An alternative quantification of redshift

1. Inverting Redshift

Redshift (z) can be quantified by comparing the observed energy (Eobs) of a photon to its original energy (Eemit):

(1)
\begin{equation} 1+z = \frac{E_{emit}}{E_{obs}} \label{eq:z} \end{equation}

If the photon is observed to have less energy than when it was emitted (Eobs < Eemit), then z > 0 and the photon is redshifted. When the photon gains energy (Eobs > Eemit), then z < 0 and the photon is blueshifted. Since the photon will always have a positive energy, Eemit / Eobs is always greater than zero, so z is always greater than -1. Thus, the range of redshifts is infinite (z > 0), and the range of blueshifts is finite (-1 < z < 0).

As an alternative, consider what happens when equation (1) is inverted and set equal to 1 + b:

(2)
\begin{equation} 1+b = \frac{1}{1+z} = \frac{E_{obs}}{E_{emit}} \label{eq:inverted} \end{equation}

When b > 0, that means the photon has gained energy, which is blueshift. When b < 0, the photon has less energy than when it was emitted, so the photon is redshifted. Since the photon's energy will never be negative or zero, b is always greater than -1. Quantified this way, the range of redshifts is finite (-1 < b < 0).

The range of redshifts can be either infinite (as z) or finite (as -b):


z > 0
   
-1 < b < 0

2. Distance

The traditional redshift-distance relationship is:
(3)
\begin{equation} d = z \frac{c}{H_{0}} \end{equation}

Where d is distance, c is the speed of light, and H0 is Hubble's constant. This equation is an approximation that is only valid for very small redshifts (z ≪ 1).

Substituting z with the alternative quantification, -b:

(4)
\begin{equation} d = -b \frac{c}{H_{0}} \label{eq:db} \end{equation}

Solving equation (2) for b and simplifying:

(5)
\begin{equation} b = - \frac{z}{1+z} \label{eq:bz} \end{equation}

Substituting (5) into (4) gives the alternative redshift-distance relationship:

(6)
\begin{equation} d = \frac{z}{1+z} \frac{c}{H_{0}} \label{eq:altd} \end{equation}

Comparing the two distance relationships (Fig. 1) shows that the distance predicted by the traditional equation climbs to infinity while the alternative equation converges on c / H0. This is due to the range of redshifts being infinite as z and finite as -b (i.e. z / (1 + z)).


Figure 1. The traditional and alternative redshift-distance relationships.

3. Lookback Time

Dividing both sides of equation (6) by the speed of light, c, gives the alternative redshift-time equation:

(7)
\begin{equation} t = \frac{z}{1+z} \frac{1}{H_{0}} \end{equation}

This equation is also the solution to the lookback time integral for what's known as an "empty" Friedmann-Lemaître-Robertson-Walker (FLRW) model.[1]

In Fig. 2, the alternative redshift-time equation is compared to the lookback times of three FLRW models: an empty model (ΩM=0, Ωλ=0), a matter-only model (ΩM=1, Ωλ=0), and the concordance model, (ΩM=0.32, Ωλ=0.68).


Figure 2. The redshift-time relationships compared to FLRW lookback times.

The empty model and the concordance model have similar predictions while the matter-only model predicts a far younger universe. The lookback times predicted by the empty FLRW model are identical to the times given by the alternative redshift-time equation.

4. Conclusion

When quantified as z the range of redshifts is infinite. When quantified as -b, however, the range is finite. The traditional and alternative quantifications of redshift lead to two distance relationships. The traditional relationship is linear, and only a valid approximation for very small values of z. The alternative relationship is identical to an empty FLRW model, and a reasonable approximation to the concordance model.

While the choice between quantifications of redshifts initially seems arbitrary and inconsequential, upon further investigation, the inverted, alternative quantification is a more accurate representation of the universe.

References

[1] K. Krisciunas, "Look Back Time, the Age of the Universe, and the Case for a Positive Cosmological Constant", J.Roy.Astron.Soc.Canada, 669 (1993) arXiv:astro-ph/9306002

email: mike@mikehelland.com

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