Cosmic Reionization and High Redshift QSO Absorption Line Systems (宇宙における第一世代天体形成)

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概要

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• Full radiative transfer in 3D space has been solved to pursue the reionization history in an inhomogeneous universe. It has been shown that the reionization of an inhomogeneous universe is not a prompt event, but a fairly slow process. Also, QSO absorption line systems are simulated with using the results of radiative transfer calculations. Lyα continuum depression (D_A) implies that the metagalactic UV intensity decreases rapidly with z at z>5, and the reionization must have taken place between z=6 and 10. Finally, it is stressed that Hα forest is a more powerful probe to explore the reionization history and the density fluctuations in the universe at z>5.

• 素粒子論グループ 素粒子研究編集部の論文
• 1999-12-20

著者

• 梅村 雅之

  筑波大学

• 梅村 雅之

  筑波大

• NAKAMOTO Taishi

  筑波大

• SUSA Hajime

  筑波大

関連論文

• HMCS-G : グリッド環境における計算宇宙物理のためのハイブリッド計算システム(グリッド応用)
• Cosmic Reionization and High Redshift QSO Absorption Line Systems (宇宙における第一世代天体形成)

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