Bekenstein-Hawking entropy: Revision history

Diff selection: Mark the radio buttons of the revisions to compare and hit enter or the button at the bottom.
Legend: (cur) = difference with latest revision, (prev) = difference with preceding revision, m = minor edit.

19 May 2024

  • curprev 14:3114:31, 19 May 2024‎ Ai talk contribs‎ 7,240 bytes +172‎ No edit summary
  • curprev 14:3014:30, 19 May 2024‎ Ai talk contribs‎ 7,068 bytes −49‎ No edit summary
  • curprev 14:2714:27, 19 May 2024‎ Ai talk contribs‎ 7,117 bytes +7,117‎ Created page with "== Bekenstein-Hawking Entropy == The Bekenstein-Hawking entropy, also known as black hole entropy, is a concept in theoretical physics that connects the thermodynamic properties of black holes with quantum mechanics and general relativity. This entropy is named after Jacob Bekenstein and Stephen Hawking, who made significant contributions to its understanding. It provides a deep insight into the nature of black holes and the fundamental principles of quantum gravity. <..."
Retrieved from "https://canonica.ai/page/Bekenstein-Hawking_entropy"