1125 lines
66 KiB
Plaintext
1125 lines
66 KiB
Plaintext
Newsgroups: rec.arts.startrek.tech
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Path: bloom-beacon.mit.edu!gatech!purdue!mozo.cc.purdue.edu!news.physics.purdue.edu!bohr.physics.purdue.edu!hinson
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From: hinson@bohr.physics.purdue.edu (Jason W. Hinson)
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Subject: Relativity and FTL Travel
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Message-ID: <D3CKFI.17J@physics.purdue.edu>
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Sender: usenet@physics.purdue.edu (News Administration)
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Organization: Physics Department, Purdue University
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Date: Thu, 2 Feb 1995 00:38:06 GMT
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Lines: 1114
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NOTE: I HOPE this is the last time I'll be posting edition 3.1 of this
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post, however I make no promises. My spare time is scarce these days,
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and I am still working on getting edition 4.0 completed. It will
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include the following: a new sectioning method; an entirly new section
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(not manditory reading if you just want to understand the FTL
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arguments) which gives more information on special relativity,
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paradoxes, and even takes a look at general relativity; and a
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re-worked FTL discussion which will talk about the various ideas for
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how one could imagine FTL travel (like wormholes, "changing the speed
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of light", etc.). This re-worked FTL section will also show why I
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think the best method for explaining FTL travel as it is depicted on
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Trek is still, by far, the one given in the edition below.
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So, be looking for edition 4.0--if not in March then in April. Thanks
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for the patience, and if you'd like to be placed on a mailing list to
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receive 4.0 via e-mail when it is finished, just let me know.
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This is edition 3.1 of this post. Only slight corrections have been
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made since version 3.0. As planned, it has become a regular monthly
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post on the rec.arts.startrek.tech newsgroup. Again, let me know if
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you think that any changes should be made.
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What is it about, and who should read it:
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This is a detailed explanation about how relativity and that
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wonderful science fictional invention of faster than light travel do
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not seem to get along with each other. It begins with a simple
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introduction to the ideas of relativity. The next section includes
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some important information on space-time diagrams, so if you are not
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familiar with them, I suggest you read it. Then I get into the
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problems that relativity poses for faster than light travel. If you
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think that there are many ways for science fiction to get around these
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problems, then you may not understand the problem that I discuss in
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the forth section, and I strongly recommend that you read it to
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increase your understanding of the FTL problem. Finally, I introduce
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my idea (the only one I know of) that, if nothing else, gets around
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the second problem I discuss in an interesting way.
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The best way to read the article may be to make a hard copy. I
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refer a few times to a diagram in the second section, and to have it
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readily available would be helpful.
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I hope you can learn a little something from reading this, or
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at least strengthen your understanding of that which you already know.
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Your comments and criticisms are welcome, especially if they indicate
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improvements that I can make for future posts.
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And now, without further delay, here it is.
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Relativity and FTL Travel
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Outline:
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I. An Introduction to Special Relativity
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A. Reasoning for its existence
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B. Time dilation effects
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C. Other effects on observers
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D. Experimental support for the theory
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II. Space-Time Diagrams
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A. What are Space-Time Diagrams?
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B. Constructing one for a "stationary" observer
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C. Constructing one for a "moving" observer
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D. Interchanging "stationary" and "moving"
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E. Introducing the light cone
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F. Comparing the way two observers view space and time
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III. The First Problem: The Light Speed Barrier
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A. Effects as one approaches the speed of light
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B. Conceptual ideas around this problem
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IV. The Second Problem: FTL Implies The Violation of Causality
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A. What is meant here by causality, and its importance
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B. Why FTL travel of any kind implies violation of causality
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C. A scenario as "proof"
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V. A Way Around the Second Problem
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A. Warped space as a special frame of reference
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B. How this solves the causality problem
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C. The relativity problem this produces
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D. One way around that relativity problem
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VI. Conclusion.
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I. An Introduction to Special Relativity
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The main goal of this introduction is to make relativity and its
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consequences feasible to those who have not seen them before. It should
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also reinforce such ideas for those who are already somewhat familiar
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with them. This introduction will not completely follow the traditional
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way in which relativity came about. It will begin with a pre-Einstein
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view of relativity. It will then give some reasoning for why Einstein's
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view is plausible. This will lead to a discussion of some of the
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consequences this theory has, odd as they may seem. Finally, I want to
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mention some experimental evidence that supports the theory.
