@Herald,
One thing at a time, your use of English is, Im afraid, not skillful. I have no idea what you are trying to convey with your usage of "Precondition". Precondition to what? and what preconditions specifically? (You fail to state that something even IS a "precondition")
You just assume everything and toss random words out of your closet.
The Cosmic background Radiation has been associated with the Big "Bang" because its existence does NOT support anything but a temperature profile associated with a rapid expansion of the Universe
The cosmic microwave background (CMB) is the thermal radiation left over from the "Big Bang" of cosmology. The CMB is a cosmic background radiation that is fundamental to our observations about the start up of the Universe because it is the oldest light in the universe.
With a traditional optical telescope, the space between stars and galaxies (the background) is completely dark. However, a sufficiently sensitive radio telescope shows a faint background glow, almost exactly the same in all directions, that is not associated with any star, galaxy, or other object. This glow is strongest in the microwave region of the radio spectrum. The CMB's serendipitous discovery in 1964 by American radio astronomers Arno Penzias and Robert Wilson , which earned them the 1978 Nobel Prize.
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The CMB is well explained as radiation left over from an early stage in the development of the universe, and its discovery is considered a landmark test of the Big Bang model of the universe. When the universe was young, before the formation of stars and planets, it was denser, much hotter, and filled with a uniform glow from a white-hot fog of hydrogen plasma. As the universe expanded, both the plasma and the radiation filling it grew cooler. When the universe cooled enough, protons and electrons combined to form neutral atoms. These atoms could no longer absorb the thermal radiation, and so the universe became transparent instead of being an opaque fog. Cosmologists refer to the time period when neutral atoms first formed as the recombination epoch, and the event shortly afterwards when photons started to travel freely through space rather than constantly being scattered by electrons and protons in plasma is referred to as photon decoupling. The photons that existed at the time of photon decoupling have been propagating ever since, though growing fainter and less energetic, since the expansion of space causes their wavelength to increase over time (and wavelength is inversely proportional to energy according to Planck's relation). This is the source of the alternative term relic radiation. The surface of last scattering refers to the set of points in space at the right distance from us so that we are now receiving photons originally emitted from those points at the time of photon decoupling.
Measurements of CMB are critical toany understandings of Cosmology , since any proposed model of the universe must explain this radiation. The CMB has a thermal black body spectrum at a temperature of 2.72548±0.00057 K. The spectral radiance dEν/dν peaks at 160.2 GHz, in the microwave range of frequencies.
The glow is very nearly uniform in all directions, but the tiny residual variations show a very specific pattern, the same as that expected of a fairly uniformly distributed hot gas that has expanded to the current size of the universe. In particular, the spectral radiance at different angles of observation in the sky contains small irregularities, which vary with the size of the region examined. They have been measured in detail, and match what would be expected if small thermal variations, generated by quantum fluctuations of matter in a very tiny space, had expanded to the size of the observable universe we see today. This is a very active field of study, with scientists seeking both better data (for example, the Planck spacecraft) and better interpretations of the initial conditions of expansion.
Although many different processes might produce the general form of a black body spectrum, no model other than the Big Bang has yet explained the fluctuations. As a result, most cosmologists consider the Big Bang model of the universe to be the best explanation for the CMB
The "Math models" you seem to deny are all satisfied by the present theory and several space craft (including the Planck satellite are studying the structure and anisotropy of the CMB radiation even closer.
Prhaps by a little closer reading you could understand things without panicking or defaulting
Quote: Forget about the Hubble constant, why don't you tell us what you think.
I think the Hubble Constant is 17 X 10^-3 meters/sec/light year.
Of course weve only been studying the Hubble constant for a few decades. Maybe it isn't really a constant.
The concept of the speed of the RECESSION of GALAXIES (as measured by red shifts) is pretty nicely proportional to its distance from us and the HUBBLE CONSTANT is that "constant" of proportionality (KInda hard to ignore it when it gives us a nice strait line for the
v=H* D
(Where the H* is the Hubble Constant).
Once again, math comes to our aid. (SEE A PATTERN HERE?)
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Can you prove this: that notwithstanding what the preconditions might be, the validity of any theory remains unshakable?
If you succeed to prove this, some day you may outperform yourself by proving that notwithstanding what the data and the evidences in support or in contradiction to a given theory might be ... and how many black boxes it may be grounded on, the validity of the theory remains unshakable
This is , perhaps your zenith of gobbledeegook. I have no idea what youre trying to communicate. See, the success of this whole A2K thing is heavily dependent on people understanding what we each are saying. Im having trouble figuring out what your points are and even what your sentence structure is?
ALL I can say is that evolution theory, (mainly the concept of evolution by natural selection) has been discovered and evidenced quite strongly over the last 155 years. ALL EVIDENCE SUPPORTS NAT SELECTION AND NO EVIDENCE REFUTES IT.