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CLM-ASTRO-003508= T_H = hbar c^3/(8 pi G M k_B)EXACT VALUEThe cited theorem establishes T_H = hbar c^3/(8 pi G M k_B) under the recorded model.Source: Particle Creation by Black Holes — Hawking black-hole temperature ↗
PROVENSemiclassical temperature of an uncharged nonrotating black hole.
The question, scope, and sources behind this Registry record.
Compute the asymptotic thermal spectrum of quantum fields on a stationary Schwarzschild background.
Current frontiers derived from accepted Claims.
The accepted equality closes this optimization result.
Assertions tied to evidence, attribution, and review.
The frontier as it changed over time.
Only accepted Claims matching the current specification contribute to the displayed bounds. Strict inequalities remain open; contradictory Claims require editorial review.