On a non-primordial origin of the cosmic background radiation and pregalactic density fluctuations |
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Authors: | H.-E. Fr hlich, V. Mü ller,H. Oleak |
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Affiliation: | H.-E. Fröhlich, V. Müller,H. Oleak |
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Abstract: | Dusty pregalactic Population III objects may provide a mechanism for an effective thermalization of the star radiation. They may generate the observed microwave background and so the high cosmic photon entropy. Assuming a tepid universe a smaller primordial entropy contribution results in reasonable mass scales and amplification factors of pregalactic density fluctuations. |
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Keywords: | Cosmic background radiation Population III objects intergalactic dust galaxy formation cosmology |
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