GR: Signature & Dimension of Embedding Space

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SUMMARY

The discussion focuses on the relationship between differential geometry, curvature tensors, and embedding spaces in General Relativity (GR). It establishes that the geometry of a lower-dimensional curved space, such as a 2D surface, does not depend on the dimensionality of the higher-dimensional embedding space. The conversation also touches on the signature of the surrounding Euclidean plane in the Einstein Field Equations (EFE) and the use of higher-dimensional spaces in cosmology. Recommendations for beginner-friendly resources include Wheeler's "Gravitation" and Spivak's "Comprehensive Introduction to Differential Geometry."

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with differential geometry concepts
  • Knowledge of curvature tensors, specifically Riemann and Ricci tensors
  • Basic grasp of Einstein Field Equations (EFE)
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  • Study the implications of the Whitney embedding theorem in differential geometry
  • Explore the concepts of curvature in Riemannian geometry
  • Learn about the signature of metrics in General Relativity
  • Investigate the role of higher-dimensional spaces in cosmological models
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Students and researchers in physics, mathematicians interested in differential geometry, and anyone seeking to deepen their understanding of General Relativity and its mathematical foundations.

dismachaerus
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Hello. I am not familiar with differential geometry and curvature tensors, yet I am having a great deal of questions to ask.
First when we lay a set of coordinates for an n-dimensional plane, let's say 2 coordinates for a surface embedded in a 4D space the vectors we begin with to describe our surface must have 4 coordinates each, right? So, no matter how we arrive at our curvature Riemann or Ricci tensor the space in which our surface is embedded must reflect in our equations somehow... I mean with an increase in the dimensionality of the embeddind space we must get a different set of equations for each 2D surface say. Or is it that the tensor equations are independent of dimensions of surrounding vector space? How is this possible?
With this in mind, what is the signature of the surrounding Euclidean plane in the EFE near a massive body? Is it (-,+,+,+,+) or (-,+,+,+,-) ? Did Einstein use 5D vectors in his equations to arrive at?
In cosmology do we often use higher than 5D embedding spaces to describe the expanding spacetimes, especially for the flat space expanding universes?
And finally, which book is good for me to start learning GR? Is Wheeler's book Gravitation right for a beginner like me or do i need more basics like Spivak's Comprehensive Introduction To Diff. Geometry?
 
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Hi dismachaerus, welcome to PF!

Actually, one of the interesting things about Riemannian geometry is that the embedding space is completely irrelevant. All of the notions of curvature and geometry are formulated purely in terms of the lower dimensional curved space and there is no need to reference any higher dimensional flat embedding space.

For example, the surface of a sphere is a 2D curved manifold which you are probably picturing in your head as being embedded in a flat 3D space. But you can do all of your differential geometry on the surface of the sphere using only the 2D curved coordinates.
 
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