Is expansion of space relative?

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SUMMARY

The discussion centers on the concept of the relative expansion and contraction of space, particularly in relation to General Relativity (GR). Participants explore whether regions of space with varying matter density experience different rates of expansion or contraction. The notion that areas with high matter density might resist expansion due to spacetime curvature is highlighted, raising questions about the implications for cosmic background radiation and redshift. The conversation emphasizes the complexity of spacetime as a dynamic entity influenced by matter rather than a static backdrop.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with cosmic background radiation
  • Knowledge of redshift phenomena
  • Concept of spacetime curvature
NEXT STEPS
  • Research the implications of General Relativity on cosmic expansion
  • Study the relationship between matter density and spacetime curvature
  • Examine the effects of cosmic background radiation on observational cosmology
  • Explore the concept of redshift in the context of expanding universe models
USEFUL FOR

Astronomers, physicists, cosmologists, and anyone interested in the dynamics of spacetime and the universe's expansion.

kmarinas86
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Could it be that some spaces are expanding more than others?

What about the reverse? Could it be that some parts of space are contracting more than others? Is it relative?

Could GR support the notion that space where matter exists is shrinking faster than space far away from matter?

Would this still conserve the cosmic background radiation? Would it still lead to its redshift?
 
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kmarinas86 said:
Could it be that some spaces are expanding more than others?

What about the reverse? Could it be that some parts of space are contracting more than others? Is it relative?

Could GR support the notion that space where matter exists is shrinking faster than space far away from matter?

Would this still conserve the cosmic background radiation? Would it still lead to its redshift?

On the scale that needs to be considered the universe, to use a non-technical term, is so samey that you'd expect any variation will be negligible.
 
kmarinas86 said:
Could it be that some spaces are expanding more than others?

What about the reverse? Could it be that some parts of space are contracting more than others? Is it relative?

Could GR support the notion that space where matter exists is shrinking faster than space far away from matter?

Would this still conserve the cosmic background radiation? Would it still lead to its redshift?

I carn't see why not - area's of space with a high density of matter would be highly curved and so 'resist' spacetime expansion. Space is defined by the distance between objects, its not an independent entity, so the relative space between two exploding stars is expanding, whereas the space around a collapsing neutron star is collapsing. I'm not sure if this applies for the Universe as a whole, since its expansion derives from the energy of the big-bang.
There does seem to be a contradiction though, because spacetime is not a permanent background, it is defined by the properties of matter - at the same time the Universe is expanding. What is doing the expanding?
 

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