Space where General Reletivity Resides

In summary, there are various geometries that can be used to describe space and its interaction with matter. These include Einstein-Cartan Space, Riemann Space, and Minkowski Space. However, the most realistic description is still under debate. The Schwarzschild metric and the Tolman-Oppenheimer-Volkoff equation can be used to model stars in astrophysics and General Relativity. The Riemann–Cartan geometry, which includes affine torsion, is an extension of Riemannian geometry and is now known as the Einstein–Cartan theory. However, the rigorous mathematical proof of convergence to this theory has not yet been done. Further research and examination into the Einstein–Cartan theory could provide
  • #1
Philosophaie
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There are many spaces: Einstein-Cartan Space, Riemann Space, Minkowski Space... Which one does the Earth and the Sun reside in? Which one has Torsion, mass etc. if any?
 
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  • #2
Those are basically just geometrical representations. It could be said that we reside in none of them or all of them, depending on how one reads the question.
 
  • #3


A model can be formulated in say Riemann space to take in account for the magnetic and gravitational field of the sun. The torsion would be zero. The metric would be the Schwarzschild metric. Affinity would be the Christoffel symbol. Then the Riemann Curvature and Ricci Tensors can be calculated. Would this be the correct model for the sun?
 
  • #4
Philosophaie said:
There are many spaces: Einstein-Cartan Space, Riemann Space, Minkowski Space... Which one does the Earth and the Sun reside in? Which one has Torsion, mass etc. if any?

Russ has basically given the complete answer. I'll toss in my two bits.

You are listing alternative geometries, that go onto space and describe how it acts. Alternative geometries, not different spaces as such.

Maybe a trivial distinction but you probably know the quotes from Einstein where he says points in space have no physical existence, no objective reality.
So the thing to focus on is the geometry. Often it is a dynamic geometry able to interact with matter, behavior governed by a Lagrangian or a differential equation.

So what your question means to me is which is the best most realistic description of geometry and how it behaves interactively with matter?

I can't tell you any final answer but obviously Minkowski geometry is highly unrealistic. It is only right if there is no matter, and not always even then. It is only approximately right if there is negligible matter in the universe. It does not expand. It is flat. It sucks.

On the other hand (strictly interpreted) Riemannian geometry has the wrong metric signature---which Minkowski at least gets right! So Riemannian is no good.

As Russ hints, all these geometries are human constructs. So the question is which is the most realistic, not which do we live in.

Of the ones you listed I'd go with Einstein Cartan.

But I also like the new version of quantum geometry that came out in 2007. It looks like it might give classical GR in the large distance limit, and also be kind of interesting and weird in the very small distance limit.
 
  • #5
A model can be formulated in Einstein-Cartan Space would have to take into account spin and torsion of which I am unfamiliar in formulating. Any suggestions on how to learn about these modeling techniques of the sun?
 
  • #6
General Relativity...


Philosophaie said:
Any suggestions on how to learn about these modeling techniques of the sun?
Use the Schwarzschild metric and the Tolman-Oppenheimer-Volkoff equation to model stars in astrophysics and General Relativity.

In Einstein's theory of general relativity, the Schwarzschild solution (or the Schwarzschild vacuum) describes the gravitational field outside a spherical, non-rotating mass such as a (non-rotating) star, planet, or black hole. It is also a good approximation to the gravitational field of a slowly rotating body like the Earth or Sun. The cosmological constant is assumed to equal zero.

In astrophysics, the Tolman-Oppenheimer-Volkoff (TOV) equation constrains the structure of a spherically symmetric body of isotropic material which is in static gravitational equilibrium, as modeled by General Relativity.

The extension of Riemannian geometry to include affine torsion is now known as Riemann–Cartan geometry.

Wikipedia said:
While it is intuitively compelling that this implies Einstein–Cartan theory, the rigorous mathematical proof of convergence to the equations of Einstein–Cartan theory has not been done.

The equivalent TOV solution for the Einstein–Cartan theory, would be an interesting examination.

Reference:
http://en.wikipedia.org/wiki/Riemannian_geometry"
http://en.wikipedia.org/wiki/Schwarzschild_metric"
http://en.wikipedia.org/wiki/Tolman-Oppenheimer-Volkoff_equation"
http://en.wikipedia.org/wiki/Einstein%E2%80%93Cartan_theory"
 
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Related to Space where General Reletivity Resides

1. What is "Space where General Relativity Resides"?

"Space where General Relativity Resides" refers to the physical space in which the theory of general relativity can be applied and observed. It is the space in which the laws of gravity, as described by Einstein's theory, govern the behavior of matter and energy.

2. How is "Space where General Relativity Resides" different from regular space?

"Space where General Relativity Resides" is different from regular space in that it takes into account the curvature of spacetime caused by the presence of mass and energy. This is described by Einstein's theory of general relativity, which replaces Newton's theory of gravity. In this space, the laws of gravity are more complex and allow for phenomena such as black holes and gravitational waves.

3. What are the key concepts of "Space where General Relativity Resides"?

The key concepts of "Space where General Relativity Resides" include the curvature of spacetime, which is caused by the presence of mass and energy, and the idea that gravity is not a force but rather a result of the curvature of spacetime. It also includes the concept of geodesics, which are the paths that objects naturally follow in curved spacetime.

4. How is "Space where General Relativity Resides" related to the Big Bang theory?

"Space where General Relativity Resides" is closely related to the Big Bang theory, as it provides the framework for understanding the expansion of the universe and the formation of galaxies and other structures. It also explains the cosmic microwave background radiation, which is a key piece of evidence for the Big Bang theory.

5. What are some practical applications of "Space where General Relativity Resides"?

The practical applications of "Space where General Relativity Resides" include GPS technology, which relies on the accuracy of general relativity to account for the curvature of spacetime and the time dilation effects of satellites. It also has applications in astrophysics, allowing us to study and understand the behavior of celestial objects such as black holes and neutron stars. Additionally, it has implications for our understanding of the origin and evolution of the universe.

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