We develop a method to extract the "effective equation of state" of the intergalactic medium from the doppler b parameter distribution of the low-density Lyman-alpha forest. We test the method on numerical simulations and then apply it to published observations of the Lyman-alpha forest at redshifts z from 0 to 4. We find that the effective equation of state is close to isothermal at redshift z=3, indicating that a second reheating of the IGM took place at z=3. This reheating can plausibly be identified with the reionization of HeII observed to occur at z about 3.
@article{arxiv.astro-ph/9906413,
title = {The Evolution of the Effective Equation of State of the IGM},
author = {Massimo Ricotti and Nickolay Y. Gnedin and J. Michael Shull},
journal= {arXiv preprint arXiv:astro-ph/9906413},
year = {2009}
}
Comments
Revised version accepted for publication in ApJ. Vol. 534 May 1, 2000 (in press); 32 pages, 13 figures, 7 tables