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The idea of relativity was around in Newton's day, but it was
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incomplete. It involved transforming from one frame of reference to
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another frame which is moving with respect to the first. The
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transformation was not completely correct, but it seemed so in the realm
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of small speeds.
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Here is an example of this to make it clear. Consider two
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observers, you and me, for example. Let's say I am on a train that
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passes you at 30 miles per hour. I throw a ball in the direction the
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train is moving, and the ball moves at 10 mph in MY point of view. Now
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consider a mark on the train tracks. You see the ball initially moving
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along at the same speed I am moving (the speed of the train). Then I
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throw the ball, and the ball is able to reach the mark on the track
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before I do. So to you, the ball is moving even faster than I (and the
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train). Obviously, it seems as if the speed of the ball with respect to
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you is just the speed of the ball with respect to me plus the speed of
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me with respect to you. So, the speed of the ball with respect to you
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= 10 mph + 30 mph = 40 mph. This was the first, simple idea for
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transforming velocities from one frame of reference to another. In other
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words, this was part of the first concept of relativity.
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Now I introduce you to an important postulate that leads to the
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concept of relativity that we have today. I believe it will seem quite
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reasonable. I state it as it appears in a physics book by Serway: "the
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laws of physics are the same in every inertial frame of reference."
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What it means is that if you observe any physical laws for a given
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situation in your frame of reference, then an observer in a reference
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frame moving with a constant velocity with respect to you should also
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agree that those physical laws apply to that situation.
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As an example, consider the conservation of momentum. Say that
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there are two balls coming straight at one another. They collide and go
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off in opposite directions. Conservation of momentum says that if you
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add up the total momentum (mass times velocity) before the collision and
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after the collision, that the two should be identical. Now, let this
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experiment be performed on a train where the balls are moving along the
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line of the train's motion. An outside observer would say that the
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initial and final velocities of the balls are one thing, while an
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observer on the train would say they were something different. However,
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BOTH observers must agree that the total momentum is conserved. They
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will disagree on what the actual numbers are, but they will agree that
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the law holds. We should be able to apply this to any physical law. If
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not, (i.e., if physical laws were different for different frames of
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reference) then we could change the laws of physics just by traveling in
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a particular reference frame.
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A very interesting result occurs when you apply this postulate to
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the laws of electrodynamics. What one finds is that in order for the
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laws of electrodynamics to be the same in all inertial reference frames,
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it must be true that the speed of electromagnetic waves (such as light)
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is the same for all inertial observers. Simply stating that may not
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make you think that there is anything that interesting about it, but it
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has amazing consequences. Consider letting a beam of light take the
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place of the ball in the first example given in this introduction. If
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the train is moving at half the velocity of light, wouldn't you expect
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the light beam (which is traveling at the speed of light with respect to
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the train) to look as if it is traveling one and a half that speed with
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respect to an outside observer? Well, this is not the case. The old
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ideas of relativity in Newton's day do not apply here. What accounts
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for this peculiarity is time dilation and length contraction.
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Now, I give an example of how time dilation can help explain a
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peculiarity that arises from the above concept. Again we consider a
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train, but let's give it a speed of 0.6 c (where c = the speed of light
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which is 3E8 m/s--3E8 means 3 times 10 to the eighth). An occupant of
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this train shines a beam of light so that (to him) the beam goes
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straight up, hits a mirror at the top of the train, and bounces back to
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the floor of the train where some instrument detects it. Now, in my
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point of view (outside the train), that beam of light does not travel
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straight up and straight down, but makes an up-side-down "V" shape
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because of the motion of the train. Here is a diagram of what I see:
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/|\
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/ | \
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/ | \
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light beam going up->/ | \<-light beam on return trip
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/ | \
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/ | \
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/ | \
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/ | \
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---------|---------->trains motion (v = 0.6 c)
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Let's say that the trip up takes 10 seconds in my point of view. The
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distance the train travels during that time is:
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(0.6 * 3E8 m/s) * 10 s = 18E8 m.
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The distance that the beam travels on the way up (the slanted line to
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the left) must be
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3E8 m/s * 10s = 30E8 m.
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Since the left side of the above figure is a right triangle, and we know
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the length of two of the sides, we can now solve for the height of the
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train:
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Height = [(30E8 m)^2 - (18E8 m)^2]^0.5 = 24E8 m.
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(It is a tall train, but this IS just a thought experiment.) Now we
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consider the frame of reference of the traveler. The light MUST travel
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at 3E8 m/s for him also, and the height of the train doesn't change
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because relativity contracts only lengths in the direction of motion.
