Volume 458, Number 2, November I 2006
|Page(s)||L29 - L32|
|Published online||15 September 2006|
Letter to the Editor
Free-bound emission from cosmological hydrogen recombination
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching bei München, Germany e-mail: email@example.com
2 Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia
Accepted: 7 September 2006
In this letter we compute the emission coming from the direct recombination of free electrons to a given shell () during the epoch of cosmological hydrogen recombination. This contribution leads to a total of one photon per recombined hydrogen atom and therefore a ~ increase in the recombination spectrum within the frequency range . In particular, the Balmer-continuum emission increases the distortion at GHz by roughly . With our 100 shell calculations for the hydrogen atom, we find that a total of ~5 photons per hydrogen atom are emitted when including all the bound-bound transitions, the 2s two-photon decay channel, and the optically thin free-bound transitions. Since the direct recombination continuum at high n is very broad, only a few n-series continuua are distinguishable and most of this additional emission below GHz is completely featureless.
Key words: cosmic microwave background
© ESO, 2006
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