SPH simulations demonstrate viscosity-driven transitions forming NBOL, RAKED, and CENBOL boundary layers in sub-Keplerian flows onto neutron stars, extending TCAF concepts.
arXiv e-prints, arXiv:1905.01538
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Timing Properties of Shocked Accretion Flows around Neutron Stars -- II. Viscous Disks and Boundary Layers
SPH simulations demonstrate viscosity-driven transitions forming NBOL, RAKED, and CENBOL boundary layers in sub-Keplerian flows onto neutron stars, extending TCAF concepts.