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Therefore, in his frame the light will reach the top of the train in
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24E8 m / 3E8 (m/s) = 8 seconds,
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and there you have it. To me the event takes 10 seconds, while
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according to him it must take only 8 seconds. We measure time in
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different ways.
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To intensify this oddity, consider the fact that all inertial
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frames are equivalent. That is, from the traveler's point of view he is
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the one who is sitting still, while I zip past him at 0.6 c. So he will
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think that it is MY clock that is running slowly. This lends itself
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over to what seem to be paradoxes which I will not get into here. If
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you have any questions on such things (such as the "twin paradox" --
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which can be understood with special relativity, by the way) feel free
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to ask me about them, and I will do the best I can to answer you.
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As I mentioned above, length contraction is another consequence
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of relativity. Consider the same two travelers in our previous example,
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and let each of them hold a meter stick horizontally (so that the length
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of the stick is oriented in the direction of motion of the train). To
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the outside observer, the meter stick of the traveler on the train will
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look as if it is shorter than a meter. Similarly, the observer on the
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train will think that the meter stick of the outside observer is the one
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that is contracted. The closer one gets to the speed of light with
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respect to an observer, the shorter the stick will look to that
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observer. The factor which determines the amount of length contraction
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and time dilation is called gamma.
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Gamma is defined as (1 - v^2/c^2)^(-1/2). For our train (for
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which v = 0.6 c), gamma is 1.25. Lengths will be contracted and time
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dilated (as seen by the outside observer) by a factor of 1/gamma = 0.8,
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which is what we demonstrated with the difference in measured time (8
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seconds compared to 10 seconds). Gamma is obviously an important number
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in relativity, and it will appear as we discuss other consequences of
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the theory.
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Another consequence of relativity is a relationship between mass,
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energy, and momentum. By considering conservation of momentum and
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energy as viewed from two frames of reference, one can find that the
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following relationship must be true for an unbound particle:
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E^2 = p^2 * c^2 + m^2 * c^4
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Where E is energy, m is mass, and p is relativistic momentum which is
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defined as
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p = gamma * m * v (gamma is defined above)
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By manipulating the above equations, one can find another way to express
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the total energy as
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E = gamma * m * c^2
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Even when an object is at rest (gamma = 1) it still has an energy of
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E = m * c^2
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Many of you have seen something like this stated in context with the
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theory of relativity.
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It is important to note that the mass in the above equations has
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a special definition which we will now discuss. As a traveler approaches
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the speed of light with respect to an observer, the observer sees the
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mass of the traveler increase. (By mass, we mean the property that
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indicates (1) how much force is needed to create a certain acceleration
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and (2) how much gravitational pull you will feel from that object).
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However, the mass in the above equations is defined as the mass measured
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in the rest frame of the object. That mass is always the same. The
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mass seen by the observer (which I will call the observed mass) is given
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by gamma * m. Thus, we could also write the total energy as
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E = (observed mass) * c^2
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That observed mass approaches infinity as the object approaches the
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speed of light with respect to the observer.
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These amazing consequences of relativity do have experimental
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foundations. One of these involves the creation of muons by cosmic rays
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in the upper atmosphere. In the rest frame of a muon, its life time is
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only about 2.2E-6 seconds. Even if the muon could travel at the speed
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of light, it could still go only about 660 meters during its life time.
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Because of that, they should not be able to reach the surface of the
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Earth. However, it has been observed that large numbers of them do
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reach the Earth. From our point of view, time in the muons frame of
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reference is running slowly, since the muons are traveling very fast
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with respect to us. So the 2.2E-6 seconds are slowed down, and the muon
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has enough time to reach the earth.
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We must also be able to explain the result from the muons frame
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of reference. In its point of view, it does have only 2.2E-6 seconds to
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live. However, the muon would say that it is the Earth which is
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speeding toward the muon. Therefore, the distance from the top of the
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atmosphere to the Earth's surface is length contracted. Thus, from its
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point of view, it lives a very small amount of time, but it doesn't have
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that far to go.
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Another verification is found all the time in particle physics.
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The results of having a particle strike a target can be understood only
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if one takes the total energy of the particle to be E = Gamma * m * c^2,
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which was predicted by relativity.
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These are only a few examples that give credibility to the theory
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of relativity. Its predictions have turned out to be true in many
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cases, and to date, no evidence exists that would tend to undermine the
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theory.
