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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Significant X-ray flux blocking in 4U 1746-37 allows the neutron star to have canonical mass and radius values of 1.59 solar masses and 13 km or 2.12 solar masses and 9.8 km.
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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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The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius
Significant X-ray flux blocking in 4U 1746-37 allows the neutron star to have canonical mass and radius values of 1.59 solar masses and 13 km or 2.12 solar masses and 9.8 km.