Chalnoth, Would there be any radiation produced by incandescence due to the vibration of hot hydrogen atoms?
I just read that the main source of the CMBR is recombination:
The baryonic matter in the universe consisted of ionized plasma, and it only became neutral when it gained free electrons during "recombination," thereby releasing the photons creating the CMBR. How much broadening is as a result of dopler shift and is the broadening significant compared to the width of the black body radation?
At the time of the CMBR would there also have been a Hydrogen transition line emission at 1420MHz which would have been redshifted to 1.29MHz?
I believe that Radio waves can propagate through ionized gases with less attenuation. Perhaps there is just too much interference in this band?
I just found this although they are looking at lower red shift frequencies:
In cosmology the line is of great interest in big bang cosmology because it is the only known way to probe the "dark ages" from recombination to reionization. Including the redshift, this line will be observed at frequencies from 200 MHz to about 9 MHz on Earth. It potentially has two applications. First, by mapping redshifted 21 centimeter radiation it can, in principle, provide a very precise picture of the matter power spectrum in the period after recombination. Second, it can provide a picture of how the universe was reionized, as neutral hydrogen which has been ionized by radiation from stars or quasars will appear as holes in the 21 centimeter background.
However, 21 centimeter experiments are very difficult. Ground based experiments to observe the faint signal are plagued by interference from television transmitters and the ionosphere, so they must be very secluded and careful about eliminating interference if they are to succeed. Space based experiments, even on the far side of the moon (which should not receive interference from terrestrial radio signals), have been proposed to compensate for this. Little is known about other effects, such as synchrotron emission and free-free emission on the galaxy. Despite these problems, 21 centimeter observations, along with space-based gravity wave observations, are generally viewed as the next great frontier in observational cosmology, after the cosmic microwave background polarization.
Source:
http://en.wikipedia.org/wiki/Hydrogen_line