Black Holes and Entropy.¶
Bekenstein, J. D. (1973). Black Holes and Entropy. Physical Review D, 7(8), 2333-2346.
Cited by¶
1 citation across 1 artifact.
Each citation links to the sentence it supports in the citing article.
Primes¶
- Entropy (Thermodynamic Sense)
- In black-hole thermodynamics, Bekenstein-Hawking entropy S_BH = A/(4L_p²) — area proportionality proposed by Bekenstein
This sourceProposes that black-hole entropy is proportional to event-horizon area (S ∝ A), violating classical extensivity and motivating entropy bounds. (See flag: the exact coefficient S = A/(4L_p²) is Hawking 1975, not Bekenstein 1973, which gave only the proportionality.)
- In black-hole thermodynamics, Bekenstein-Hawking entropy S_BH = A/(4L_p²) — area proportionality proposed by Bekenstein
Verification¶
Does it exist? Confirmed. This work's DOI resolves to a registered record, which fixes its identity. That is all it fixes.
Does it back the claim? Not recorded. The single citation of this work carries no recorded support check.
Support is checked per citation rather than per work — the same source can be cited soundly in one article and wrongly in another. Per-citation recording began recently, so a citation with no recorded check is a gap in the record rather than evidence it went unchecked.
See how references were verified.
Registry ID ref:bcb7deddc9ff · see in the full table