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Angular Momentum Transport in the Convection Zone of a 3D MHD Simulation of a Rapidly Rotating Core-collapse Progenitor

  • Authors: Ryota Shimada, Lucy O. McNeill, Vishnu Varma, Keiichi Maeda, Takaaki Yokoyama, Bernhard Müller

Ryota Shimada et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 3.

The horizontal axis shows the inverse of the Rossby number, and the vertical axis shows the ratio between the magnetic and kinetic energy. The color of each point indicates the corresponding time in the simulation that satisfies the quasi-steady state condition, as shown by the rainbow colorbar (t = 300–480 s; Equation (10)). The black solid line represents the best fit to the quantities taken from the 3D MHD simulation.

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