Cosmological and astrophysical constraints from the Lyman-alpha forest flux probability distribution function

TL;DR

This study uses the Lyman-alpha forest flux PDF and hydrodynamical simulations to constrain cosmological parameters and the IGM's thermal state at redshifts 2-3, finding results consistent with WMAP but with larger uncertainties.

Contribution

It provides new constraints on cosmological parameters and the IGM thermal state using flux PDF data, and explores the impact of combining flux PDF with SDSS power spectrum data.

Findings

Flux PDF constraints align with WMAP data but with larger errors.

Inverted IGM temperature-density relation (gamma ~ 0.5-0.75) is favored.

Joint analysis suggests higher sigma_8 and IGM temperatures, indicating potential systematic errors or incomplete models.

Abstract

We use the probability distribution function (PDF) of the lya forest flux at z=2-3, measured from high-resolution UVES/VLT data, and hydrodynamical simulations to obtain constraints on cosmological parameters and the thermal state of the intergalactic medium (IGM) at z 2-3. The observed flux PDF at z=3 alone results in constraints on cosmological parameters in good agreement with those obtained from the WMAP data, albeit with about a factor two larger errors. The observed flux PDF is best fit with simulations with a matter fluctuation amplitude of sigma_8=0.8-0.85 \pm 0.07 and an inverted IGM temperature-density relation (gamma ~ 0.5-0.75), consistent with our previous results obtained using a simpler analysis. These results appear to be robust to uncertainties in the quasar (QSO) continuum placement. We further discuss constraints obtained by a combined analysis of the high-resolution flux PDF and the power spectrum measured from the Sloan Digital Sky Survey (SDSS) lya forest data. The joint analysis confirms the suggestion of an inverted temperature-density relation, but prefers somewhat higher values (sigma_8 ~ 0.9) of the matter fluctuation amplitude than the WMAP data and the best fit to the flux PDF alone. The joint analysis of the flux PDF and power spectrum (as well as an analysis of the power spectrum data alone) prefers rather large values for the temperature of the IGM, perhaps suggesting that we have identified a not yet accounted for systematic error in the SDSS flux power spectrum data or that the standard model describing the thermal state of the IGM at z ~ 2-3 is incomplete.