Cosmological molecular hydrogen and the distortion of the relict radiation spectrum

Details Cosmological molecular hydrogen and the distortion of the relict radiation spectrum Cosmological molecular hydrogen and the distortion of the relict radiation spectrum

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..88...21k&link_type=abstract

Astrophysics and Space Science, vol. 88, no. 1, Nov. 1982, p. 21-30.

Astronomy and Astrophysics

Astrophysics

4

Astronomical Spectroscopy, Cosmology, Hydrogen, Molecular Spectra, Photons, Relic Radiation, Distortion, Emissivity, Molecular Oscillations, Molecular Rotation

Scientific paper

The distortions of the relict radiation spectrum in the wavelength region shorter than 120 microns are considered. These distortions are due to the emission of photons under the formation of molecular hydrogen in the expanding universe, in the cosmological epoch with reshift value in the 40-200 range. It is shown that the real intensity of the relict radiation in the region of the wavelength under consideration must significantly exceed Planck's intensity, with a radiation temperature amounting to 2.8 K.

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