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Sorry, you and all our scientists MUST except the observation as is.You must agree that based on wien-law the source temp for λ peak at 2000 is 2.75K.We can't argue about it.
I have already explained that infinite Universe with infinite sources of 2.75K can easily emit BBR spectrum.
Wiens-law is very clear as it gives the source temp for each detected λ peak.
They just want to keep the BBT alive.
They clearly know that based on wien-Law a 2.75K temp source for the CMBR is a fatal problem for the BBT
That is a fatal mistake.
At this phase I fully understand the real meaning of wiens-law
Quote from: Dave Lev on 03/03/2023 19:57:46Sorry, you and all our scientists MUST except the observation as is.You must agree that based on wien-law the source temp for λ peak at 2000 is 2.75K.We can't argue about it.No.I could post a blue square here.And then I could fit it to the Wein law and it would tell me that your computer screen is hotter than the surface of the sun.
He would say that if it was a thermal spectrum of a stationary object, it was the spectrum of something at 2.725K.
Only if you are stupid enough to ignore the fact that something may have happened to the spectrum between it leaving the source and it reaching us.
But I think he would also realise it could also be the spectrum of a hotter or a colder thing that was moving away or towards him.because he would, at least, have heard of Doppler's work.But if you told him it was the emission spectrum of low pressure hydrogen gas at 2.725K he would laugh at you.
At this phase I don't care how do we get this spectrum and if it is due to stationary object or not.
Hence, based on the OBSERVED spectrum of the CMBR its expected source temperature should be 2.725K
QuoteQuote from: Dave Lev on Today at 15:56:33Hence, based on the OBSERVED spectrum of the CMBR its expected source temperature should be 2.725KUnless the source is moving or something else is happening which you refuse to consider.
Quote from: Dave Lev on Today at 15:56:33Hence, based on the OBSERVED spectrum of the CMBR its expected source temperature should be 2.725K
I fully agree to consider everything.
However, I hope that we can finely agree on the following:Based on the OBSERVED spectrum of the CMBR its expected source temperature should be 2.725K, Unless the source is moving or something else is happening .Do you agree?
Quote from: Dave Lev on 04/03/2023 19:25:22However, I hope that we can finely agree on the following:Based on the OBSERVED spectrum of the CMBR its expected source temperature should be 2.725K, Unless the source is moving or something else is happening .Do you agree?I have said that all along.It's good that you agree, even if it took a while.
Can you please be more specific about that change?Do you have an idea what was the peak of the spectrum when it is leaving the source?Do you mean that at the source the peak was about 750 in order to meet the source of the Hydrogen recombination temp (which is 3000K)?Can you please explain how could it keep its BBR spectrum while it change its peak so dramatically?
Can you please explain how could it keep its BBR spectrum while it change its peak so dramatically?
Quote from: Dave Lev on 04/03/2023 20:02:45Can you please explain how could it keep its BBR spectrum while it change its peak so dramatically?It's really very easy.Move away from the source quickly.Doppler shift will give you the same "shaped" spectrum but shifted to longer wavelength so it looks like it has come from a cooler source.As has been pointed out, you cited a source which told you this.
Based on the OBSERVED spectrum of the CMBR its expected source temperature should be 2.725K, Unless the source is moving or something else is happening .
We can claim that:At T = 3500K, λrest = 750 nmThe T temp of the Hydrogen recombination is 3000K.Let's assume that its λrest is 780 nmAt T = 3000K, λrest = 780 nm (assumption)Based on the following CMBR data:https://www.astro.ucla.edu/~wright/CMB.htmlThe peak of the CMBR is at 2 mm (or 2000nm)Hence,CMBR λobserved = 2000nmZ CMBR= (λobserved -λrest) / λrest = (2000 - 780) / 780 = 1.564
Once again, you have missed something important.There is only one plausible thing in the universe which emits a black body spectrum without some sort of band or line structure superimposed on it.And that's a hot, fairly dense hydrogen plasma.If you do not believe that, please put forward an alternative that would emit BBR.So we absolutely unequivocally KNOW that it started out hot.Again, if you think there's another explanation, please let us know