Is My Proper Time the Same as Cosmological or Conformal Time?

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SUMMARY

The discussion centers on the relationship between proper time, cosmological time, and conformal time for an observer traveling with the Hubble flow. It establishes that if an observer is at rest relative to the Cosmic Microwave Background (CMB), their proper time aligns closely with cosmological time, while deviations occur for other velocities. The discussion employs the Friedmann-Robertson-Walker (FRW) metric to illustrate the differences between cosmological time and conformal time, concluding that for a free-falling co-moving observer, proper time equates to conformal time.

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  • Understanding of the Friedmann-Robertson-Walker (FRW) metric
  • Knowledge of proper time and conformal time concepts
  • Familiarity with the Cosmic Microwave Background (CMB)
  • Basic principles of general relativity and spacetime diagrams
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  • Study the implications of the Friedmann-Robertson-Walker (FRW) metric in cosmology
  • Explore the relationship between proper time and cosmological time in different frames
  • Investigate the effects of velocity relative to the CMB on time measurements
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Astronomers, physicists, and students of cosmology who are interested in the nuances of time measurement in the context of general relativity and the expanding universe.

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As an observer who is simply traveling with the Hubble flow is my proper time the same as the cosmological time or is it equal to the conformal time?
 
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If you are at rest relative to the CMB, otherwise you will get a different value. For typical velocities relative to the CMB (just the motion of galaxies, not relativistic spacecraft s), the difference is very small compared with the current timing uncertainties.
 
mfb said:
If you are at rest relative to the CMB, otherwise you will get a different value. For typical velocities relative to the CMB (just the motion of galaxies, not relativistic spacecraft s), the difference is very small compared with the current timing uncertainties.

I think I am a free-falling co-moving observer rather than simply a co-moving observer.

My local spacetime should therefore be flat - in other words my local frame is inertial.

Starting with the FRW metric with cosmological time t and co-moving spatial co-ordinates:

\large ds^2 = -dt^2 + a(t)^2 [ \frac{dr^2}{1-kr^2} + r^2(d\theta^2+\sin^2\theta d\phi^2)]

I rewrite the FRW metric with conformal time \tau and co-moving spatial co-ordinates:

\large ds^2 = a(t)^2(-d\tau^2 + \frac{dr^2}{1-kr^2} + r^2(d\theta^2+\sin^2\theta d\phi^2))

where an element of conformal time d\tau is given by

\large d\tau = \frac{dt}{a(t)}

The worldline of a radial lightbeam according to the re-written metric is given by

\large d\tau = \frac{dr}{\sqrt{1-kr^2}}

For small r this metric describes a locally flat spacetime in which light travels on diagonals on a spacetime diagram. This is consistent with the co-ordinate system of a free-falling observer with a local inertial frame.

Therefore I think my proper time is conformal time.
 
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