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In the above discussion of relativity's effects on space and time
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we have looked at only length contraction and time dilation. However,
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there is a little more to it than that, and the next section attempts to
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explain this to some extent.
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II. Space-Time Diagrams
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In this section we examine certain constructions known as space-
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time diagrams. After a short look at why we need to discuss these
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diagrams, I will explain what they are and what purpose they serve.
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Next we will construct a space-time diagram for a particular observer.
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Then, using the same techniques, we will construct a second diagram to
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represent the coordinate system for a second observer who is moving with
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respect to the first observer. This second diagram will show the second
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observer's frame of reference with respect to the first observer;
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however, we will also switch around the diagram to show what the first
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observer's frame of reference looks like with respect to the second
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observer. Finally, we will compare the way these two observers view
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space and time, which will make it necessary to first discuss a diagram
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known as a light cone.
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In the previous section we talked about the major consequences of
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special relativity, but now I want to concentrate more specifically on
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how relativity causes a transformation of space and time. Relativity
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causes a little more than can be understood by simple length contraction
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and time dilation. It actually results in two different observers
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having two different space-time coordinate systems. The coordinates
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transform from one frame to the other through what are known as a
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Lorentz Transformation. Without getting deep into the math, much can be
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understood about such transforms by considering space-time diagrams.
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A space-time diagram gives us a means of representing events
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which occur at different locations and at different times. For the
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space part of the diagram, we will be looking in only one direction, the
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x direction. So, the space-time diagram consists of a coordinate system
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with one axis to represent space (the x direction) and another to
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represent time. Where these two principle axes meet is the origin.
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This is simply a point in space that we have defined as x = 0 and a
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moment in time that we have defined as t = 0. In Diagram 1 (below) I
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have drawn these two axes and marked the origin with an o.
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For certain reasons we want to define the units that we will use
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for distances and times in a very specific way. Let's define the unit
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for time to be the second. This means that moving one unit up the time
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axis will represent waiting one second of time. We then want to define
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the unit for distance to be a light second (the distance light travels
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in one second). So if you move one unit to the right on the x axis, you
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will be looking at a point in space that is one light second away from
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your previous location. In Diagram 1, I have marked the locations of
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the different space and time units (Note: In my diagrams, I am using
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four spaces to be one unit along the x axis and two character heights
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to be one unit on the time axis).
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With these units it is interesting to note how a beam of light is
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represented in our diagram. Consider a beam of light leaving the origin
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and traveling to the right. One second later, it will have traveled one
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light second away. Two seconds after it leaves it will have traveled
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two light seconds away, and so on. So a beam of light will always make
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a line at an angle of 45 degrees to the x and t axes. I have drawn such
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a light beam in Diagram 2.
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Diagram 1 Diagram 2
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t t
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^ ^
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| | light
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+ + /
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+ + /
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-+---+---o---+---+---> x -+---+---o---+---+-> x
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+ +
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+ +
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At this point, we want to decide exactly how to represent events
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on this coordinate system. First, when we say that we are using this
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diagram to represent the reference frame of a particular observer, we
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mean that in this diagram the observer is not moving. We will call this
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observer the O observer. So if the O observer starts at the origin,
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then one second later he is still at x = 0. Two seconds later he is
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still at x = 0, etc. So, he is always on the time axis in our
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representation. Similarly, any lines drawn parallel to the t axis (in
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this case, vertical lines) will represent lines of constant position.
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If a second observer is not moving with respect to the first, and this
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second observer starts at a position two light seconds away to the right
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of the first, then as time progresses he will stay on the vertical line
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that runs through x = 2.
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Next we want to figure out how to represent lines of constant
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time. To do this, we should first find a point on our diagram that
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represents an event which occurs at the same time as the origin (t = 0).
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To do this we will use a method that Einstein used. First we choose a
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point on the t axis which occurred prior to t = 0. Let's use an example
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where this point is occurs at t = -3 seconds. At that time we send out
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a beam of light in the positive x direction. If the beam bounces off of
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a distant mirror at t = 0 and heads back toward the t axis, then it
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will come back to the us at t = 3 seconds. So, if we send out a beam at
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t = -3 seconds and it returns at t = 3 seconds, then the event of it
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bouncing off the mirror occurred simultaneously with the time t = 0.
