Could a Collapsing Universe Result in a Cosmological Blueshift?

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The discussion centers on the possibility of a cosmological blueshift if the universe had stopped expanding and started collapsing 10 million years ago. Participants debate the appropriate scale factor-redshift formula, suggesting that the collapsing universe would indeed result in blueshifted spectra. They argue that if the universe contracted over a significant period, some galaxies could exhibit a negative redshift (z), indicating shorter wavelengths. The consensus is that the ratio of wavelengths remains positive, with z being greater than -1. The conversation concludes with a light-hearted question about Einstein's popularity among teenagers.
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If the Universe stopped expansion 10 million years ago and started to collapse
Whould it their be such a thing as cosmological blueshift?


Would the scalefactor-redshift be R=1/(z - 1) or R=1/(1+z)?

I think since universe is collapsing then spectra will be blueshifted!

The scale factor is still relevant but the formula is changed to 1/1(z-1)!
 
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2203312 said:
If the Universe stopped expansion 10 million years ago and started to collapse
Whould it their be such a thing as cosmological blueshift?Would the scalefactor-redshift be R=1/(z - 1) or R=1/(1+z)?

I think since universe is collapsing then spectra will be blueshifted!

The scale factor is still relevant but the formula is changed to 1/1(z-1)!

If the universe had stopped expanding only fairly recently, like say a billion years ago, and had started to contract, then some galaxies would have a NEGATIVE z.

It would continue to be true that 1+z equals the ratio by which distances have changed while the light is in transit.

Some light would have z = 0 for example if the light was emitted 2 billion years ago and for the first billion year that it was in transit there was expansion and then for the next billion years there was contraction---then there would be no net change in the wavelength.
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You don't need any new formula. You can always assume that 1+z is the ratio of distances, and also the ratio of wavelengths.
If the universe had been contracting for several billion years, so there was enough time for some distances to contract by a factor of 10, then there would be some galaxies with z = -0.9
That means the ratio of wavelengths is 1+z = 0.1
The wavelengths are ten times shorter----in other words bluer, more UV

The way that z is defined it cannot take on the value -1 or any value more negative than -1. The ratio of wavelengths is always a positive number 1+z>0 and that means that z>-1.
 
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Many thanks,
Now the big question

How did Einstein get so popular with teenage kids and that hair style?
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
Why was the Hubble constant assumed to be decreasing and slowing down (decelerating) the expansion rate of the Universe, while at the same time Dark Energy is presumably accelerating the expansion? And to thicken the plot. recent news from NASA indicates that the Hubble constant is now increasing. Can you clarify this enigma? Also., if the Hubble constant eventually decreases, why is there a lower limit to its value?
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