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Thanks for the reference, I downloaded & read the paper. I am actually quite amazed at the idea that this paper was written (evidently) by physics department faculty. The flaws are very elementary, and should have been obvious even to a first year physics student. To explain why I say this, let me point out two important formulae concerning blackbody radiation. They are the Stefan-Boltzmann Law and Plank's Radiation Formula (follow the links to see the equations and examine the physics). The Stefan-Boltzmann Law allows one to compute the total power radiated by a blackbody at a given temperature. One can also solve the equation backwards; given a total power, one can derive the temperature that a blackbody would need to have, in order to radiate that much power. This is commonly called the effective blackbody temperature, acknowledging the fact that the source of energy could be far from a blackbody. The Planck Radiation Formula is more complicated, because it describes the spectral energy distribution of the radiation from a blackbody at a given temperature. In other words, it describes the energy as a function of wavelength or frequency. If you integrate Planck's formula over all wavelengths (or frequencies), you get the power that shows up in the Stefan-Boltzmann law. Now, according to the paper both Gillaume (in 1896) and Eddington (in 1926), predicted the cosmic background. That is clearly not true, because both used the Stefan-Boltzmann law to compute the effective blackbody temperature, the temperature that a blackbody would have were it to radiate the total energy in the background starlight. But as Eddington points out (in the paragraph after the one that is qouted in the paper), the starlight is not in thermodynamic equilibrium. Neither Guillaume nor Eddington mentions Planck's formula. I don't think that Guillaume mentions the spectral energy distribution, but Eddington does, in making the point that his temperature is an effective blackbody temperature (Eddington's words), and that the background is not in thermodynamic equilibrium (which Eddington certainly knew meant that it could not have a blackbody spectrum). So far as I can tell, the discussion of Regener & Nernst concerns cosmic ray energies, and is not relevant to cosmic microwave background. Born's temperature is, as far as I can tell, a kinetic temperature of the scattering medium that produces the redshift in Finlay-Freundlich's tired light redshift model. I don't see the connection to a background radiation field here either. The fact appears to me that there has never been any prediction of the cosmic background temperature to match the big bang prediction, from any static model. And none were presented in the paper by Assis & Neves. They did not reference any predictions concerning the spectrum of the background radiation, and that's the real point of alluding to the success of the big bang in predicting the cosmic background temperature. Here the point is that the CMB spectrum is the most precise fit to Planck's formula ever seen, including laboratory black body experiments. That was the key prediction of big bang cosmology. Competing cosmologies can produce thermal background, but only as a special case, or as an improbable event. But only big bang cosmology requires that the spectrum of the background radiation conform to Planck's formula. So why isn't this in "against the mainstream"? |
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http://www.geocities.com/kingvegeta80/BBT.html Quote "Original estimates on the CMB's temperature ranged from 20°K (est. by George Gamow) to 30°K (est. by Jim Peebles). The Stefan/Boltzmann law states that the amount of energy in a blackbody radiation field is proportional to its temperature to the fourth power (see the appendix). So here we have estimated energy output amounts as follows, which is measured in watts per square metre: Gamow est.: 20°K4= 9 x 10-3 Watts/m2 Peebles est.: 30°K4= 4.6 x 10-2 Watts/m2 Actual temp.: 2.7°K4 = 3.01 x 10-6 Watts/m2 So we now have the original estimates of having anywhere from about 3000 to over 15,000 times energy than what is actually observed. Even Robert Dicke claimed that his group had estimated a temperature of 10°K, but that still yields just over 188 times what is actually observed. The observed temperature indicates a much more diffuse universe as was previously thought, ruling out the oscillating universe model. Ironically, non-expanding universe models predicted the 3 °K background radiation long before Penzias and Wilson discovered it (there is a link to a paper on this on Vincent Sauvé's page). Edited to add this link http://www.dfi.uem.br/~macedane/history_of_2.7k.html The temperature is only an immediate problem for a closed (esp. oscillating) BB universe, but still also poses major problems for other high-Omega value scenarios, including the flat (Ω=1) universe scenario that is the most widely accepted. The real problem is the smoothness of the CMB. It is something that greatly contradicts original estimates. Irregularities in the CMB are supposed to reflect clumps in the early universe that would later condense into structures like galaxies. Original observations showed that it was completely smooth, but this later turned out not to be the case. When the COBE (Cosmic Background Explorer) satellite was deployed in November of 1989, it carried instruments to analyze the CMB. It has since detected anisotropies of one part in 100,000. The CMB was once again headline news, with some headlines calling it "the most important discovery of all time" and other even more gratuitous praises. However, even these irregularities were too small. The original estimates of anisotropy (made throughout the 1970s) required fluctuations of about one part in 1000--a hundred times more irregular than what is actually observed--to form even small structures like galaxies (that's not including clusters and superclusters, see below). These all indicate a universe way too diffuse to comply with the BBT." |
