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A Unification of the Micro and Macro Physics in the Intracluster Medium of Nearby Clusters

Published onMay 31, 2019
A Unification of the Micro and Macro Physics in the Intracluster Medium of Nearby Clusters
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Abstract

The vast bulk of the hot baryons in the Universe is in the form of the intracluster medium. All major cosmological simulations assume the astrophysical plasma to be inviscid. It is critical to constrain the effective transport coefficient of the intracluster medium to truly understand the baryonic processes in the Universe.

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