Gravitational Radiation from Nonaxisymmetric Spherical Couette Flow in a Neutron Star


The gravitational-wave signal generated by global, nonaxisymmetric shear flows in a neutron star is calculated numerically by integrating the incompressible Navier-Stokes equation in a spherical, differentially rotating shell. At Reynolds numbers Re 3#10 the laminar Stokes flow is unstable, and helical, oscillating Taylor-Görtler vortices develop. The… (More)


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