marcus
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Hello Wimms, just saw your post. Only time for a quick answer. You replied to this frome me:
[[... "does the frequency really decrease as space
expands" and yes indeed it does. The frequencies in the
CMBR have declined by a factor of 1000.
Space stretching out makes their wavelengths longer and
that lowers their frequency by the same factor. Space
has expanded by a factor of 1000 since those photons were emitted and so their wavelengths are 1000 times longer and
their frequencies correspondingly lower.]]
In your reply you said:
Originally posted by wimms
Wait, just only 1000 times?? 13billion lightyears radius that was once singularity, expanded just 1000 times?
And, if even photon looses energy due to expansion, then anything should loose energy to expansion. Or, even, which is first, expansion causing loss of energy, or loss (dissipation) of energy causing expansion?
Since big bang there has been FAR more expansion than merely by a factor of 1100-----the factor for the CMBR.
The expansion has been by factor of 1100 since the epoch called "last scattering" or "recombination" which is when those CMB photons are thought to have been emitted.
The picture is of a clearing fog (actually hot plasma).
Above a certain temperature hydrogen gas is opaque, like the sun is opaque, because it is ionized into glowing plasma and is highly reactive with light. The electrons absorb and re-emit photons frantically.
Then as the plasma cools it suddenly becomes transparent because the neutral atoms form----no more free electrons.
The moment it becomes transparent, the photons are set free and fly essentially forever.
This cooling and transparency was reached at year 300 thousand, approx. This is the moment of origin of the CMB.
Matter behaves differently from light, in expansion. Matter too has an energy density (its mass-energy) but this falls off only as the cube------the energy simply spreads out into larger volume.
But light energy falls off as the fourth power. Because not only do there get to be fewer photons per volume but also each photon has its wavelength stretched out. This differential in the decline has an interesting effect. It changes the relative importance of matter versus light over time.
You ask which came first. The conventional view is that the expansion is a give and that the loss in CMB energy is simply one consequence of that.
Good question, thanks!
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