Physical Properties of the Lyman Alpha Forest in a Cold Dark Matter Cosmology

Details Physical Properties of the Lyman Alpha Forest in a Cold Dark Matter Cosmology Physical Properties of the Lyman Alpha Forest in a Cold Dark Matter Cosmology

1997-06-10

arxiv.org/abs/astro-ph/9706087v1

Astrophys.J.465:63-79,1998

Astronomy and Astrophysics

Astrophysics

AAS LaTex, 35 pp, 19 figures (17 embedded), 2 GIF figures, and one GIF Plate. Accepted to ApJ. A complete .ps version is avail

Scientific paper

10.1086/305260

We discuss the origin and physical nature of the Lya forest absorption systems as found in hydrodynamical simulations of the Intergalactic Medium in a standard Cold Dark Matter cosmology (Omega=1, H0=50 km/s/Mpc, sigma_8=0.7). The structures of the systems that give rise to the Lya forest span a wide range in morphologies, depending on the density contrast. The absorption properties of the forest clouds correlate strongly with those of the underlying physical systems from which they arise. The highest column density systems (log N_HI > 15), correspond to highly overdense spheroidal structures, moderate column density systems (13 < log N_HI < 14), correspond to filaments, and the lowest density absorption systems originate from discrete fluctuations within underdense regions a few megaparsecs across, cosmic minivoids. Most of the intergalactic HeII opacity arises from these underdense regions. We are able to account for the distribution of optical depths in our synthesized spectra entirely by absorption due to discrete systems. We find that virtually all the baryons in the simulation fragment into structures that we can identify with discrete absorption lines, with at most 5% remaining in a smoothly distributed component (the Gunn-Peterson effect). We compare our results with the cloud ionization parameters inferred from Keck HIRES measurements of carbon and silicon in the Lya forest. Combining with constraints imposed by measurements of the mean intergalactic HI opacity, we find 0.03 < Omega_b < 0.08 and 0.3 < (Gamma_HI/ 10^-12 s^-1) < 1 at z=3-3.5.

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