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Geometry of Look-Back



 
 
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Old December 11th 12, 05:41 PM posted to sci.astro.research
Eric Flesch
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Posts: 321
Default Geometry of Look-Back

Not much work seems to be done nowadays on open (aka hyperbolic) or
closed (aka spherical) manifolds, but it's instructive to consider
what they would look like as a nightsky. The answer is they would
look just the same as flat space, but if one were to hop in a rocket
and travel out there, one would find that objects are closer than
their angular size indicates in an open manifold (i.e.,
"foreshortened"), and in a closed manifold they would be further away
than expected.

So nowadays we model that we can't visually distinguish at all between
these alternative curvatures. But spectroscopy illustrates how nature
finds ways to convey information -- astronomers of 100 years ago would
be astonished at how much signal there is in mere light. My
supposition is that there is indeed a visual way to distinguish
between open, flat, and closed manifolds, and that the cosmological
redshift shows us the way.

Regardless of all the complex constructs of standard cosmology, the
simple anchor is that cosmological redshift results from recession.
No recession, no big bang. So alternative viewpoints of the redshift
are not welcome to some -- which is no reason not to try, of course.

Lopez-Corredoira gave a useful review of static models in his paper
"Angular Size Test on the Expansion of the Universe" (2010
IJMP,19,245; arxiv:1002.0525) and observed (as have others) that 1/z
is well-fit to angular size across all redshifts -- without need of
evolution, dark matter, dark energy, whatever. Occam is calling.

So these are threads for me to follow, hopefully to assemble into a
coherent whole, after the holidays. cheers, Eric.
 




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