Here's a brief (stretching the definition of "brief"), simple introduction to special relativity I typed up for something else a few months back. Might help some browsers of this forum.
Before 1905
The story began four centuries ago with Galileo Galilei. Galilean relativity said that the basic laws of physics are the same in all inertial reference frames (
an inertial reference frame is one in which there’s no acceleration—there’s no change in speed or direction); this is called the relativity principle. Galileo’s thought experiment involved a sailor dropping a knife from the top of the mast of a moving ship. Someone in the water watching as the ship goes by would see the falling knife follow a curved path because, while gravity is pulling it downwards, it also has a horizontal (forward) velocity—that of the ship. The sailor (and anyone on the ship), however, sees the knife fall from the top of the mast to the bottom; it’s as if the ship were sitting still (they all, like the knife, share the ship’s forward velocity so they don’t notice it).
So the laws of physics appeared to work exactly the same in every inertial reference frame (whether "moving" or "stationary"); playing ping pong in your basement is no different than playing on an airplane that isn’t accelerating. These early forms of relativity assumed that the lengths of objects and the rate at which time passes were the same in all inertial reference frames as well.
Then in the late nineteenth century electricity and magnetism were unified and described by Maxwell’s famous equations which revealed that light itself is nothing but an electromagnetic wave. The equations predicted that light would move at a certain speed, c, or about 3.00 x 10^8 m/s. But in which reference frame did light move at precisely this speed?
*Surely if one moved toward a light source at half the speed of light he would measure the speed of light to be 3/2 c (the regular speed of light plus his own speed) and if he moved away from a light source at ½ c he would measure the speed of light to be only ½ c (the regular speed of light minus his own speed). So it was thought that there must be some special reference frame in which one measures the speed of light to be exactly the one predicted by theory. It was also believed that since light is a wave it must propagate through some medium (like water waves through water or a wave on a string)—they called this the ether. The speed of light predicted by Maxwell was thought to be with respect to this ether.
*
Sadly this didn’t satisfy the relativity principle. Maxwell’s equations were different in different inertial frames. The laws of electricity and magnetism seemed to change with the reference frame. There was a state of absolute rest, a special inertial frame: that of the ether. An experiment to measure the earth’s speed relative to this ether was cooked up by Albert Michelson (the first American to win the Nobel Prize in Physics and inventor of the Michelson interferometer, still widely used today—in gravity wave detectors, for example) of Cleveland’s Case School of Applied Science and Edwin Morley of Cleveland’s Western Reserve University (the two merged in 1967 to form Case Western Reserve University). They essentially measured the speed of light in two perpendicular directions; it makes sense that if such an ether exists the measured speed of light would depend on the direction it traveled. The result was puzzling—the light seemed to travel at the same speed in both directions.
Enter Einstein
In 1905 a lowly patent clerk (but one well-trained in physics—crackpots not trained in physics often gloss over that point in their bid for martyrdom) suggested that the principle of relativity
does hold for electromagnetism. He advanced the theory today known as the special theory of relativity. And it was a doozy. Let’s take a look at it.
The theory is based on two postulates. The first is the familiar principle of relativity: the laws of physics are the same in all inertial reference frames. The second concerns the constancy of the speed of light: it says that light moves through empty space at a speed, c, that’s independent of the speed of the source or the observer.
That second postulate is often difficult for people to swallow. It says that no matter how fast you’re going, no matter if you’re heading toward or away from a light source, you’ll always measure the same value for the speed of light. Drive at 99.999999% of the speed of light and turn on the headlights--you still measure the light to race away from you at the standard speed of light. So the ideas above between the red asterisks are incorrect. Those were commonsense, intuitive notions; but the universe doesn’t work that way.
It’s important to realize that motion and speed are relative—those words only mean something when speaking of some reference point. It turns out there is no state of absolute rest, no ether. When you’re going "35 miles per hour" in your car that’s relative to the ground. Relative to the guy behind you who’s doing 30mph you’re only going 5 mph. So out in deep space what does it mean when Captain Picard gives the order for all stop? I imagine they have some reference point when they say that (or bad writers). But it’s important to understand that below when I say something like "he’s moving at 99% of the speed of light" that only means
relative to some other observer (this (and any) mover can consider himself to be at rest--this helps in understanding why everyone measures the speed of light to have the same value).
The consequences
Now I’m going to tell you some things without really showing how or why they come about (though I’ll try when it's possible). That will keep this simple without messy derivations and the harder parts of the theory getting in the way.
Three of the most basic mechanical quantities are affected by this: time, length, and mass. However, the effect only becomes noticeable at relativistic (meaning close to the speed of light) speeds, which is why nobody hit on this theory until the beginning of the 20th century.
Time dilation
It turns out that at speeds close to the speed of light (once again this is relative to someone else) time itself slows down. This means that if you stayed here on the earth and I sped off at 75% of the speed of light you would (assuming you had an amazingly powerful telescope to peer into my spacecraft and see my clocks) observe my clocks as taking longer to tick off one second than your own. This means that I would age more slowly than you and all that good stuff. But remember, this is
relativity. Since I’m moving in an inertial reference frame I could easily say that
I’m at rest and that you're the one moving away from me at 75% of the speed of light. Each observer sees the other’s clock as running slowly. Very symmetric.
A more mathematical look (and the simple explanation as to how it follows from special relativity) isn't too tough to produce or follow but it's a little peripheral to this first post.
