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The Topology of Cosmological Reionization

  • Authors: Khee-Gan Lee, Renyue Cen, J. Richard Gott III, and Hy Trac

Lee et al. 2008 The Astrophysical Journal 675 8.

  • Provider: AAS Journals

Caption: Fig. 3.

Left: Contour threshold densities as a function of ν (or equivalently, volume fraction f; see eq. [1]) at different redshifts. Note that the threshold densities do not decrease monotonically in the early phases, between ﹩z\sim 25﹩ and ﹩z\sim 17﹩ (see discussion in text). Right: Redshift evolution of the threshold densities at ﹩f=0.93﹩ or ﹩\nu =-1.5﹩ (dotted line), ﹩f=0.5﹩ or ﹩\nu =0﹩ (solid line), and ﹩f=0.07﹩ or ﹩\nu =1.5﹩ (dashed line).

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