Rapid neutrino cooling through the neutron superfluid transition in neutron stars creates a dense Kibble-Zurek vortex tangle — quantum turbulence — with densities far above the rotational vortex density.
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3 Pith papers cite this work, alongside 36 external citations. Polarity classification is still indexing.
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TDGL quench simulations of chiral 3He films reproduce Kibble-Zurek vortex scaling and reveal a post-freeze-out population asymmetry between triangular and crescent vortex cores.
citing papers explorer
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Generation of Quantum Turbulence by Neutrino Cooling in Neutron Stars
Rapid neutrino cooling through the neutron superfluid transition in neutron stars creates a dense Kibble-Zurek vortex tangle — quantum turbulence — with densities far above the rotational vortex density.
- Excitation of Collective Modes in a Chiral Superfluid by Thermal Quench