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
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
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
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
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
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 ( 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
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.
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
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
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.
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.
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