About this document
Rindler Spacetime and Black Hole Geometry by Youssef Qanqache is a document available to read on EtoBox.
Lecture 3 of the Holographic Duality course discusses Rindler spacetime and the causal structure of black holes, focusing on the region near the horizon. It introduces the concept of proper distance from the horizon and explains the relationship between Rindler coordinates and Minkowski spacetime. Additionally, the lecture covers Penrose diagrams and the derivation of black hole temperature as perceived by stationary observers, highlighting the connection between black hole thermodynamics and quantum field
- Author
- Youssef Qanqache
- Language
- EN