Have I got the right picture for cosmological redshift?

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SUMMARY

The discussion centers on cosmological redshift as explained by Sean Carroll, contrasting it with Doppler redshift. In a flat universe, two galaxies can be separated by distance ## s##, and if one galaxy is propelled away, no Doppler redshift occurs when the photon reaches the stationary galaxy. Conversely, in an expanding universe, the same photon experiences redshift due to the expansion of space itself, even though the galaxies remain at distance ## s##. This distinction highlights that distant galaxies are not necessarily moving away in the traditional sense, prompting further exploration of the implications of the Hubble constant.

PREREQUISITES
  • Understanding of cosmological redshift and its formula
  • Familiarity with the concept of Doppler redshift
  • Basic knowledge of metric expansion in cosmology
  • Awareness of the Hubble constant and its significance in cosmology
NEXT STEPS
  • Study the mathematical derivation of the cosmological redshift formula
  • Examine the implications of the Hubble constant on cosmic expansion
  • Learn about the differences between cosmological and Doppler redshift in detail
  • Explore Sean Carroll's theories on the expanding universe and related thought experiments
USEFUL FOR

Astronomers, cosmologists, physics students, and anyone interested in the fundamental concepts of cosmic expansion and redshift phenomena.

George Keeling
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TL;DR
I have a question on cosmological redshift which I have just learned about from Sean Carroll. After calculating it for an expanding universe he does a thought experiment to show that it is different to Doppler redshift which would be detected if two galaxies were flying away from each other in a flat (therefore not expanding) universe.
Summary: I have a question on cosmological redshift which I have just learned about from Sean Carroll. After calculating it for an expanding universe he does a thought experiment to show that it is different to Doppler redshift which would be detected if two galaxies were flying away from each other in a flat (therefore not expanding) universe.

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Here's Sean Carroll's thought experiment:
We have flat universe L on the left with two galaxies separated by distance ## s##. A photon is emitted from galaxy 1, galaxy 2 is quickly propelled to a separation of ##2s##, galaxy 2 stops and the photon arrives. Since the galaxies are now not relatively moving there would be no Doppler redshift.

On the right the galaxies are also separated by ## s## but, instead of moving a galaxy, the universe expands by a factor of 2 (it briefly gets a metric like ## ds^2=-dt^2+t^2dx^2##), then stops expanding and then the photon arrives. According to the cosmological redshift formula, the photon has a redshift.

This implies that the galaxies in universe R are still separated by ## s##, because rulers would expand along with everything else. One can also check this by drawing out and back light paths before and after expansion.

This is spooky. It also implies that in our 'expanding' universe distant galaxies are not really moving away! One also wonders how we tell that it's cosmological not Doppler redshift.

Have I got the picture roughly right? The next step will be to compare these to real values like the Hubble constant.
 
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