期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 381, 期 1, 页码 L35-L39出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1745-3933.2007.00361.x
关键词
radiative transfer; methods : numerical; HII regions; intergalactic medium; quasars : absorption lines; cosmology : theory
We examine a large set of synthetic quasar spectra to realistically assess the potential of using the relative sizes of highly ionized near-zones in the Ly alpha and Ly beta forest as a probe of the neutral hydrogen content of the intergalactic medium (IGM) at z > 6. The scatter in the relative near-zone size distribution, induced by underlying fluctuations in the baryonic density field and the filtering of ionizing radiation, is considerable even for fixed assumptions about the IGM neutral fraction. As a consequence, the current observational data cannot distinguish between an IGM which is significantly neutral or one which is highly ionized just above z = 6. Under standard assumptions for quasar ages and ionizing luminosities, a future sample of several tens of high-resolution Lya and Ly beta near-zone spectra should be capable of distinguishing between a volume-weighted neutral hydrogen fraction in the IGM which is greater or less than 10 per cent.
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