?

Gravity in a hollow shell refers to the gravitational force experienced by an object inside a spherical shell that has a uniform mass distribution. In this scenario, the gravitational force experienced by the object is a combination of the gravitational pull of all the mass elements in the shell, taking into account both Newtonian and relativistic effects.

4. How does the formula for gravity in a hollow shell differ from the formula for gravity in a solid sphere?

The formula for gravity in a hollow shell takes into account the nonadditive behavior and relativistic self-interaction of gravity in the shell, while the formula for gravity in a solid sphere only considers the gravitational pull of the mass elements inside the sphere. As a result, the formula for gravity in a hollow shell is more complex and involves additional factors to account for these effects.

5. What are the practical applications of understanding gravity in a hollow shell?

Understanding the nonadditive and relativistic behavior of gravity in a hollow shell is important for accurately predicting and modeling the motion of objects in space, such as planets, stars, and galaxies. It also has implications for the study of general relativity and the behavior of gravity in extreme conditions, such as near black holes.

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