Derive Newtonian gravity from symmetry?

In summary: So it would be accurate to say that one is more fundamental than the other.In summary, it is possible to derive laws of Newtonian gravity from some symmetries. It can be derived from Gauss's law and spherical symmetry, if that's what you mean.
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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.
 
  • #3
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?
 
  • #4
You just have to assume spherical symmetry, including that [itex]\vec g[/itex] is in the radial direction.
Then, [itex]\int\int{\vec g}\cdot{\vec{dA}}=-g\int\int dA=-4\pi R^2=-4\pi Gm[/itex].
 
  • #5
Meir Achuz said:
You just have to assume spherical symmetry, including that [itex]\vec g[/itex] is in the radial direction.
Then, [itex]\int\int{\vec g}\cdot{\vec{dA}}=-g\int\int dA=-4\pi R^2=-4\pi Gm[/itex].

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?
 
  • #6
Why do you say that? Gauss's law is [itex]\int\int{\vec g}\cdot{\vec{dA}}=-4\pi Gm[/itex], with no mention of Newton's law.
 
  • #7
Meir Achuz said:
Why do you say that? Gauss's law is [itex]\int\int{\vec g}\cdot{\vec{dA}}=-4\pi Gm[/itex], 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.
 

1. What is the concept of symmetry in relation to Newtonian gravity?

Symmetry is the idea that certain physical laws and phenomena remain unchanged or invariant under certain transformations. In the case of Newtonian gravity, this refers to the symmetry of space and time, meaning that the laws of gravity are the same regardless of where or when they are observed.

2. How does symmetry help to derive Newtonian gravity?

By assuming the symmetry of space and time, we can use mathematical equations and principles to derive the laws of gravity. This is known as the principle of least action, which states that the path an object takes between two points is the one that minimizes the action (or energy) required. This leads to the equations of motion for objects under the influence of gravity.

3. What are the key equations used to derive Newtonian gravity from symmetry?

The key equations used are Newton's second law of motion (F=ma), the law of universal gravitation (F=Gm1m2/r^2), and the principle of least action (S=∫Ldt). These equations, along with the assumption of symmetry, can be used to derive the equations of motion for objects under the influence of gravity.

4. Are there any limitations to deriving Newtonian gravity from symmetry?

Yes, there are some limitations to this approach. For example, it does not take into account the effects of relativity or quantum mechanics, which are necessary for understanding gravity on a larger scale. Additionally, it only applies to objects with mass and does not account for more complex phenomena such as dark matter.

5. How does the concept of symmetry apply to other areas of science and physics?

Symmetry is a fundamental concept in many areas of science and physics. It is used to explain and understand various phenomena, from the behavior of subatomic particles to the structure of the universe. It also plays a crucial role in the development of theories and laws, such as the laws of thermodynamics and conservation of energy.

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