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To use this in our diagram, we first pick two points on the t
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axis that mark t = -3 and t = 3 (let's call these points A and B
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respectively). We then draw one light beam leaving from A in the
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positive x direction. Next we draw a light beam coming to B in the
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negative x direction. Where these two beams meet (let's call this point
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C) marks the point where the original beam bounces off the mirror. Thus
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the event marked by C is simultaneous with t = 0 (the origin). A line
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drawn through C and o will thus be a line of constant time. All lines
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parallel to this line will also be lines of constant time. So any two
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events that lie along one of these lines occur at the same time in this
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frame of reference. I have drawn this procedure in Diagram 3, and you
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can see that the x axis is the line through both o and C which is a line
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of simultaneity (as one might have expected).
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Now, by constructing a set of simultaneous time lines and
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simultaneous position lines we will have a grid on our space-time
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diagram. Any event has a specific location on the grid which tells when
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and where it occurs. In Diagram 4 I have drawn one of these grids and
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marked an event (@) that occurred 3 light seconds away to the left of
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the origin (x = -3) and 1 light seconds before the origin (t = -1).
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Diagram 3 Diagram 4
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t t
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| | | | | | |
|
|
B ---+---+---+---+---+---+---
|
|
| \ | | | | | |
|
|
+ \ ---+---+---+---+---+---+---
|
|
| \ | | | | | |
|
|
+ \ ---+---+---+---o---+---+--- x
|
|
| \ | | | | | |
|
|
-+---+---o---+---+---C- x ---@---+---+---+---+---+---
|
|
| / | | | | | |
|
|
+ / ---+---+---+---+---+---+---
|
|
| / | | | | | |
|
|
+ /
|
|
| /
|
|
A
|
|
|
|
|
|
|
|
|
Now comes an important addition to our discussion of space-time
|
|
diagrams. The coordinate system we have drawn will work fine for any
|
|
observer who is not moving with respect to the O observer. Now we want
|
|
to construct a coordinate system for an observer who IS traveling with
|
|
respect to the O observer. The trajectories of two such observers have
|
|
been drawn in Diagrams 5 and 6. Notice that in our discussion we will
|
|
always consider moving observers who pass by the O observer at the time
|
|
t = 0 and at the position x = 0. Now, the traveler in Diagram 5 is
|
|
moving slower than the one in Diagram 6. You can see this because in a
|
|
given amount of time, the Diagram 6 traveler has moved further away from
|
|
the time axis than the Diagram 5 traveler. So the faster a traveler
|
|
moves, the more slanted this line becomes.
|
|
|
|
|
|
Diagram 5 Diagram 6
|
|
t t
|
|
| / | /
|
|
+ + /
|
|
| / | /
|
|
+ + /
|
|
|` |/
|
|
-+---+---o---+---+--- x -+---+---o---+---+- x
|
|
,| /|
|
|
+ / +
|
|
/ | / |
|
|
+ / +
|
|
/ | / |
|
|
|
|
|
|
What does this line actually represent? Well, consider an object
|
|
sitting on this line, right next to our moving observer. If a few
|
|
seconds later the object is still sitting on that line (right next to
|
|
him), then in his point of view, the object has not moved. The line is
|
|
a line of constant position for the moving observer. But that means
|
|
that this line represents the same thing for the moving observer as the
|
|
t axis represented for the O observer; and in fact, this line becomes
|
|
the moving observer's new time axis. We will mark this new time axis as
|
|
t' (t-prime). All lines parallel to this slanted line will also be
|
|
lines of constant position for our moving observer.
|
|
Now, just as we did for the O observer, we want to construct
|
|
lines of constant time for our traveling observer. To do this, we will
|
|
use the same method that we did for the O observer. The moving observer
|
|
will send out a light beam at some time t' = -T, and the beam will
|
|
bounce off some mirror so that it returns at time t' = +T. Then the point
|
|
at which the beam bounces off the mirror will be simultaneous with the
|
|
origin, where t' = t = 0.
|
|
There is a very important point to note here. What if instead of
|
|
light, we wanted to throw a ball at 0.5 c, have it bounce off some wall,
|
|
and then return at the same speed (0.5 c). The problem with this is
|
|
that to find a line of constant time for the moving observer, then the
|
|
ball must travel at 0.5 c both ways in the reference frame of the MOVING
|
|
observer. But we have not yet defined the coordinate system for the
|
|
moving observer, so we do not know what a ball moving at 0.5 c with
|
|
respect to him will look like on our diagram. However, because of
|
|
relativity, we know that the speed of light itself CANNOT change from
|
|
one observer to the next. In that case, a beam of light traveling at c
|
|
in the frame of the moving observer will also be traveling at c for the
|
|
O observer. So no matter what observer we are representing on our
|
|
diagram, a beam of light will ALWAYS make a 45 degree angle with respect
|
|
to the x and t axes.
