The two-point correlation function of randomly distributed Lyman alpha clouds

Details The two-point correlation function of randomly distributed Lyman alpha clouds The two-point correlation function of randomly distributed Lyman alpha clouds

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..127f&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 127-128 (SEE N93-26706 10-90)

Physics

Background Radiation, Lyman Alpha Radiation, Mean Free Path, Quasars, Statistical Correlation, Monte Carlo Method, Photons, Red Shift, Ultraviolet Radiation

Scientific paper

It is often assumed that Ly-alpha forest clouds are randomly distributed, intergalactic objects that are highly ionized by the UV background produced by quasars. If these assumptions are true, fluctuations in the UV background should produce a nonzero two point correlation function in the Ly-alpha forest. This effect, which is really just a generalization of the proximity effect, is more significant at high redshift (z is approximately 3-4) because the mean free path for UV photons is smaller there, and the fluctuations correspondingly larger. This effect was studied using both the semi-analytic techniques of Zuo's recent papers and Monte Carlo simulations. The correlation function is expected to have a small yet potentially measurable amplitude that is consistent with current upper limits. Furthermore, the signature of this effect is distinctive because the nonzero correlation function extends over the photon mean free path, which is larger than the expected scale of large-scale structure. Observations or upper limits on this effect could provide information about the source of the ionizing background at high redshifts and the nature of the Ly-alpha forest clouds.

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