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1
What is a black hole?
2
Dimensional Analysis
3
Fundamental Constants
4
Building Equations
5
Physics of Black Holes
6
Area of event horizon
7
An important observation
8
Black Hole Entropy
9
Hawking Radiation
10
Black Hole Thermodynamics
11
Hawking Temperature
12
Time taken for a black hole to evaporate
13
Stefan Boltzmann Law
14
Evaporating Black holes
15
Primordial Black holes
16
A dramatic end
17
The information paradox
18
The holographic principle
Description:
Explore the fascinating world of black holes in this 41-minute video lecture. Delve into the physics behind these enigmatic cosmic objects, starting with their basic definition and progressing to advanced concepts like Hawking radiation and black hole thermodynamics. Learn how to derive Hawking's famous equation for black hole temperature using advanced high school mathematics. Discover the principles of dimensional analysis, fundamental constants, and how to build equations relevant to black hole physics. Investigate the area of the event horizon, black hole entropy, and the time it takes for a black hole to evaporate. Examine intriguing topics such as primordial black holes, the information paradox, and the holographic principle. Gain insights into the dramatic end of black holes and their significance in our understanding of the universe.

Deriving Hawking's Most Famous Equation - What Is the Temperature of a Black Hole?

Physics Explained
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