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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 3.

Radial profiles of AM transport for the fiducial model (ξTS = 1) at z = 0. From top to bottom, we show the angular frequency, the local net AM change due to radial transport (﹩{\rm{\Delta }}{{ \mathcal J }}_{R}﹩ in Equation (14)), and the effective shear viscosity associated with the Maxwell stress νeff. Curves of different colors correspond to snapshots between ﹩\bar{t}=15﹩ and 380 ms.

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