An introduction to modern astronomy's most important questions. The four sections of the course are Planets and Life in The Universe; The Life of Stars; Galaxies and Their Environments; The History of The Universe.
Special Relativity
Loading...
Del curso dictado por University of Rochester
Confronting The Big Questions: Highlights of Modern Astronomy
255 calificaciones
University of Rochester
255 calificaciones
De la lección
How do Stars Evolve and Die?
The Life of Stars - Star formation, fusion and stellar middle age, black holes and stellar death-
Conoce a los instructores
Adam FrankProfessor
Physics and Astronomy
So when Einstein thought about physics and what happens on
moving platforms like a [UNKNOWN] rocket ship versus stationary platforms.
He was able, because of his genius, to see something that no one else saw before.
That these usual rules that we expect from moving, not very
close to the speed of light have fooled us in some sense.
And what Einstein really what he was really bothered by
was he tried to imagine what it would be like to ride a light beam.
You know we've, we've already seen light is a a, a
wave of electric magnetic energy moving with the speed of light.
And what he understood was, or what he found was there was a paradox.
There was a paradox as he tried to imagine what it would be
like to look at a light from a, from someone, standing on the ground.
And watching light going by, or if you could ride the light wave.
And it was, that is what
led him to really change his and our understanding about the
way space and time are coupled together, how they work together.
In order to do this Einstein had to change physics
such that he invented or came up with two new postulates.
And out these postulates he was going to build an entirely different physics.
So let's look at these postulates.
The first one is that the laws of physics
are the same in all, what are called inertial frames
of reference.
So, these are frames of reference with no accelerations occurring on them.
So your rocket motor can't be on.
You have to just be cruising through space, you know, the motor's turned off.
You can't be orbiting either because in an orbiting frame of reference.
You still are accelerating because, you're, you're orbiting.
So what Einstein said was that, in these inertial
frames, all the physics has to be the same.
You shouldn't be able to tell the difference
from one inertial frame to the other.
Any laws of physics you have should be the same.
Every observer, basically, can argue that he or she is
at rest while all the other observers are in motion.
So what this means is when you're driving in a car and the windows are blackened.
You shouldn't be able to do any experiment
that tells whether or not you're the one moving.
Or whether it's the, the ground around you which is moving past you.
The second one is particularly radical, which is that the
speed of light should be the same for all observers.
So no matter what you're doing, no
matter how you're moving relative to everybody else.
Your measurement of the speed of light should be the
same as everybody else's measurement of the speed of light.
And to understand why that's so radical, we have
to go back to our example of adding velocities.
Right?
Remember we saw that the with the pellet gun.
That the person standing on the ground as
the rocket ship goes by measures the velocity to be the speed of the rocket
plus the speed of the pellet as it leaves the muzzle of the gun, right.
But what Einstein said is that if that was a laser beam
rather than a pellet gun then everybody measure the same speed of light.
That, the, if I shoot the laser on the rocket with the windows
blackened, I will see the laser beam move away from me at the
speed of light, which we call C.
But the person on the ground will have to measure the exact same speed.
There can be no indication that, there are no
addition of velocities with, when it comes to light.
Such that you have to add mind motion relative to
the person on the ground plus the speed of light.
And what that does is it changes physics dramatically.
And in order to get the speed of light to be the same for
everybody observing it, you have to allow space
and time to be able to become distorted.
They can become they are no longer absolute
each in their own category in some sense.
Because any measurement of speed is always a measurement of how
far something has gone, over some duration, over some amount of time.
And if you need the speed of light to
always be the same, no matter who is measuring it.
It means
you have to allow space and time
to contract or expand for each individual observer.
In order to keep the speed of light, keep that measurement the same.
And that is really the remarkable
conclusion of what we call special relativity.
This was Einstein's first step into relativity.
That space and time are not absolute, in that they
have to be joined together in something we call space/time.
And that each person's
measurements of space, or measurements of time will be
different depending on how they're moving relative to everyone else.
So for me, a second or a, a meter will be different than for you.
What you measure to be a second or a meter.
Depending on how we're moving relative to each other.
So space and time individually become flexible, they become malleable And
what doesn't change is this overall thing we now call space-time.
So the change
in time, the flow of time from one frame of
reference to another is often called, referred to as time dilation.
And the video that accompanies this lecture gives you nice
example of the mechanics of time dilation, how The time, the
flow of time in one frame of reference will be
different from the flow of time in another frame of reference.
But perhaps the best way anecdotally, so to
speak, to talk about the effects of time dilation,
is to discuss what's called the twin paradox.
And this can be proven, you know, very explicitly using the mathematics
of special relativity, which turns out to be actually not very complicated.
But basically the idea is if you have twins who are
born on Earth and, you know, of course they're aging together.
And then when they're both 20 one of the twins gets
into a spaceship and decides to fly off to a faraway planet.
In a spaceship that is moving very close to the speed
of light.
Because none of these relativistic effects, show up unless
your moving very close to the speed of light.
What will happen is, is as the twin is flying to the the
other planet, and then flying back, very close to the speed of light.
Time for that twin will move more slowly, meaning, literally, the
number of heartbeats that they have experienced, the ticking of their clocks.
that, their time will flow more slowly relative
to the twin on Earth.
So when the twin lands, it will be
perhaps three years that they will have experienced on
the spaceship, whereas the twin who stayed home
Will now be, will be 30 years for them.
So the, the, the twin will get out of the space ship
to greet their, their sibling and suddenly they see an old person.
It'll be very shocking for them if they didn't know about time dilation.
And this is the most dramatic example of how space and time
have to distort The, for the twin
on the spaceship, they didn't notice any difference.
Time flowed for them just the way it always does.
But it's only when they meet up with someone who wasn't traveling.
Who was not in their frame of reference that this
effect of time moving at a different speed becomes apparent.
So really, what we learned from special relativity is
that space and time alone are no longer absolute.
That each can grow or shrink depending
on how, people are moving relative to each other.
And we know have to think about this new quantity called space time.
Which is the most, which is really what is absolute.
Which is really the ground of physical reality.
So, with that, now we're able to take the next step
forward in our understanding and begin to talk about General relativity.
And general relativity is where Einstein went beyond just
inertial frames and began to consider accelerations as well.
[BLANK_AUDIO]
Explora nuestro catálogo
Inscríbete de manera gratuita y obtén recomendaciones personalizadas, actualizaciones y ofertas.
Coursera brinda acceso universal a la mejor educación del mundo, al asociarse con las mejores universidades y organizaciones, para ofrecer cursos en línea.
© 2018 Coursera Inc. Todos los derechos reservados.
