2.3.3  The Velocity of Recession of a Distant Galaxy.

The recessional velocity that is to be derived here is for a galaxy far from the centre of the Universe and also at a time when the second phase of evolution is well established. This scenario has been chosen so that the resulting relationship can be approximated for comparison with empirical results determined via observations on the Earth at the present day.

The velocity of recession of such a galaxy is determined from the internal temporal rate of the Universe in phase II, which from Fig. 3, for the general point si, is given by

ui = æ
è
1- au si2

su3
ö
ø
1/2

 
(2.18)

The velocity of any mass subject to an Acceleration Potential in a Relativistic Domain is given by [2], Eq. (3.2), repeated here for convenience

×
s
 
= cu æ
è
1- u2

u02
ö
ø
1/2

 
(2.19)
Applying this using (2.18) to a distant receding galaxy, there is after minor reduction
×
s
 

i 
= ui

u0
( gmu )1/2 æ
è
si2

su3
- s02

su03
ö
ø
1/2

 
(2.20)
Where
si is the current radial position of the distant galaxy from the centre of the Universe.
s0 is the initial radial position of the galaxy from the centre of the Universe, i.e. the radial position where its inward motion from Phase I was halted in Phase II.
u0 is the temporal rate at s0.
su0 is the radius of the Universe when si=s0.
The temporal rate u0 is given by
u0 = æ
è
1- au s02

su03
ö
ø
1/2

 
(2.21)

If the point of inflexion, the point where the inward motion of the galaxy from phase I is halted in phase II, is close to the centre, then by comparison with si and su, s0 may be approximated to zero, and therefore u0 may be approximated to unity. Eq. (2.20) may then be restated as

×
s
 

i 
@ ui æ
è
gmu

su3
ö
ø
1/2

 
si
(2.22)

Eq. (2.22) shows that the velocity of recession for a distant galaxy is directly proportional to its distance from the centre of the Universe. This agrees with the empirical results of Edwin Hubble in 1929 and others since. The coefficient of (2.22) can therefore be compared with the Hubble constant. This will form the subject of the next Section.

2.3.4  Derivation of a Theoretical Expression for the Hubble Constant.

With the results obtained in Section 2.3.3, the derivation of this relationship has already been effected and from (2.22) can be stated directly as

H0 = ui æ
è
gmu

su3
ö
ø
1/2

 
(2.23)

Accordingly (2.20) is the full theoretical version of Hubble's law of motion for receding galaxies in phase II.

It should be noted that, because su varies with time, thereby causing a variation in ru the matter density of the Universe, from (2.23) and (2.24) below, it is therefore evident that H0 is in fact not a constant but will also vary with time. However, in view of the magnitude of the parameters involved, mass, radius and density of the Universe, such variation will only be significant over cosmological periods. Furthermore, the presence of ui in (2.23) shows that H0 also varies with distance from the centre of the Universe. This variation is again however, due to the nature of ui, a small one. These matters will be discussed in more detail in Section 3.

The relationship expressed by (2.23) can of course only be verified by comparing the numerical value it produces with those derived empirically. From (2.23) it can be seen that this would require knowledge of the energy mass of all matter in the Universe, together with its radius. Neither of these parameters are known. In addition, knowledge of ui is required which effectively means that the location in question, i.e. the point of measurement, (the Earth), in relation to the centre of the Universe is also needed. Again, an unknown parameter. Although ui is a variable as is evident from (2.18), its value will always be just below unity. Therefore to enable an estimate of H0 to be made, ui will be taken as unity which will accordingly give a slightly high value for H0. Therefore, with ui = 1, rewriting (2.23), as

H0 = æ
è
4

3
pgru ö
ø
1/2

 
(2.24)
where
ru is the average density of all matter in the Universe.

enables a value for H0 to be computed using current estimates for ru. The average density of all matter in the Universe has been estimated from such exercises as counts of stellar objects per unit stellar volume and the density then calculated via estimates of the masses of the objects counted. Two such estimated densities are shown in the following table.

ru (g/cm3)ReferenceNote
1 x 10-29[8]1
6.69 x 10-29[9]2
Table 1 Average Density of All Matter in the Universe.
Notes:-
1:- By comparison with the second estimate, some allowance for the mass of dark matter may have been made here, but has not been stated.
2:- This figure, calculated from the proton mass given in [10], is quoted as the equivalent proton mass per cubic metre, (0.4), and incorporates the assumption that the mass of proposed dark matter in the Universe is 10 times that of luminous matter.

