5.4 Star
build-up
rate
According to measurements performed
by the Hubble space telescope, there are, at the borders of the
observable
universe, at least ten times as many low- luminous galaxies than in our
cosmic vicinity [38]:
“The early universe was crowded
by more- than- average blue galaxies having apparent, strong emission
lines.
From this can be concluded that they built up stars much faster than
today’s
galaxies, as only an extensive population of very hot suns is able to
excite
the gas within the system to such a strong luminosity. Such hot suns
only
exist for a relatively short period of some million years and therefore
must have built up incessantly, at that time.”
This high star build-up rate in
the early universe resulting from observation coincides with the CTH,
which
also demands a higher star build-up rate for the past than for today:
(M
~ t 2/3,
~ t - 1/3 ).
The short duration of stars’ life
in the early universe from today’s view also comes the way of the CTH,
as at that time, the typical time t (cosmic
time) was extended in relation to the now time: Dt
/D
t ~ t -1/3
5.5
Discrepancy
between distance and red shift of supernovae in far galaxies
Under the title: “Revolution
in
the cosmology ”, a rather strange picture of the universe’s development
was presented, based on the measurement of the space- time by means
of
so- called 1a- supernovae [40], p. 38 ff:
“The finding:
Some billion years ago, the
universe
expanded slower than today. Therefore, contrary to present assumption,
the expansion rate increases.
The observation:
The decisive indication to the
increased expansion rate of the cosmos was given by supernovae in far
galaxies,
the observed maximum luminosity of which is a measure for their
distance
.”
According to this, the observed
supernovae would be more distant than their red shifts indicate, or,
resp.
, their red shifts would be lower than their distance indicates.
|
|
|
|
|
|