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Reionization: characteristic scales, topology and observability

Iliev, Ilian ; Pen, Ue-Li ; McDonald, Patrick ; Shapiro, Paul ; Mellema, Garrelt ; Alvarez, Marcelo

In: Astrophysics and Space Science, 2009, vol. 320, no. 1-3, p. 39-43

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    Titel
    • Reionization: characteristic scales, topology and observability
    Autor
    • Iliev, Ilian. Institut für Theoretische Physik, Universität Zürich, Winterthurerstrasse 190, 8057, Zürich, Switzerland
    • Pen, Ue-Li. Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, M5S 3H8, Toronto, ON, Canada
    • McDonald, Patrick. Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, M5S 3H8, Toronto, ON, Canada
    • Shapiro, Paul. Department of Astronomy, University of Texas, 78712-1083, Austin, TX, USA
    • Mellema, Garrelt. Stockholm Observatory, AlbaNova University Center, Stockholm University, 106 91, Stockholm, Sweden
    • Alvarez, Marcelo. Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 94305, Stanford, CA, USA
    Dokumententyp
    • Postprint
    Sprache
    • Englisch
    Veröffentlicht in
    • Astrophysics and Space Science, 2009, vol. 320, no. 1-3, p. 39-43. Springer Netherlands
    Andere elektronische Ausgabe
    OAI-PMH-ID
    • oai:doc.rero.ch:312974
    Summary
    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