Spacetime Curvature via Triangle

In summary, the conversation discusses the concept of defining curvature on a 2D manifold using a triangle and how this applies in 3D. It is explained that in 3D, there are multiple independent components for the curvature tensor and the specific one chosen depends on the orientation of the triangle. A visual illustration of this concept is provided using an animated example from Wikipedia.
  • #1
Narasoma
42
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I understand the mechanism of defining the curvature of a 2D manifold via triangle. But I don't understand how this works in 3D. Meanwhile, Lawrence Krauss mentioned in his book A Universe from Nothing it does.

How does this work in 3D?
 
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  • #2
The same way it works in 2D except in 3D there are more than one independemt component for the curvature tensor and which one you single out depends on the planar orientation of the triangle.
 
  • #3
If you are looking for a visual analog to the triangle, here's one from Wikipedia.
It is animated, so watch it for a while until you see all the vectors.
https://en.wikipedia.org/wiki/Riemann_curvature_tensor

Riemann_curvature_motivation_shpere.gif


An illustration of the motivation of Riemann curvature on a sphere-like manifold. The fact that this transport may define two different vectors at the start point gives rise to Riemann curvature tensor. The right angle symbol denotes that the inner product (given by the metric tensor) between transported vectors (or tangent vectors of the curves) is 0.
 
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FAQ: Spacetime Curvature via Triangle

What is spacetime curvature?

Spacetime curvature is a concept in physics that describes the bending of space and time caused by the presence of massive objects. It is a fundamental principle of Einstein's theory of general relativity.

How is spacetime curvature measured?

Spacetime curvature is measured using the mathematical concept of Riemann curvature tensor, which describes the curvature of spacetime at a given point. This can be calculated using the geometry of triangles formed by the paths of light rays in the presence of massive objects.

What is the role of triangles in understanding spacetime curvature?

Triangles play a crucial role in understanding spacetime curvature because they allow us to visualize the bending of space and time caused by massive objects. By measuring the angles and sides of triangles formed by light rays, we can calculate the curvature of spacetime.

Can spacetime curvature be observed?

Yes, spacetime curvature can be observed through the phenomenon of gravitational lensing. This occurs when light from distant objects is bent by the curvature of spacetime caused by massive objects, such as galaxies or black holes.

How does spacetime curvature affect our daily lives?

While spacetime curvature may seem like a concept that only applies to the vastness of the universe, it actually has tangible effects on our daily lives. For example, GPS systems must take into account the curvature of spacetime in order to accurately calculate position and time. Without this understanding of spacetime curvature, our GPS systems would not work correctly.

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