Accelerated expansion of the universe

Accelerated expansion of the universe

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Accelerated expansion of the universe Juergen Barsuhn 02-06-2010
Posted by Juergen Barsuhn on February 6, 2010, 4:36 am
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About half a century ago the expansion of the universe was
widely accepted and there were only small islands of
disbelief e.g. around Sir Fred Hoyle. It was expected that
the expansion velocity should decrease due to the masses in
the universe. The only question discussed further was,
whether the expansion would nevertheless continue infinitely
or would come to a halt, followed by a collapse.

Nowadays many (or most?) cosmologists believe in a
possibility not seen in those old times: the expansion is
accelerated, the expansion velocity is increasing. AFAIK
this is based on the luminosities of far distant supernovae,
leading to the conclusion that their home galaxies are
farther distant from us than anticipated from their
redshift. How reliable are these newly derived distances?
The age of the compared supernovae is dependent on their
distance. Maybe supernovae in the infant times of our
universe had - for some unknown reasons - a higher
luminosity. - I remind on the correction of galactic
distances that was necessary when the difference between
population I and population II Cepheids became apparent.

All the best Jurgen

Posted by Phillip Helbig---undress to re on February 6, 2010, 3:49 pm
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Fred Hoyle doubted many things, but not the expansion of the universe.
He doubted the big bang, and instead preferred a steady-state universe,
one which always looked the same. If this expands (as Hoyle---and most
cosmologists---believe on account of the cosmological redshift), then it
has to expand exponentially, with new matter being continuously created
to keep the mean density constant. (The latter is not in conflict with
observations, since the rate of creation is below detection thresholds.)

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This applies a) for a big-bang universe and b) if one neglects the
cosmological constant. Note that models with the cosmological constant
were discussed already during the 1920s. The main reason for
discounting them for a while was that calculations in them are much more
complicated and the observations weren't good enough to distinguish
between models anyway.

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As mentioned above, this was already discussed by Friedmann in the
1920s.

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To calculate the distance from the redshift, one has to assume a
cosmological model. It would be more correct to say that the galaxies
are fainter than would be expected from their redshift if one assumes no
cosmological constant.

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The distance is calculated, not derived. The error in the measurement
of the redshift is negligible. The problem is the luminosity. While
the apparent luminosity can be measured, there is some scatter because
there is some scatter in absolute luminosity. Since having a good idea
about the absolute luminosity is essential for this line of research, a
lot of work has gone into establishing that the supernovae are standard
candles.

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Maybe. But there is no reason to believe this, neither theoretically
nor observationally.

- I remind on the correction of galactic
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Yes, science is a self-correcting process, but that doesn't mean that
everything must be incorrect.

Posted by Juergen Barsuhn on February 22, 2010, 4:18 am
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Phillip Helbig---undress to reply schrieb:
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...... Thank you for all your comments that I have cut in
this reply
in order to concentrate on a detail ...

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......
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....These are the type Ia supernovae thought to be white
dwarf collapsing to a black hole if they gain some mass and
exceed a certain threshold. If you think of accretion and
the collapse starts as soon as the standard mass limit is
exceeded, it is easy to think of a standard candle. However,
if the supernova results from the merging of two white
dwarfs - and that is what recent results from Chandra
indicate - things appear more complicated. You may think of
two merging white dwarfs that together just exceed the mass
limit. Or of two white dwarfs each just a little bit below
the mass limit. As a rough guess I would expect twice the
luminosity of the first case. - How does one manage this
problem?
All the best Jurgen

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