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High Redshift Intergalactic Medium: Probes and Physical Models

Shiv K. Sethi
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Abstract

Recent years have seen major advances in understanding the state of the intergalactic medium (IGM) at high redshift. Some aspects of this understanding are reviewed here. In particular, we discuss: (1) Different probes of IGM like Gunn-Peterson test, CMBR anisotropies, and neutral hydrogen emission from reionization, and (2) some models of reionization of the universe.

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Shiv K. Sethi. 2004-11-02. High Redshift Intergalactic Medium: Probes and Physical Models. https://arxiv.org/abs/astro-ph/0411050

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