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Measuring the equation of state of the high-z intergalactic medium using curvature statistics

, , and . (2015)cite arxiv:1502.05140Comment: 5 pages, 4 figures, 1 table.

Abstract

Using hydrodynamical simulations, we explore the use of the mean and percentiles of the curvature distribution function to recover the equation of state of the high-$z$ ($2 < z < 4$) intergalactic medium (IGM). We find that the mean and percentiles of the absolute curvature distribution exhibit tight correlation with the temperatures measured at respective characteristic overdensities $\Delta_i$'s at each redshift. Hence, they provide nearly independent probes of the same underlying temperature-density distribution, and can in principle be used to simultaneously recover both parameters $T_0$ and $\gamma$ of the IGM effective equation of state. We quantify the associated errors in the recovered parameters $T_0$ and $\gamma$ from the intrinsic scatter in the characteristic overdensities and the uncertainties in the curvature measurement.

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[1502.05140] Measuring the equation of state of the high-z intergalactic medium using curvature statistics

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