Re: Cosmic_Inflation is an artificial model of the Planck_Length transition...

In article <Jeff_Relf_2006_Jun_11_DcQh@xxxxxxxxx>, Jeff?ĶRelf
<Jeff_Relf@xxxxxxxxx> wrote:

As I've point out many times before,
Cosmic_Inflation is an artificial model of the Planck_Length transition,
and it explains nothing that an ever-constant lambda wouldn't explain better
and with much, much more evidence

IN language even YOU can understand (i.e wiki)

http://en.wikipedia.org/wiki/Horizon_problem

"Inflationary theory allows for a solution to the problem (along with
several others such as the flatness problem) by positing a short 10-32
second period of exponential expansion (dubbed inflation) within the
first minute or so of the history of the universe. During inflation,
the universe would have increased in size by an enormous factor; enough
to account for the observed isotropy of today's particle horizon
looking back to the time the cosmic microwave background. The universe
before inflation is causally connected and doesn't come back into
causal contact until a much later time."

(Read up on Thermal Equilibrium and Black Body)

http://en.wikipedia.org/wiki/Flatness_problem

"Currently, observations indicate that ? is between 0.98 and 1.06 - in
other words, that the universe's density is very close to or exactly
the critical value. In its very early history, an ? only very slightly
above 1 would have resulted in a very rapid big crunch, while with an ?
only very slightly below 1, the universe would have expanded so fast
that stars and galaxies could not have formed. The fact that
approximately 14 billion years after its formation, the universe still
has an ? so close to unity indicates that ? must have been within one
part in 1015 of unity when the universe formed.

The problem is that a simple big bang theory cannot explain how an ? so
close to unity could arise. The problem is solved by the hypothesis of
an inflationary universe, in which very shortly after the Big Bang, the
universe increased in size by an enormous factor. Such an inflation
would have smoothed out any non-flatness originally present and
resulted in a universe with a density extremely close to the critical
density."

http://en.wikipedia.org/wiki/Monopole_problem#Attempts_to_find_monopoles

" Non-inflationary Big Bang cosmology suggests that monopoles should be
plentiful, and the failure to find magnetic monopoles is one of the
main problems that led to the creation of cosmic inflation theory. In
inflation, the visible universe was much smaller in the period before
inflation, and despite the very short time before inflation, it would
have been small enough for the whole visible universe to have been
within the horizon, and thus not requiring many monopoles, perhaps only
one. At the moment, versions of inflation seem to be the most likely
cosmological theories."


Now your homework for this week is to go to a library, get a copy of
Parallel Worlds by Kaku and read pgs 78 ~ 105. I will be asking
questions..

--
The greatest enemy of science is pseudoscience.

Jaffa cakes. Sweet delicious orangey jaffa goodness, and an abject lesson why
parroting information from the web will not teach you cosmology.
.

Relevant Pages

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