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Which consequence results when stellar mass exceeds the Tolman-Oppenheimer-Volkoff limit?

A)Uncontrollable spacetime curvature accelerates collapse
B)Neutron degeneracy pressure arrests collapse
C)Thermonuclear ignition halts accretion
D)Gravitational waves disperse stellar material

💡 Explanation

Uncontrollable spacetime curvature accelerates collapse because gravity overwhelms all opposing forces when the Tolman-Oppenheimer-Volkoff limit is reached given the mass. This produces runaway curvature with black hole formation, rather than stabilization, therefore B, C, and E are incorrect.

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