Thermal quenches into chiral superfluid ³He-A excite Higgs and clapping modes whose PSD and Kibble-Zurek exponents depend on Langevin damping, with z crossing smoothly from 1 to 2 while ν stays near 1/2.
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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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Excitation of Collective Modes in a Chiral Superfluid by Thermal Quench
Thermal quenches into chiral superfluid ³He-A excite Higgs and clapping modes whose PSD and Kibble-Zurek exponents depend on Langevin damping, with z crossing smoothly from 1 to 2 while ν stays near 1/2.
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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.