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CLM-ASTRO-003509= t_evap = 5120 pi G^2 M^3/(hbar c^4)EXACT VALUEThe cited theorem establishes t_evap = 5120 pi G^2 M^3/(hbar c^4) under the recorded model.Source: Black hole explosions? — Ideal Schwarzschild black-hole evaporation lifetime ↗
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