Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

14 pages, 10 figures, submitted to MNRAS

Scientific paper

10.1111/j.1365-2966.2006.10292.x

The intergalactic neutral hydrogen which is responsible for the Lyman alpha forest of quasar absorption is a tracer of much larger amounts of ionised hydrogen. The ionised component has yet to be detected directly, but is expected to scatter CMB photons via the Sunyaev-Zel'dovich (SZ) effect. We use hydrodynamic simulations of a LambdaCDM universe to create mock quasar spectra and CMB sky maps. We find that the high-z Lya forest gas causes temperature fluctuations of the order of 1 muK rms in the CMB on arcmin scales. The kinetic and thermal SZ effects have a similar magnitude at z=3, with the thermal effect becoming relatively weaker as expected at higher z. The CMB signal associated with lines of sight having HI column densities > 10^18 cm^-2 is only marginally stronger than that for lower column densities. The strong dependence of rms temperature fluctuation on mean Lya absorbed flux, however, suggests that the CMB signal effectively arises in lower density material. We investigate the use of the cross-correlation of the Lya forest and the microwave background to detect the SZ effect at redshifts 2-4. In so doing we are able to set direct limits on the density of diffuse ionised intergalactic baryons. We carry out a preliminary comparison at a mean redshift z=3 of 3488 quasar spectra from SDSS Data Release 3 and the WMAP first year data. Assuming that the baryons are clustered as in a LambdaCDM cosmology, and have the same mean temperature, the cross-correlation yields a weak limit on the cosmic density of ionised baryons Omega_(b,I), which is Omega_(b,I) < 0.8 at 95% confidence. With data from upcoming CMB telescopes, we anticipate that a direct detection of the high redshift ionised IGM will soon be possible, providing an important consistency check on cosmological models.

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

Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift 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 Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-167475

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