Derive Newtonian gravity from symmetry?

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Discussion Overview

The discussion explores the possibility of deriving Newtonian gravity from symmetries, particularly focusing on Gauss's law and spherical symmetry. Participants examine the relationship between these concepts and the foundational aspects of gravitational laws.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that Newtonian gravity can be derived from Gauss's law and the assumption of spherical symmetry.
  • Others argue that while Gauss's law can express gravitational flux as \(-4\pi Gm\), it may still rely on Newton's law to establish the relationship between gravitational acceleration and mass.
  • A later reply questions whether the gravitational flux can be derived independently of Newton's law, suggesting a potential equivalence between the two statements rather than a derivation.

Areas of Agreement / Disagreement

Participants express differing views on whether Gauss's law can be considered independent of Newton's law, indicating that multiple competing perspectives remain unresolved.

Contextual Notes

There are assumptions regarding spherical symmetry and the direction of gravitational acceleration that are not explicitly defined, which may affect the derivation process discussed.

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Is it possible to derive laws of Newtonian gravity from some symmetries?
 
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It can be derived from Gauss's law and spherical symmetry, if that's what you mean.
 
Meir Achuz said:
It can be derived from Gauss's law and spherical symmetry, if that's what you mean.

Is one more fundamental than the other? You can certainly consider a sphere ##S## centred on a point mass and look at ##\iint_S \vec{g} \cdot d\vec{A}= \iint_S -\frac{Gm}{r^2} \hat{r} \cdot d\vec{A} = -4\pi G m##, but can the constant on the right be obtained without referring to Newton's law of gravitation in the first place?
 
You just have to assume spherical symmetry, including that \vec g is in the radial direction.
Then, \int\int{\vec g}\cdot{\vec{dA}}=-g\int\int dA=-4\pi R^2=-4\pi Gm.
 
Meir Achuz said:
You just have to assume spherical symmetry, including that \vec g is in the radial direction.
Then, \int\int{\vec g}\cdot{\vec{dA}}=-g\int\int dA=-4\pi R^2=-4\pi Gm.

But don't we still need to use that ##g = \frac{Gm}{r^2}##, Newton's law, in order to get that ##-g\iint dA = -4\pi R^2 \frac{Gm}{r^2} = -4\pi G m##? In other words, is there a way to derive that the gravitational flux is ##-4\pi G m## without referring to Newton's law of gravitation?
 
Why do you say that? Gauss's law is \int\int{\vec g}\cdot{\vec{dA}}=-4\pi Gm, with no mention of Newton's law.
 
Meir Achuz said:
Why do you say that? Gauss's law is \int\int{\vec g}\cdot{\vec{dA}}=-4\pi Gm, with no mention of Newton's law.

Fair enough, my point was just that the two seem to be equivalent statements of the same law, and it is not so much deriving one from the other as re-stating it in a different form.
 

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