The hydrodynamic response of small-scale structure to reionization drives large IGM temperature fluctuations that persist to z = 4
Christopher Cain, Evan Scannapieco, Matthew McQuinn, Anson D'Aloisio,, Hy Trac

TL;DR
This study uses high-resolution simulations to show that small-scale hydrodynamic responses to reionization create persistent temperature fluctuations in the IGM, impacting Lyα forest observations at redshifts up to 4.
Contribution
The paper demonstrates that resolving small-scale structures is crucial for accurately modeling IGM temperature fluctuations caused by reionization, which previous lower-resolution simulations overlooked.
Findings
Small-scale temperature fluctuations persist until z ≤ 4.
High-resolution simulations reveal a 10% increase in Lyα flux power at certain scales.
Pre-heating by X-Rays slightly reduces temperature fluctuation effects.
Abstract
The thermal history and structure of the intergalactic medium (IGM) at is an important boundary condition for reionization, and a key input for studies using the Ly forest to constrain the masses of alternative dark matter candidates. Most such inferences rely on simulations that lack the spatial resolution to fully resolve the hydrodynamic response of IGM filaments and minihalos to HI reionization heating. In this letter, we use high-resolution hydrodynamic+radiative transfer simulations to study how these affect the IGM thermal structure. We find that the adiabatic heating and cooling driven by the expansion of initially cold gas filaments and minihalos sources significant small-scale temperature fluctuations. These likely persist in much of the IGM until . Capturing this effect requires resolving the clumping scale of cold, pre-ionized gas, demanding…
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Taxonomy
TopicsOcean Waves and Remote Sensing · Lattice Boltzmann Simulation Studies
