Главная
Study mode:
on
1
Einstein’s most important equation
2
Why Newton’s equations are so important
3
The two kinds of relativity
4
Why is it the geometry of spacetime that matters?
5
The principle of equivalence
6
Types of non-Euclidean geometry
7
The Metric Tensor and equations
8
Interstellar and time and space twisting
9
The Riemann tensor
10
A physical theory of gravity
11
How to solve Einstein’s equation
12
Using the equation to make predictions
13
How its been used to find black holes
Description:
Explore Einstein's lesser-known but most significant equation in this 54-minute lecture by Sean Carroll at The Royal Institution. Delve into the complexities of general relativity, understanding how spacetime curvature relates to mass and energy distribution. Learn about Newton's equations, the two types of relativity, and the importance of spacetime geometry. Discover the principle of equivalence, non-Euclidean geometry, and key concepts like the Metric Tensor and Riemann tensor. Examine how Einstein's equation forms a physical theory of gravity, its solutions, and practical applications in predicting phenomena and detecting black holes. Gain insights into the twisting of time and space as depicted in the film Interstellar, and unravel the mysteries of the universe through this comprehensive exploration of Einstein's groundbreaking work.

The Secrets of Einstein's Unknown Equation - Spacetime Curvature and General Relativity

The Royal Institution
Add to list