General Relativity: Spatial Inversion Symmetry

In summary, the conversation discusses the limitations of describing transformations of the type x \rightarrow -x in spacetime, particularly in the case of static spacetime. The speaker poses a question about the vanishing of cross terms in coordinates with a Killing vector and the proof for this symmetry. They also mention the possibility of rotational symmetries having no cross terms and the implications for symmetries without corresponding translation symmetries. The expert summarizes that while this symmetry can exist locally in general relativity, there are challenges in defining it globally for an arbitrary spacetime.
  • #1
Slereah
7
0
I am unable to find any source describing at any lengths transformations of the type

[itex]x \rightarrow -x[/itex]

beyond the case of static spacetime (and even in the case of static spacetime, it is rarely the fundamental definition, which tends to be more along the lign of orthogonality with an hyperplane, [itex]\xi_{[a} \nabla_b \xi_{c]}[/itex]).

So my question is, if I have a space reversal symmetry, do the cross terms of that coordinates always vanish (if that coordinate also has a Killing vector at least), and is the most obvious proof ([itex]x \rightarrow -x, \ g_{xy} dx dy = -g_{xy} dx dy \rightarrow g_{xy} = 0[/itex] the correct one. Also, does it mean that all rotational symmetries have no cross terms, since they have [itex]\mathbb{Z}_2[/itex] as a subgroup?

If there is such a symmetry without a corresponding translation symmetry, does it just imply that the cross terms are odd functions?
 
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  • #2
You certainly have this symmetry locally in GR. Globally, there is not even any way to define the operation for an arbitrary spacetime. For example, there is not guaranteed to be a coordinate chart that covers all of spacetime, nor do you have any guarantee that the spacetime is orientable.
 
  • #3
Sure, but let's say we have a spacetime that can admit such a symmetry. Let's say [itex]\mathbb{R} \times \mathbb{R}^3[/itex], with a distribution of matter symmetrical by reflection along some plane.
 

Related to General Relativity: Spatial Inversion Symmetry

1. What is spatial inversion symmetry in general relativity?

Spatial inversion symmetry in general relativity refers to the property of the theory that states that the laws of physics remain unchanged when the spatial coordinates are inverted or reversed. This means that if we were to flip the space around us, the laws of physics would still hold true.

2. How does spatial inversion symmetry affect our understanding of gravity?

Spatial inversion symmetry plays a crucial role in our understanding of gravity as it allows us to make predictions about the behavior of objects and the curvature of space-time. This symmetry, along with other symmetries in general relativity, helps us to formulate the theory and make accurate predictions about the effects of gravity.

3. Is spatial inversion symmetry always present in general relativity?

Yes, spatial inversion symmetry is always present in general relativity. This is because the theory is based on the principle of equivalence, which states that the laws of physics are the same for all observers in any inertial reference frame. As a result, spatial inversion symmetry is a fundamental aspect of the theory.

4. Can spatial inversion symmetry be broken in certain situations?

Yes, spatial inversion symmetry can be broken in certain situations, such as when dealing with strong gravitational fields or in the presence of matter with high energy densities. In these cases, the effects of gravity can cause deviations from the expected symmetrical behavior.

5. How does spatial inversion symmetry relate to other symmetries in general relativity?

Spatial inversion symmetry is one of the many symmetries present in general relativity, including time translation symmetry, rotational symmetry, and Lorentz symmetry. These symmetries work together to form the foundation of the theory and allow us to make accurate predictions about the behavior of matter and energy in the universe.

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