Cosmological H II regions and the photoionization of the intergalactic medium

Mathematics – Logic

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

29

Big Bang Cosmology, H Ii Regions, Intergalactic Media, Photoionization, Quasars, Absorption Spectra, Red Shift

Scientific paper

The generalization of the classical H II region problem to the case of a point source of ionizing radiation in a cosmologically expanding gas in a Friedmann-Robertson-Walker universe is summarized. An application of this work is described in which is tested the hypothesis that quasars photoionize the IGM to the degree implied by the well-known absence of a Gunn-Peterson effect. Recent studies of faint quasars at high redshift, which suggest a decline in the number density of quasars for z greater than three, imply that the H II regions of high-redshift quasars cannot overlap early enough to satisfy the Gunn-Peterson test. This suggests that either the observations are failing to detect the true number density of high-redshift quasars or else something else must ionize the IGM at high redshift.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cosmological H II regions and the photoionization of the intergalactic medium does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cosmological H II regions and the photoionization of the intergalactic medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological H II regions and the photoionization of the intergalactic medium will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1740299

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.