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arXiv · 1801.08187

From Heavy-Ion Collisions to Compact Stars: Equation of State and Relevance of the System Size

Sylvain Mogliacci·Isobel Kolbé·W. A. Horowitz
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Abstract

In this article, we start by presenting state-of-the-art methods allowing us to compute moments related to the globally conserved baryon number, by means of first principle resummed perturbative frameworks. We focus on such quantities for they convey important properties of the finite temperature and density equation of state, being particularly sensitive to changes in the degrees of freedom across the quark-hadron phase transition. We thus present various number susceptibilities along with the corresponding results as obtained by lattice quantum chromodynamics collaborations, and comment on their comparison. Next, omitting the importance of coupling corrections and considering a zero-density toy model for the sake of argument, we focus on corrections due to the small size of heavy-ion collision systems, by means of spatial compactifications. Briefly motivating the relevance of finite size effects in heavy-ion physics, in opposition to the compact star physics, we present a few preliminary thermodynamic results together with the speed of sound for certain finite size relativistic quantum systems at very high temperature.

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Sylvain Mogliacci, Isobel Kolbé, W. A. Horowitz. 2018-01-24. From Heavy-Ion Collisions to Compact Stars: Equation of State and Relevance of the System Size. https://doi.org/10.3390/universe4010014

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