Can space-time homogeneity put limits

In summary, the conversation discusses the gauge-invariance of classical electrodynamics and whether all of spacetime can be considered homogeneous. The concept of homogeneity is only applicable on a large scale and conflicts with gauge invariance. The article mentioned is available at www.arxiv.org and further explanation can be found in the cosmological principle.
  • #1
dextercioby
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...on the gauge-invariance of classical electrodynamics ?

I'm thinking of flat Minkowski space-time of SR in which a charged particle moves and generates an electromagnetic field described by the well-known Lie/nard - Wiechert potential.

In this situation can we say all spacetime is homogenous ? If so, then can we infer that the gauge freedom of the L-W potential is disturbed, meaning that the gauge-parameter is necessarily 0 ?

If you think the questions and the whole subject of this post are idiotic, then the same label can be ascribed to the article phys:0609152 available at www.arxiv.org.

Daniel.

P.S. I share your feeling: WTF ?
 
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  • #2
AFAIK, space-time is only homogeneous in the large. I.e. we have large lumps of matter (planets, galaxies, stars). We say that space-time is homogenoeous only when averaging over a large volume. In the later case we make this sort of averaged homogeniety "the cosmological principle" http://en.wikipedia.org/wiki/Cosmological_principle

The same sort of principle applies to charge. The flux tubes around Jupiter illustrate that there can be important electromagnetic inhomogoneities locally. It's only on the "grand scale" that we expect homogeneity.

Basically, if there is a conflict, gauge invariance trumps homogeneity.
 
  • #3
So you're saying the article is not a bunch of crap. Ok. then.

Daniel.
 

FAQ: Can space-time homogeneity put limits

Can space-time homogeneity put limits on the expansion of the universe?

Yes, space-time homogeneity is one of the fundamental assumptions of the standard model of cosmology. It states that the universe is isotropic and homogeneous on large scales, meaning that the properties of the universe are the same in all directions and at all points in space. This assumption helps us understand the expansion of the universe and can also put limits on the rate of expansion.

How does space-time homogeneity affect the distribution of matter in the universe?

Space-time homogeneity plays a crucial role in the formation and distribution of matter in the universe. It allows us to predict how matter is distributed on large scales and how galaxies and clusters of galaxies are distributed throughout the universe. Without this assumption, our understanding of the structure of the universe would be limited.

Can space-time homogeneity explain the cosmic microwave background radiation?

Yes, the theory of space-time homogeneity helps explain the cosmic microwave background radiation, which is the residual radiation left over from the Big Bang. This radiation is nearly uniform in all directions, which is consistent with the assumption of space-time homogeneity.

Are there any observations that contradict the assumption of space-time homogeneity?

There have been some observations that suggest that space-time homogeneity may not hold at extremely large scales. For example, the "Cold Spot" in the cosmic microwave background radiation may indicate a lack of homogeneity on scales larger than 1.8 billion light-years. However, further research and observations are needed to confirm these findings.

How does space-time homogeneity impact our understanding of the early universe?

Space-time homogeneity plays a crucial role in our understanding of the early universe. It allows us to make predictions about the universe's evolution and the formation of structures such as galaxies and clusters of galaxies. It also helps us understand the origin of the cosmic microwave background radiation and the overall structure of the universe.

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