How to pronounce “time dilation” in English

And you get the time dilation equation, just as Einstein derived it in 1905.

And so more time dilation than here at the surface of the Earth.

How much time dilation, in principle, could we get?

This idea of time dilation seems like just a thought experiment or some notion that Einstein's come up with surely doesn't happen in the real world.

We call it 'time dilation.'

The point is that encapsulates time dilation, because time is nothing more than how many times

of self, time dilation.

One aspect of that curvature connecting to the time dilation is curvature produces time dilation regardless of relative motion.

There, time dilation goes to infinity.

So you started with an explanation of how time dilation, it depends more on acceleration than actual velocity of the observer, but then when you got into the Pythagorean theorem

this is what leads to the idea of time dilation.

Because of time dilation, I managed to have less time elapse.

So Steve introduced one aspect of special relativity, time dilation.

This notion of time dilation is part of Einstein's special theory of relativity.

And as we were talking about, it doesn't take an infinite time, even though there's time dilation.

So that's what leads to all of these puzzles and paradoxes about length contraction and time dilation and all those other things.

So I'm going to explain one aspect that we would describe black holes from the perspective of time dilation.

OK, so we're going to use this idea that curvature introduces time dilation to get to black holes.

So the curvature becomes very, very large and the time dilation can become an arbitrarily large factor.

So you told us that close to the event horizon, the time dilation, time runs slower compared

And to have that, you need a four-dimensional space-time structure that related, basically, length contraction and time dilation

So in special relativity, when we were moving relative to each other, that we perceive time dilation.

And so now if we get closer to that higher curvature region, there's going to be more time dilation.

So if it goes near the surface of the white dwarf, there's going to be quite a lot of time dilation, a lot of curvature.

Now, for neutron stars, the curvature is so strong near the surface that the time dilation becomes significant.

So now you can explain-- Yeah, let me use a couple of my simple demos to reinforce what Frans is saying out time dilation.

So along with what's called time dilation, the slowing down