Generation of Quantum Turbulence by Neutrino Cooling in Neutron Stars
J. A. Sauls

TL;DR
This paper explores how neutrino cooling induces quantum turbulence in neutron star interiors through the Kibble-Zurek mechanism, predicting high vortex densities during superfluid formation.
Contribution
It applies the Kibble-Zurek mechanism to neutron star superfluidity, providing quantitative vortex density predictions based on cooling models and superfluid gap parameters.
Findings
High vortex densities predicted during superfluid transition in neutron stars.
Quantum turbulence characterized by a network of vortex lines and loops.
Vortex density depends on cooling mechanisms and superfluid gap models.
Abstract
The interior crust and much of the liquid core of neutron stars is believed to be a quantum liquid mixture of neutron and proton superfluids and a relativistic electron liquid. Quantized vortices in the neutron superfluid and quantized flux lines in the proton superconductor are topological defects of these hadronic condensates. I consider the formation of the superfluid state in young neutron stars under non-equilibrium conditions imposed by the neutrino cooling rate. The nonequilibrium phase transition implies that the onset of superfluidity is accompanied by the generation of quantized vortices based on the mechanism envisioned by Kibble in the context cosmic string formation in an evolutionary models of an expanding universe, and further developed by Zurek for nonequilibrium phase transitions in quantum liquids such as \Hefour. I discuss the Kibble-Zurek mechanism (KZM) and scaling…
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