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http://www.ifi.unicamp.br/~assis/ Of course, his views are towards the static model side, so may not appeal to a wide audience. Quote:
The biggest problem for static models is not in predicting the CMBR spectrum, but rather that there is still not a redshift mechanism that everyone can sign on to. My view is that once we have the redshift mechanism, some of the other problems, like the CMBR spectrum and time dilation in SNe, will come out at the same time. For static modellers, though, these sorts of problems can serve as useful clues to the nature of the solution. Quote:
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http://redshift.vif.com/JournalFiles...F/V02N3INT.PDF Quote:
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There is another argument to show that static models can account for the CMBR temperature. If we take the average rate of input of stellar radiation into space, over a sufficiently large volume of space, we find that it equals the rate at which energy is lost from the CMBR due to redshift in the CMBR photons. This shows at minimum that there is an energy balance in a static model. The BB can't explain this. Here's a ref where this is discussed: http://redshift.vif.com/JournalFiles...F/v05n3edw.pdf Quote:
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What do you think of the "bullet list" (currently revised edition - see original post)? I am considering a second complimentary paraphrased list, Robin Williams' style, to help explain them but I mainly want a quick outlined version that I can memorize for reference. Should I do so? Anyone think entropy should be a bullet???? Is there any evidence to support that a process could create negative entropy for the universe? No fair dumping any wastes outside our known universe (at least until evidence supports an alternative). I always liked the rephrased second law...."heat won't go from a cooler to a hotter, you can try if you like but you far better notter"!
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And I would suggest that anyone contradicting claims made by TT does so at the peril of their credibility.
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Quote "Original estimates on the CMB's temperature ranged from 20°K (est. by George Gamow) to 30°K (est. by Jim Peebles). The Stefan/Boltzmann law states that the amount of energy in a blackbody radiation field is proportional to its temperature to the fourth power (see the appendix). So here we have estimated energy output amounts as follows, which is measured in watts per square metre: Gamow est.: 20°K4= 9 x 10-3 Watts/m2 Peebles est.: 30°K4= 4.6 x 10-2 Watts/m2 Actual temp.: 2.7°K4 = 3.01 x 10-6 Watts/m2 So we now have the original estimates of having anywhere from about 3000 to over 15,000 times energy than what is actually observed. Even Robert Dicke claimed that his group had estimated a temperature of 10°K, but that still yields just over 188 times what is actually observed. |
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Everything I need to know I learned through Googling. |
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http://www.dfi.uem.br/~macedane/history_of_2.7k.html Quote:
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What is the date of publication? Edited Why the temperature for the predicted black-body curve was so different than the observations have reported? And (I repeat)theoricians working outside the Big Bang model were able to do a better job in their temperature prediction with the datas available at the time. |
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"The Physics of the Expanding Universe," George Gamow, Vistas in Astronomy 2, 1726-32 [1956] which predicts a 6 degree background. However, I have to admit that I haven't worked the calculations through in detail to confirm that this is supposed to be a black body. Quote:
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I agree, however, that there needs to be evidence that the pro-BB camp predicted the black-body curve ahead of time. Unfortunately, my physics and math are a little too rusty to be able to verify this without an effort.
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Read ToSeek previous post Quote:
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I repeat: The blackbody prediction is inherent in the big bang theory. If there was a big bang, there must have been a time when the universe was in thermal equilibrium. Period. No big bang theorist needed to publish this obvious fact.
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That is exactly the notion than they have predicted a PERFECT blackbody curve than I doubt. Of course based on the temperature expected from 6K to 50K they have speculated than the CMBR will show a black- body curve. Quote:
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