B Do EFEs Physically Describe Something?

  • Thread starter Thread starter Megaton
  • Start date Start date
Click For Summary
The Einstein field equations (EFEs) in general relativity (GR) relate stress-energy, which includes energy, momentum, and pressure, to spacetime curvature, allowing for the description of various gravitating objects like planets and stars. While the EFEs provide a mathematical framework, they can also yield physical predictions, such as frame dragging effects around massive bodies. The geodesic equation, which explains gravity's effects, is distinct from the EFEs but is necessary for understanding motion in curved spacetime. Topology and geometry are different concepts; the EFEs primarily address geometric aspects of spacetime rather than topological properties. Overall, the EFEs serve as both a mathematical tool and a means to describe physical phenomena in the universe.
Megaton
Messages
9
Reaction score
1
Hi I'm new to this so please don't butcher me. I am just a enthusiastic individual with a huge interest in theoretical physics.

In GR, the Einstein field equations relate energy and momentum (I think) to curvature, then to local flat geometry (I think) my question is do the EFEs physically describe something (ie: a rotating spherical object like Earth or a large nebula etc...) or are they a purely mathematical tool used to describe local geometry in relation to energy and momentum. I know the geodesic equation is needed to explain the "force" of gravity which results, I'm just wondering if they also to describe the topology as well.

I have always found this confusing, and can not seem to get a clear answer on it, thanks to anyone would cold help.
 
Physics news on Phys.org
Megaton said:
the Einstein field equations relate energy and momentum (I think) to curvature

More precisely, they relate stress-energy, which includes energy and momentum (density) but also includes pressure and other stresses, to a portion of curvature, the Einstein tensor.

Megaton said:
then to local flat geometry

I'm not sure what you mean by this. The fact that spacetime can be considered flat locally is not due to the EFE (although the EFE is certainly consistent with it).

Megaton said:
do the EFEs physically describe something (ie: a rotating spherical object like Earth or a large nebula etc...)

Solutions to the EFE, i.e., metric tensors, physically describe spacetimes that can contain various kinds of gravitating objects, like planets, stars, black holes, etc.

Megaton said:
I know the geodesic equation is needed to explain the "force" of gravity

The geodesic equation is not the same as the EFE.

Megaton said:
i'm just wondering if they also to describe the topology as well.

The topology is something else again; topology is not the same as geometry.
 
  • Like
Likes Megaton
You can think of the Field Equations as like Newton's law of gravity (note: the EFEs aren't quite equivalent to the Newtonian force equation - but it'll do for this explanation). Both tell you how gravity works in a general sense, but you need to feed in specific details in order to describe a specific situation. So, for example, to describe the solar system in Newtonian gravity you would write the gravitational force on a small mass m as
$$\vec F=-Gm\left (
\frac {M_{sun}}{|\vec r- \vec r_{sun}|^3}(\vec r- \vec r_{sun})+
\frac {M_{mercury}}{|\vec r- \vec r_{mercury}|^3}(\vec r- \vec r_{mercury})+
\frac {M_{venus}}{|\vec r- \vec r_{venus}|^3}(\vec r- \vec r_{venus})+\ldots\right) $$
plus terms for all other planets, moons, etc. Which is rather more complicated than ##F=GMm/r^2##.

The EFEs are (mathematically) worse than Newtonian gravity for a number of reasons. First, as you and Peter noted, there are more things than just mass that go into the "source" term. Secondly, the equations are non-linear, so the solution for mass 1 plus the solution for mass 2 is not the same as the solution for mass 1 plus mass 2. The combination of the two (and other factors, like an extra dimension) is why I can write the Newtonian solution for multiple point masses off the top of my head but you need computer support to do the same thing for the full GR solution.

As Peter says, topology and geometry are different things. A good example is the Asteroids computer game. The whole thing takes place in flat space described by Euclidean geometry. If you couldn't move your spaceship off the edge of the screen, that would be a finite bounded Euclidean space - the topology and geometry of a sheet of paper. But the game let's you move off one edge of the screen and on to the opposite edge. The geometry is the same (triangles have 180 degree interior angles, circles have ##c=2\pi r## etc.), but the topology is toroidal - like the surface of a donut.
 
Last edited:
  • Like
Likes Megaton
Megaton said:
Hi I'm new to this so please don't butcher me. I am just a enthusiastic individual with a huge interest in theoretical physics.

In GR, the Einstein field equations relate energy and momentum (I think) to curvature, then to local flat geometry (I think) my question is do the EFEs physically describe something (ie: a rotating spherical object like Earth or a large nebula etc...) or are they a purely mathematical tool used to describe local geometry in relation to energy and momentum. I know the geodesic equation is needed to explain the "force" of gravity which results, I'm just wondering if they also to describe the topology as well.

I have always found this confusing, and can not seem to get a clear answer on it, thanks to anyone would cold help.

GR as a theory definitely makes experimental predictions. I'd go so far as to call them "physical" predictions, though it's not quite clear what that term means in abstract or to you.

I believe I recall reading that one doesn't need any more assumptions than the EFE to get the complete theory of GR, but perhaps I'm missing some small seemingly innocuous assumptions. For instance, I think I recall it being said that one doesn't need to assume geodesic motion of test particles as a separate assumption, but I also recall that there may be some seemingly innocuous assumptions required to prove that, related to the positivity of the energy density. I'm not sure if such seemingly fine points are of interest to you, though I suspect you're just looking for the "big picture".

The big picture would be that if you have a ball of matter, like a rotating Earth, you can get experimental predictions out of the math, for instance the "frame dragging" results of GPB, and other, less subtle, predictions.

You might find some situations where you would require information about the properties of the matter itself which is separate from the EFE's to make those predictions, and there might be some situations where the information is not known for a certanity. The structure of neutron stars would, I think, fall into this category, there are some reasonable theories about them, but I believe there may be some uncertanities in their structure relating not to the EFE's, but to the "physical" properties of neutron degenerate matter itself.

Sorry if this isn't an exact answer, but the question is general, and a lot depends on whether your trying to get a razor-sharp answer or just a general "feel".
 
  • Like
Likes Megaton
Thanks for your prompt answers that helps a lot.

I am currently studying philosophy and have a weird obsession with finding a Theory of everything. I understand that GR and QM (plus many other factors) are required to explain a TOE, and am curious to see what real world life applications a TOE would bring.

Understanding the overall picture of Theoretical Physics and Physical Cosmology are essential to understanding a TOE, which is what I am trying to do.

Thanks for all your help
 
In Birkhoff’s theorem, doesn’t assuming we can use r (defined as circumference divided by ## 2 \pi ## for any given sphere) as a coordinate across the spacetime implicitly assume that the spheres must always be getting bigger in some specific direction? Is there a version of the proof that doesn’t have this limitation? I’m thinking about if we made a similar move on 2-dimensional manifolds that ought to exhibit infinite order rotational symmetry. A cylinder would clearly fit, but if we...

Similar threads

  • · Replies 99 ·
4
Replies
99
Views
11K
  • · Replies 5 ·
Replies
5
Views
1K
Replies
39
Views
2K
Replies
3
Views
735
Replies
40
Views
7K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 58 ·
2
Replies
58
Views
3K
  • · Replies 28 ·
Replies
28
Views
2K
  • · Replies 9 ·
Replies
9
Views
1K
Replies
21
Views
3K