Fig. 2.

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Evolution of the reference model. The stellar rotation period and radius are shown in panels a and b, respectively. The different torque contributions are shown in panel c. The accretion torque Γacc, the influence of the magnetic star-disk interaction ΓME, the APSW torque ΓW, and the internal contributions due to variation of the stellar moment of inertia Γint are shown as a solid blue line, dashed blue line, dotted blue line, and dash-dotted blue line, respectively. The total torque Γtot, defined as the sum of the other torque contributions, is shown as a solid black line. A gray dashed line marks the change between the spin-up and spin-down regimes.
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