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The Hidden Hypotheses Behind the Big Bang It is quite unavoidable
that many philosophical a priori assumptions lurk behind the debate
between supporters of the Big Bang and the anti-BB camp. The same
battle has been waged in physics between the determinists and the
opposing viewpoint. Therefore, by way of introduction to this
symposium, I would like to discuss, albeit briefly, the many
"hypotheses," essentially of a metaphysical nature, which are often
used without being clearly stated. The first hypothesis is the idea
that the Universe has some origin, or origins. Opposing this is the
idea that the Universe is eternal, essentially without beginning,
no matter how it might change-the old Platonic system, opposed by
an Aristote lian view Or Pope Pius XII or Abbe Lemaitre or
Friedmann versus Einstein or Hoyle or Segal, etc. The second
hypothesis is the need for a "minimum of hypotheses" -the sim
plicity argument. One is expected to account for all the
observations with a mini mum number of hypotheses or assumptions.
In other words, the idea is to "save the phenomena," and this has
been an imperative since the time of Plato and Aristotle. But
numerous contradictions have arisen between the hypotheses and the
facts. This has led some scientists to introduce additional
entities, such as the cosmologi cal constant, dark matter, galaxy
mergers, complicated geometries, and even a rest mass for the
photon. Some of the proponents of the latter idea were Einstein, de
Broglie, Findlay-Freundlich, and later Vigier and myself."
The Hidden Hypotheses Behind the Big Bang It is quite unavoidable
that many philosophical a priori assumptions lurk behind the debate
between supporters of the Big Bang and the anti-BB camp. The same
battle has been waged in physics between the determinists and the
opposing viewpoint. Therefore, by way of introduction to this
symposium, I would like to discuss, albeit briefly, the many
"hypotheses", essentially of a metaphysical nature, which are often
used without being clearly stated. The first hypothesis is the idea
that the Universe has some origin, or origins. Opposing this is the
idea that the Universe is eternal, essentially without beginning,
no matter how it might change-the old Platonic system, opposed by
an Aristote lian view! Or Pope Pius XII or Abbe Lemaitre or
Friedmann versus Einstein or Hoyle or Segal, etc. The second
hypothesis is the need for a "minimum of hypotheses" -the sim
plicity argument. One is expected to account for all the
observations with a mini mum number of hypotheses or assumptions.
In other words, the idea is to "save the phenomena", and this has
been an imperative since the time of Plato and Aristotle. But
numerous contradictions have arisen between the hypotheses and the
facts. This has led some scientists to introduce additional
entities, such as the cosmologi cal constant, dark matter, galaxy
mergers, complicated geometries, and even a rest mass for the
photon. Some of the proponents of the latter idea were Einstein, de
Broglie, Findlay-Freundlich, and later Vigier and myself.
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Astrophysik II: Sternaufbau / Astrophysics II: Stellar Structure (English, German, French, Paperback, Softcover reprint of the original 1st ed. 1958)
Marshal H. Wrubel, H. C. Arp, G. R. Burbidge, E Margaret Burbidge, Hans E. Suess, …
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R3,063
Discovery Miles 30 630
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Ships in 10 - 15 working days
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Sects. 12, 13. 89 sequence and that subgiant and fainter stars in
globular clusters have ultraviolet excesses. When dealing with
stars whose physical properties are imperfectly under stood, such
as in globular cluster stars, we cannot rely too heavily on the
empiri cal calibration by the kinds of stars used to define Fig. 5,
to determine their true, unreddened U-B, B-V curve. But if by a
combination of arguments, principally the reddening in the region
of the stars we do known about, we can assign a fairly probable
unreddened U-B, B-V curve to a group of stars about which we know
little, the argument may be turned around. In this case some
information may be gained about the energy envelope of the stars by
examining the differences between the normal two-color index curves
for the unknown group of stars compared to the known. In general
there seem to be two possible causes for different stars defining
different normal sequences in the U-B, B-V plane. One, the relative
energy distribution in the continuum in the U, B and V photometry
bands are different. An example of this is the effect of the Balmer
depression in supergiants. This, of course, requires deviation from
black body radiation curves for one or both groups of stars. This
cause seems to be the dominant effect for very blue, hot stars
where the depression of the continuum by absorption lines is at a
minimum."
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