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Fig. 3

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Evolution of rotochemical heating in the ηnpe − T space for a superfluid star with the same parameters of Fig. 1. Upper panel: evolution with Δn = 0.05 MeV for different initial conditions (dotted-dashed lines) that converge to the same limit cycle (solid line). The quasi-steady state is indicated (star). Lower panel: evolution of the limit cycle for Δn = 0.04, 0.05, 0.06 MeV. The arrows indicate the path of the cycles A-B, B-C, and C-A for the star with Δn = 0.05 MeV.

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