Using a figure of 6.67 x 10- 8 cm3/g.sec2 for g, [7], insertion of the numbers in Table 1 into (2.24) gives a range of values for H0 as


H0 = 1.67 x 10-18     to    4.3 x 10-18 sec-1
(2.25)

However, Hubble's constant is normally quoted in units of Km/sec/10 6 L.Y., and the corresponding numbers from (2.25) in these units are


H0 = 15.8     to    40.7 Km/sec/10 6 L.Y.
(2.26)
with an average of

H0 = 28.3 Km/sec/10 6 L.Y.
(2.27)

To compare this figure with empirically derived estimates, reference is made to Table 2 below where, from the "Big Bang" model of the Universe's origin, most figures have been quoted in years for the age of the Universe.

Reference Age of UniverseActual/Equivalent Value of H0
(Years x 109) (Km/sec/10 6 L.Y.)
[8]1030
[9]-20
[11]13 to 2213.6 to 23.1
[12]10 to 2014.9 to 30
[13]10 to 2014.9 to 30
[14]1520.1
[14]-29.8
Table 2 Empirical Estimates of Hubble's Constant
The average of all the figures for H0 in Table 2 is

H0 = 22.6 Km/sec/10 6 L.Y
(2.28)
which concurs exactly with more modern estimates, [15].

Thus the comparison between the theoretical, Eq.(2.27), and the empirical, Eq.(2.28), values for H0 yields agreement to within some 18%. Considering the difficulty in determining such parameters as galactic distance, velocities via the Doppler shift in spectral wavelength, and galactic masses etc, this degree of agreement is considered very good. Even so, despite the improvement that could be realised by the inclusion of the correct value for ui, it is seen that the larger of the two theoretical figures is considerably larger than the largest empirical figure. As noted earlier, the estimate for the average density of matter in the Universe, upon which this figure is based, has, via the mass to light ratio comparison method been inflated by a factor of 10. However, if it exists at all, that method of assessment of the density of dark matter, may be flawed due to the effect of the solar wind on free particles within the Solar System, dark or otherwise. Hence the higher figure for density used in the theoretical computation for H0 may be too high. If this were the case, the agreement between the theoretically and empirically derived figures could be closer.

Finally, it is necessary to further clarify this derivation, and the comparison of H0 with empirical results, for their cosmological time of applicability. The values of average density in Table 1 involve observations over wide parts of the cosmos from the astronomically nearby to the cosmologically distant. In doing so, the observations are of the Universe as it was in the past. The greater the distances the further in the past are the objects being observed. Because the density of the Universe is changing with time, the particular value of density that is eventually arrived at is therefore a composite made up from observed objects from relatively recent cosmological periods to extremely remote ones. This density will therefore correspond to some particular cosmological time somewhere in between the two extreme times associated with the applicable observations. Call this time tC. Consequently, the theoretical value of Hubble's constant will likewise correspond to this particular past cosmological time tC.

In a similar manner, the empirical determinations of the Hubble constant will suffer from exactly the same problem. The further away an observed galaxy is, the further back in time will its measured parameters correspond to. As a result the empirical values of the Hubble constant shown in Table 2 above will represent parameters over a past cosmological period. The average will therefore, as in the case of the density, correspond to some past cosmological time. The fact that the theoretical and empirical figures of H0 agree relatively well is because their cosmological times of applicability are very close. This coincidence occurs simply because the objects observed in the determination of both parameters, density of the Universe and the empirical values of H0, were from the same statistical population.

C1 Version 2.1.1
Ó P.G.Bass March 2006

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