Do EFEs Physically Describe Something?

  • Context: High School 
  • Thread starter Thread starter Megaton
  • Start date Start date
Click For Summary

Discussion Overview

The discussion revolves around the physical interpretation of the Einstein field equations (EFEs) in general relativity (GR). Participants explore whether the EFEs describe physical entities, such as rotating objects or nebulae, or if they serve merely as mathematical tools for relating energy, momentum, and curvature in spacetime. The conversation touches on concepts of geometry, topology, and the implications of GR in experimental predictions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants suggest that the EFEs relate stress-energy, which includes energy, momentum, and pressure, to curvature through the Einstein tensor.
  • Others argue that while solutions to the EFEs can describe spacetimes with various gravitating objects, the EFEs themselves do not directly imply local flat geometry.
  • A participant compares the EFEs to Newton's law of gravity, noting that both require specific details to describe particular situations, but highlights the complexity of the EFEs due to their non-linear nature.
  • There is a discussion about the distinction between topology and geometry, with examples illustrating how they can differ despite having the same geometric properties.
  • One participant mentions that GR makes experimental predictions, suggesting that the EFEs can lead to physical predictions, though the clarity of what constitutes "physical" is questioned.
  • Concerns are raised about potential assumptions needed to derive results from the EFEs, particularly regarding the properties of matter in extreme conditions like neutron stars.

Areas of Agreement / Disagreement

Participants express varying views on whether the EFEs physically describe something or are purely mathematical. There is no consensus on the interpretation of the EFEs, and multiple competing views remain regarding their implications and the assumptions involved in their application.

Contextual Notes

Some participants note that the understanding of the EFEs may depend on additional assumptions about the properties of matter and energy, which could affect the predictions made using the equations. There is also mention of uncertainties related to specific physical scenarios, such as neutron stars.

Who May Find This Useful

This discussion may be of interest to individuals studying theoretical physics, general relativity, or those exploring the philosophical implications of a Theory of Everything (TOE). It could also benefit those curious about the relationship between mathematical formulations and physical reality in the context of GR.

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   Reactions: 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   Reactions: 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   Reactions: 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
 

Similar threads

  • · Replies 39 ·
2
Replies
39
Views
2K
  • · Replies 99 ·
4
Replies
99
Views
12K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 58 ·
2
Replies
58
Views
4K
  • · Replies 3 ·
Replies
3
Views
914
  • · Replies 40 ·
2
Replies
40
Views
8K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 9 ·
Replies
9
Views
1K
  • · Replies 28 ·
Replies
28
Views
2K
  • · Replies 21 ·
Replies
21
Views
3K