Which outcome regarding spacetime geometry results when adding mass to a neutron star near the Tolman–Oppenheimer–Volkoff limit?

💡 Explanation

Gravitational collapse to a black hole results because exceeding this mass limit overcomes all internal pressure supports leading to gravitational singularity formation, via runaway "equivalence" effects. Therefore, collapse occurs rather than pressure increase, because gravity dominates under these conditions as mass increases.

• Which outcome arises due to star light bending around a blackhole?
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• Which outcome results during uranium enrichment at elevated temperatures?