Does time expand along with space?

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SUMMARY

The discussion centers on the relationship between the expansion of space and the perception of time in cosmology, specifically using the flat Friedmann-Robertson-Walker (FRW) metric. The proper distance between co-moving points scales with the scale factor \(a(t)\), indicating that space expands. However, while light emitted from a source experiences redshift due to this expansion, it does not imply that cosmological time intervals expand in the same manner. Instead, the time intervals remain constant for a comoving observer, with the observed effects attributed to the redshift of light rather than time expansion.

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  • Understanding of the flat Friedmann-Robertson-Walker (FRW) metric
  • Familiarity with concepts of proper distance and scale factor \(a(t)\)
  • Knowledge of cosmological redshift and its implications
  • Basic grasp of time dilation effects in cosmology
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jcap
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Sorry to go on about this topic. I'll get it out of my system soon!

The flat FRW metric is given by:
$$ds^2=-c^2dt^2+a(t)^2dr^2$$
If we take ##dt=0## then we get:
$$ds=a(t)\ dr$$
The proper distance between co-moving points scales with ##a(t)##. Thus we find that space expands.

If we take ##ds=0## to find the null geodesic followed by a light beam we get:
$$c\ dt=a(t)\ dr$$
Surely this implies that cosmological time intervals expand in the same way as space intervals?
 
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This implies ## dt=\frac{c}{a(t)}dr ##, which is a useful relation but says nothing of "time expansion".
If ##\tau## is the proper time of a comoving observer, and ##\delta## the distance in his reference frame to another comoving object situated at comoving distance ##r##,
##\quad\tau=t## (no time expansion)
##\quad\delta=a(t)r## ("space expansion")

But you may be referring to the time dilation effect when this observer looks at a comoving source. Light emitted by that source at ##t## and ##t+dt## is received at ##t'## and ##t'+\frac{dt}{a(t)}## because the second pulse was emitted from a more distant source than the first - this is actually the same thing as the redshift ot a distant source due to expansion.
 
Last edited:
jcap said:
Surely this implies that cosmological time intervals expand in the same way as space intervals?

No, it implies that the wavelength of light expands with ##a(t)##--i.e., that the light gets redshifted as the universe expands, as wabbit said.
 

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