2002/06/25 by T. Theuns, Tom Theuns, M. Bernardi +11 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #Physics #Quasar #Redshift #Reionization #Sample (material) #Sky #astro-ph
paper · pdf · doi:10.1086/342531
published as Astrophys.J.574:L111-L114,2002 · 4 pages, 3 figures. Minor changes, to be published in ApJL
arxiv created 2002/06/25 · openalex publication_date 2002/08/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The expansion of the universe leads to a rapid drop in the hydrogen Ly effective optical depth of the intergalactic medium (IGM), N/Aeff(1+z)3.8, between redshifts 4 and 3. Measurements of the temperature evolution of the IGM and of the He ii opacity both suggest that He ii reionizes in this redshift range. We use hydrodynamical simulations to show that the observed temperature increase associated with He ii reionization leads to a relatively sudden decrease in N/Aeff around the reionization epoch of 10%. We find clear evidence for such a feature in the evolution of N/Aeff determined from a sample of 1100 quasars obtained from the Sloan Digital Sky Survey. He ii reionization starts at redshift 3.4 and lasts for z0.4. The increase in the IGM temperature also explains the widths of hydrogen absorption lines as measured in high-resolution spectra.