Universality and emergent fluid from string breaking in the Schwinger model via tensor networks
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The Schwinger model is a useful theoretical laboratory for studying various problems in quantum field theory, especially as it incorporates confinement of charges. In this talk, I describe our recent work on analyzing the correlation between the energy, pressure and spatial quantum entanglement produced by two light-like jets in the massive Schwinger model. Using tensor network methods for real-time quantum evolution, we show that for m/g>1/pi, a nearly perfect and chargeless effective fluid behavior appears around the mid-rapidity region with a (non-thermal) universal energy-pressure relationship. The evolution of energy and pressure for this range of masses is strongly correlated with the rise of the spatial entanglement entropy, indicating a key role of quantum dynamics - in contrast to the behaviour for small masses.