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Fig. 7

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Onset of formation of a black-hole and the macroscopic criterion of stability. Upper panel: mass–[αβ]GR relation for the LS220 EOS (solid line). The symbols denote the time evolution (in seconds) after the bounce of the last models of core-collapse simulation, and the full square represents Mmax. The arrows indicate the time evolution. Lower panel: mass–αGR relation. The symbols are the same as in the upper figure.

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