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Reionization: characteristic scales, topology and observability
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2009 (English)In: Astrophysics and Space Science, ISSN 0004-640X, E-ISSN 1572-946X, Vol. 320, no 1-3, 39-43 p.Article in journal (Refereed) Published
Abstract [en]

Recently the numerical simulations of the process of reionization of the universe at z>6 have made a qualitative leap forward, reaching sufficient sizes and dynamic range to determine the characteristic scales of this process. This allowed making the first realistic predictions for a variety of observational signatures. We discuss recent results from large-scale radiative transfer and structure formation simulations on the observability of high-redshift Ly- α sources. We also briefly discuss the dependence of the characteristic scales and topology of the ionized and neutral patches on the reionization parameters.

Place, publisher, year, edition, pages
2009. Vol. 320, no 1-3, 39-43 p.
Keyword [en]
High-redshift, Galaxies: formation, Intergalactic medium, Cosmology: theory, Radiative transfer, Methods: numerical
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Astronomy
Identifiers
URN: urn:nbn:se:su:diva-31871DOI: 10.1007/s10509-008-9865-9ISI: 000264174700008OAI: oai:DiVA.org:su-31871DiVA: diva2:278853
Available from: 2009-11-30 Created: 2009-11-30 Last updated: 2017-12-12Bibliographically approved

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Mellema, Garrelt
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