Issue |
A&A
Volume 458, Number 2, November I 2006
|
|
---|---|---|
Page(s) | L29 - L32 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20066191 | |
Published online | 15 September 2006 |
Letter to the Editor
Free-bound emission from cosmological hydrogen recombination
1
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching bei München, Germany e-mail: jchluba@mpa-garching.mpg.de
2
Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia
Received:
4
August
2006
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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