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Talk1 h 13 min

How hot glue becomes a nearly perfect fluid: the problem of thermalization in ultra-relativistic heavy ion collisions

Raju Venugopalan · CERN

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About

The hottest matter on earth is created when gluons (with a sprinkling of quark-antiquark pairs) are liberated in the collisions of ultra-relativistic heavy ions at the RHIC and LHC colliders. A fully *ab initio* understanding of how this strongly correlated gluon matter thermalizes and flows is lacking. We review progress towards solving this problem and discuss surprising recent numerical results-in particular the discovery of a universal non-thermal fixed point (typical of weak wave turbulence) in an expanding non-Abelian plasma. Remarkably, the self-similar behavior of this fluid is identical to those of over-occupied N component self-interacting scalar theories that model, for instance, the behavior of cold atomic gases. We discuss possible insights into the hottest fluids produced on earth obtained from the coldest fluids--in particular, the possible formation of transient Bose-Einstein condensates. We also discuss another recent development: a computation of the off-equilibrium sphaleron transition rate in the over occupied plasma, and its implications. Our discussion will be grounded in the empirical constraints from the heavy-ion experiments. As an example, time permitting, we will outline how rare high multiplicity proton-nucleus collisions further test the "unreasonable effectiveness of hydrodynamics" as a description of the tiny and ephemeral droplets of quark-gluon matter created at RHIC and the LHC..

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The talk

  1. How hot glue becomes a nearly perfect fluid: the problem of thermalization in ultra-relativistic heavy ion collisions 2016-03-02 · 1 h 13 min · CERN's player

Credits and licence

Institution
CERN
Department
TH Theoretical Seminar
Speaker
Raju Venugopalan
Year
2016
Language
English
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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