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Non-singular Gravitational Collapse Avoids Singularity, Rebounds, And Deviates From Hawking Radiation
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Non-singular Gravitational Collapse Avoids Singularity, Rebounds, And Deviates From Hawking Radiation
Research reveals that collapsing stars may not always form black holes with singularities, instead bouncing back from collapse and emitting particles in a way that deviates from predicted thermal radiation, potentially resolving problematic conditions within the collapse process
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