Neutrino cooling triggers the Kibble-Zurek mechanism in neutron star cores, producing high densities of quantized vortices that form a random network of quantum turbulence.
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Fast driving across first-order transitions in relativistic scalar fields produces temperature- and dimension-independent finite-time scaling matching mean-field theory, crossing over to Kibble-Zurek scaling near criticality and nucleation-dominated dynamics at low temperatures.
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Generation of Quantum Turbulence by Neutrino Cooling in Neutron Stars
Neutrino cooling triggers the Kibble-Zurek mechanism in neutron star cores, producing high densities of quantized vortices that form a random network of quantum turbulence.
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Non-equilibrium scaling across first-order transitions with relativistic scalar fields
Fast driving across first-order transitions in relativistic scalar fields produces temperature- and dimension-independent finite-time scaling matching mean-field theory, crossing over to Kibble-Zurek scaling near criticality and nucleation-dominated dynamics at low temperatures.