The physical meaning of expansion in cosmology

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SUMMARY

The discussion focuses on the physical interpretation of expansion in cosmology, emphasizing that space should not be objectified as a material substance. Instead, it is suggested that one should think of distances between stationary observers, particularly in relation to the Cosmic Microwave Background (CMB). The conversation highlights Hubble's Law, which states that distances between these observers are increasing at a rate of approximately 1/140 of a percent every million years, decreasing asymptotically to 1/160 percent in the far future. The importance of General Relativity (GR) is acknowledged, noting its predictive power regarding geometric behavior and the necessity of avoiding misconceptions about space and spacetime.

PREREQUISITES
  • Understanding of Hubble's Law and its implications in cosmology.
  • Familiarity with General Relativity (GR) and its geometric interpretations.
  • Knowledge of the Cosmic Microwave Background (CMB) and its significance in cosmological measurements.
  • Concept of stationary observers in the context of cosmological distances.
NEXT STEPS
  • Research the implications of Hubble's Law on the expanding universe model.
  • Explore the mathematical framework of General Relativity and its predictions about curvature.
  • Investigate methods for measuring cosmological distances, including the distance ladder technique.
  • Study the differences between space and spacetime in cosmological contexts.
USEFUL FOR

Astronomers, cosmologists, physics students, and anyone interested in understanding the nuances of cosmic expansion and the implications of General Relativity in modern cosmology.

  • #31
Garth said:
The "space that expands" is that described by the FRW metric - yes it does require a smattering of GR and also the interpretation of the observation of Hubble red shift, marcus has clearly defined it and distinguished it from 'ordinary space'.

Garth

Perhaps one simplistic model, might be to think of a manifold (i.e. continuum) being stretched uniformly for a given stage of universe (i.e. for given value of Hubble parameter). Then concomitantly (i.e. for given value of Hubble parameter), one also has local depressions forming (i.e. indentations i.e. curvature), representing local gravitational aggregation.
 
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  • #32
Garth said:
Such as "cosmological space"??

Garth
Yes. This is well defined. Just 'space' --- so often used --- is much too vague for informed discussions.
 
  • #33
marcus said:
This post is admittedly vague---it is merely meant to convey my attitude about GR. Briefly, my attitude is don't live in a straight-jacket of Greek expectations about geometry.
I feel I should point out that even the Greeks were capable of imagining non-Euclidean phenomena; e.g. that a pair of lines, in defiance of the Parallel postulate, could be in a situation where the interior angles add up to less than 180°, but the lines merely tended towards each other indefinitely without crossing. And, of course, they had all those lively debates about our notions of space. :smile:
 

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