Episode #428
Sean Carroll: General Relativity, Quantum Mechanics, Black Holes & Aliens
Sean Carroll is a theoretical physicist, author, and host of Mindscape podcast.
What this episode covers
Sean Carroll is a theoretical physicist, author, and host of Mindscape podcast.
Where to start
Introduction
The whole point of relativity is to say there's no such thing as right now when you're far away. That is doubly true for what's inside a black hole. You might think, "Well, the galaxy is very big." It's really not. It's some tens of thousands of light years across and billions of years old. You don't need to move at a high fraction of the speed of light to fill the galaxy. The number of worlds is ...
Start at 0:00
General relativity
In book one of the series, The Biggest Ideas in the Universe called Space, Time, Motion, you take on classical mechanics, general relativity by taking on the main equation of general relativity and making it accessibly easy to understand. Maybe at the high level, what is general relativity? What's a good way to start to try to explain it? Probably the best way to start to try to explain it is special relativity, which came first, 1905. It was the culmination of many decades of people putting things together. But it was Einstein in 1905. In fact, it wasn't even Einstein. I should give more credit to Minkowski in 1907. Einstein in 1905 figured out that you could get rid of the ether, the idea of a rest frame for the universe and all the equations of physics would make sense with the speed of light being a maximum.
Start at 1:54
Black holes
I think a nice way to test the difference between objective reality and the observed reality is what happens at the edge of the horizon of a black hole. Technically, as you get closer to that horizon, time stands still? Yes and no. It depends on exactly how careful we are being. Here is a bunch of things I think are correct. If you imagine there is a black hole, spacetime, the whole solution Einstein's equation, and you treat you and me as what we call test particles. We don't have any gravitational fields ourselves. We just move around in the gravitational field. That's obviously an approximation. Okay. But let's imagine that.
Start at 14:13
People and topics
Key takeaways
- Introduction
- General relativity
- Black holes
- Hawking radiation