2.2. The Intergalactic Extinction Model
Interstellar and host (or internal, extragalactic) extinctions have been studied extensively close to earth on MW, LMC and SMC, and on host galaxies respectively. It has been essential to apply corrections to distance moduli to account for such extinctions when estimating distances or the intrinsic brightness of the source. Brout and Riess [
5] give a comprehensive review on these extinctions. However, similar types of extinctions due to intergalactic media in between the host galaxy and MW/LMC/SMC along the vast distances of light travel has not been accounted for, which should increase with distance and thus become increasingly critical as our modern telescopes look into deeper space on the Gpc scale, resulting in overestimation of distances.
Intergalactic extinctions (IEs) may occur after the emitted light of a star leaves its host galaxy and before it enters the LMC/SMC/MW range. IE increases with distance, and may come from three sources:
To gauge on the significance of intergalactic extinction source 1 above, Let’s do a rough estimation by answering the question: how likely would one expect to have a galaxy or galaxies in the line-of-sight between the light source and an earth observer? It’s a battle of two sheer numbers: the very large number of galaxies in the very large volume of the universe. Detailed in the
Appendix A, the answer is: 6% probability per Gpc if the source is a galaxy, and 25% probability per Gpc if the source is a star (Cepheid, Supernova etc). These conservatively estimated probabilities are significant and must not be ignored.
Unlike interstellar and host extinctions, intergalactic extinction cannot be estimated with extinction curves since there is no photometric nor spectroscopic data available for unidentified extinction media. However, we can still model and estimate its effect statistically. We now apply the exponential decay function e
-2d/D to the photon rate in Eq. (2): N=(N
0/4πd
2)*e
-2d/D = N
0/4π(de
d/D)
2 with the decay coefficient written as 2/D for subsequent convenience. Thus, the intergalactic extinction (IE) model can be written simply as
where dL is the indirectly measurable luminosity distance and D is a constant. D/2 is the distance by which 36.8% (1/e) photons remain alive from extinction, or the mean life-distance (analogue to mean lifetime for decays over time) of photons. (D was estimated to be 21.0 Gly with the Pantheon+ SN data as discussed in section 3 below.)
Figure 1 shows the behavior of d
L versus d under three different parameter values of D=13, 21, 29 Gly, and d
L=d as D->∞. The luminosity distance d
L approximates the true distance d well for small distance (d<<D) but deviates upwards exponentially.
It is important to note that only d
L can be calculated with the distance modulus m-M=5logd
L-5. The true distance d in a static universe (or the proper distance in an expanding universe) can only be calculated after the parameter D is estimated. These properties of d
L and d are independent of cosmological models, expanding or static. In the case of expanding universe models such as ΛCDM, the distance modulus overestimates the proper distance d with d
L, unless corrections are made to the modulus formula; and further, Hubble’s law is the ratio of recession velocity to the measured luminosity distance, and not to the proper distance. Since v=H
0d
L, we can place velocity v on the vertical axis in
Figure 1 which implies that the universe is decelerating instead of accelerating as the v-d curve is above the straight v=H
0d (or d
L=d). One may conclude an accelerating universe by using d
L but that is delusional as d
L is an overestimation.
2.3. The Redshift Model
Similar to the IE model, to model the light energy depletion due to redshift of each photon in the light, we apply the exponential decay function e
-d/Δ to Eq. (3): E
λ=E
λ0*e
-d/Δ, or λ= λ
0e
d/Δ. Since λ=λ
0(1+z),
where Δ is a constant. For d<<Δ and d<<D, with Taylor expansions, Eq. (4) and (5) reduce to d
L=d and z=d/Δ. Thus, we have Hubble’s law z=d
L/Δ in which Δ=c/H
0 and H
0 is the Hubble constant, and Δ
13.8 Gly is in fact the familiar Hubble distance. Given an observed value of z, the true distance to the light source can also be calculated simply with Eq. (5’). The observed d
L is very useful for estimation purposes but is not the true distance and is delusional as it does not take intergalactic extinction into account. Zhang [
7] offered an additional and interesting explanation of the physics at play for photons to redshift over distance.
Under this model, for each Hubble distance Δ traveled, the photon’s wave length is redshifted by e-1 (~1.72) or the associated photon energy remaining is 1/e (~36.8%). Δ is also the expected value of distance weighted by the energy level as probability density during a photon's entire trip from distance zero to infinity. While Δ=Hubble distance, it does not have the same interpretation here as under the expanding universe hypothesis as there is no expanding space and recession velocity in a static universe.
2.4. The Combined Empirical Model
Figure 2 shows the functions d
L(d) and z(d) graphically. Substituting Eq. (5’) into Eq. (4), we obtain the empirical d
L-z relationship:
Figure 2.
the functions dL(d) at D=21Gly, and z(d).
Figure 2.
the functions dL(d) at D=21Gly, and z(d).
In terms of the distance modulus μ
m-M=5logd
L-5,
Eq. (6) and (7) are equivalent and have two parameters, Δ (or H
0=c/Δ) and D (or Δ/D), which can be empirically estimated. (The total flux can also be written as E(d)=E
0e
-d(1/Δ+2/D) where E
0 is energy at source.)
Figure 3 and
Figure 4 shows the graphs of Eq. (6) and (7) respectively. The d
L-z relationship is a s-curve
1 closely approximating the straight d
L=Δz or Hubble’s law, with deviations
13.4% over 0
z
125 (for Δ=13.5 Gly and D=21 Gly taken from empirical estimation discussed in section 3 below). In other words, the luminosity distance per unit (100%) of redshift is roughly 13.5 Gly.
Note also the symmetry between Eq. (4) and (5) in terms of d
L/d and λ/λ
0(=1+z). We may call r
λλ/λ
0 the redshift ratio, and r
dd
L/d the dimshift ratio (as the light is shifted dimer by extinction). We take first derivatives with respect to d in (4) and (5) and get
Thus, Δ/D (0.64 per Pantheon+ SN sample) can be interpreted as the percentage change in the dimshift ratio as one percentage change in the redshift ratio or in wavelength λ.