Length contraction
It turns out that length contracts when you’re moving very fast (along the direction of motion). So when I buzz you (who is "stationary") going 75% of c you’ll measure my spacecraft to be shorter than I would measure it to be. But it isn’t just the length of the craft that shrinks but distance itself. An example using what we learned above about time dilation will help (after these visuals stolen from
here).
Spaceship Moving at the 10 % the Speed of Light
Spaceship Moving at the 86.5 % the Speed of Light
Spaceship Moving at the 99 % the Speed of Light
Spaceship Moving at the 99.99 % the Speed of Light
The third closest star to the sun is called Wolf 359 (Trek fans will recognize the name as the site of the first battle between Starfleet and the Borg in which Starfleet had its balls handed to it) and it’s 7.8 light years away. That means that at the speed of light it would take 7.8 years to get there. Moving at 90% of the speed of light it should take about 8.7 years to get there. Makes sense, doesn’t it? But wait: 8.7 years as measured by observers back on earth is much longer than what our relativistic astronaut will measure (time slows down for him). After 2 years and 4 months pass for the people back on earth, the astronaut will just be reaching the one year mark on his calendar. So when 8.7 years have passed for the people of earth and they know their astronaut must surely have reached Wolf 359 he’ll have experienced not quite 3 years and 10 months. So what can explain the fact that he completed what should have been an 8.7 year trip in less than half the time?
The distance to Wolf 359 must have contracted from the astronaut’s point of view. That explains how he could travel so far in such a short time—the distance itself shrank.
Again, the situation is symmetric. The people "at rest" on earth see the spacecraft shrink with respect to the distance (which they see as unchanged), whereas the astronaut sees his spacecraft’s length as unchanged but the distance to Wolf 359 is contracted (by the same factor as the people on earth see the length of his spacecraft contracted). Neither side is "wrong."
Mass
This is a tricky one. You could say that when moving at speeds close to c (again, as viewed by someone "at rest") an object’s mass increases. Mass is essentially a measure of how difficult it is to accelerate an object; so if objects become more massive the closer they get to the speed of light then it becomes more and more difficult to accelerate them further. Which is why c is the ultimate speed limit and nothing with mass could ever reach it.
Now if you were to go deeper into special relativity you would discover that this concept is not often used anymore (though it’s a good way for those new to the theory to visualize the "c as a cosmic speed limit" concept). Energy and momentum are the quantities that are really considered here. Einstein himself said:
Quote:
It is not good to introduce the concept of the mass of a moving body for which no clear definition can be given. It is better to introduce no other mass concept than the "rest mass" m. Instead of introducing M [the "relativistic mass" that’s dependent on velocity] it is better to mention the expression for the momentum and energy of a body in motion.
So that’s that.
You may be wondering where these come from or, alternatively, you may have heard of something called the "Lorentz transformation equations." We’ve been talking about how different observers see different things and yet neither is incorrect; suppose we have two observers, each defining his own coordinate system. The Lorentz transformations are how one would convert from one coordinate system to the other. It is in this conversion that we discover the above consequences of the theory (for example, that time is measured differently by the two observers in the different coordinate systems); they are the connection between those consequences and the original two postulates of the theory we mentioned above. But we’re avoiding the math here which means we must avoid the transformations themselves.
Two more important consequences
There are two more extremely important consequences of the theory that came later (i.e. were not a part of the original paper). One is directly attributable to Einstein, the other is not.
E=mc^2
Perhaps the most famous equation in physics. It gives the speed of light squared as the conversion factor between mass and energy. It shows that mass can be converted into energy (as in when matter and antimatter annihilate leaving behind only photons) and vice versa (as in pair production—high energy photons "split" into a matter-antimatter pair). Very important to nuclear physics as well.
The actual equation for relativistic energy is: E^2 = p^2 c^2 + m^2 c^4. When an object is considered to be at rest (i.e. when you’re in the same inertial reference frame as it is) then the velocity is zero and the momentum, p (m*v) is 0. It then reduces to the familiar equation.
Spacetime
This one isn’t Einstein’s. A former professor of his named Minkowski is the one who unified space and time. This can help you visualize why time slows down (as seen by others) for you as you approach the speed of light—the more you move through space, the less you move through time. A bit crude but it's helpful. This also ensures that units of distance can function as units of time and vice versa. For example, a second can be used as a unit of distance—that which a beam of light traverses in one second (about 3.00 x 10^8 meters as we said above). This idea is behind the notion of time as the fourth dimension: it’s simply a component of 4-dimensional spacetime.
The light cone
The light cone represents the points in spacetime which information about an event can reach, taking into account the c speed limit (it's impossible graph all the spatial axes along with time so they always drop a few). Anything outside the cone is inaccessible. The cones are formed by beams of light; they’re at a 45° angle to show that light travels through just as much space as it does time (it’s said to be
lightlike). Events that are separated such that some material object could travel between them are said to be
timelike.
Spacelike events are those that even light can’t connect.
Concluding thoughts
That's the bare bones of special relativity. I've left out some notable concepts like interval but I think this is enough to give anyone an idea of what's being talked about when special relativity is discussed. The lack of images couldn't really be helped, though I think the few I put in worked.
All of the predictions of special relativity have been thoroughly tested experimentally and the theory had to be taken into account for quantum mechanics to work correctly. Recently there have been suggestions that revisions (more like additions) should be made to the theory to take into account certain things.
Follow that?