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Early Reionization in Cosmology

Published in Infrared Physics & Technology. 1994, vol. 35, no. 2-3, p. 83-94
Abstract The cosmic microwave background (CMB) anisotropies have turned out to represent one of the most stringent 'bottle necks' for scenarios of large scale structure formation. As a possibility to relax this constraint, it has been proposed that early reionization can damp CMB fluctuations on small scales due to photon diffusion in the ionized plasma. As an example, I investigate the recently proposed scenario with cold dark matter (CDM) and texture seeds. There, an analysis of CMB anisotropies shows that early reionization is a crucial ingredient for this scenario. Without damping, the small scale anisotropies would dominate and exceed observed limits. In this paper I present analytical and numerical results for the amount of damping due to early reionization for CMB perturbations induced by a collapsing texture. Furthermore, the spectral distortion of the CMB due to Compton scattering of the hotter plasma electrons is calculated. Next I discuss the physical processes which lead to a system of coupled ordinary differential equations for the degree of ionization, the electron temperature and the evolution of the ionizing radiation.
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DURRER, Ruth. Early Reionization in Cosmology. In: Infrared Physics & Technology, 1994, vol. 35, n° 2-3, p. 83-94.

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Deposited on : 2009-02-26

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