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Spinning Down Neutron-star Merger Remnants with the Tayler–Spruit Dynamo: Global Simulations Reveal the Formation of Massive Disks and Neutron-rich Ejecta

  • Authors: Harry Ho-Yin Ng, Elias R. Most

Harry Ho-Yin Ng and Elias R. Most 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 4.

Shear viscosity for the TS dynamo at two different postmerger times, ﹩\bar{t}﹩. Shown are the (left) effective viscosity computed from the simulation with ξTS = 1, νeff, and (right) analytic prescription used in stellar evolution, νFPJ (J. Fuller et al. 2019). Here, ρ is the baryon rest-mass density.

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