|
|
In Diagram 7, I have labeled a point A' which occurs some amount
|
|
of time before t' = 0 and a point B' which occurs the same amount of
|
|
time after t' = 0. I then drew the two light rays as before and found
|
|
the point where they would meet (C'). Thus, C' and o occur at the same
|
|
time in the eyes of the moving observer. Notice that for the O
|
|
observer, C' is above his line of simultaneity (the x axis). So while
|
|
the moving observer says that C' occurs when the two observers pass (at
|
|
the origin), the stationary observer says that C' occurs after the two
|
|
observers have passed by one another. In Diagram 8, I have drawn a line
|
|
passing through C' and o. This line represents the same thing for our
|
|
moving observer as the x axis did for the O observer. So we label this
|
|
line x'.
|
|
From the geometry involved in finding this x' axis, we can state
|
|
a general rule for finding the x' axis for any moving observer. First
|
|
recall that the t' axis is the line that represents the moving
|
|
observer's position on the space-time diagram. The faster O' is moving
|
|
with respect to O, the greater the angle between the t axis and the t'
|
|
axis. So the t' axis is rotated at some angle (either clockwise or
|
|
counterclockwise, depending on the direction O' is going--left or right)
|
|
away from the t axis. The x' axis is a line rotated at the same angle,
|
|
but in the _opposite_ direction (counterclockwise or clockwise) away
|
|
from the x axis.
|
|
|
|
|
|
Diagram 7 Diagram 8
|
|
t t t'
|
|
| / | /
|
|
+ B' + /
|
|
| / \ | / __--x'
|
|
+ / C' + / __C'-
|
|
|/ / |/__--
|
|
-+---+---+---o---/---+---+- x -+---+---+-__o---+---+---+- x
|
|
/| / * __-- /|
|
|
/ / __-- / +
|
|
// | -- / |
|
|
A' + / +
|
|
/ | / |
|
|
|
|
|
|
Now, x' is a line of constant time for O', and any line drawn
|
|
parallel to x' is also a line of constant time. Such lines, along with
|
|
the lines of constant position form a grid of the space-time coordinates
|
|
for the O' observer. I have tried my best to draw such a grid in
|
|
Diagram 9. If you squint your eyes while looking at that diagram, you
|
|
can see the skewed squares of the coordinate grid. You can see that if
|
|
you pick a point on the space-time diagram, the two observers with their
|
|
two different coordinate systems will disagree on when and where the
|
|
event occurs.
|
|
As a final note about this, think back to what really made these
|
|
two coordinate systems look differently. Well, the only thing we
|
|
assumed in creating these systems is that the speed of light is the same
|
|
for all observers. In fact, this is the only reason that the two
|
|
coordinate systems look the way they do.
|
|
|
|
In our understanding of space-time diagrams, I also want to
|
|
incorporate the idea that all reference frames that move with a constant
|
|
velocity are considered equivalent. By this I mean that O was
|
|
considered as the stationary observer only because we defined him as
|
|
such. Then, when I called O' the moving observer, I meant that he was
|
|
moving with respect to O. However, we should just as easily be able to
|
|
define O' as the stationary observer. Then, to him, O is moving away
|
|
from him to the left. Then, we should be able to draw the t' and x'
|
|
axes as the vertical and horizontal lines, while the t and x axes become
|
|
the rotated lines. I have done this in Diagram 10. By examining this
|
|
Diagram, you can confirm that it makes sense to you in light of our
|
|
discussion thus far.
|
|
|
|
|
|
Diagram 9 Diagram 10
|
|
t' t t'
|
|
+-----------------/-------+ \ |
|
|
| / /_-/""/ /__/-"/ / _| \ +
|
|
|/-"/ / _/--/" / /_-/""/| \ |
|
|
| /_-/""/ /__/-"/ / _/-->x' \ +
|
|
|"/ / _/--/" / /_-/""/ | \|
|
|
|/_-/""/ /__o-"/ / _/--/| ---+---+---o-__+---+--- x'
|
|
| / _/--/" / /_-/""/ /_| | ""--__
|
|
|-/""/ /__/-"/ / _/--/" | + ""--x
|
|
|/ _/--/" / /_-/""/ /__/| |
|
|
|""/ /__/-"/ / _/--/" / | +
|
|
+-------------------------+ |
|
|
|
|
The last thing I want to do in this discussion is to compare the
|
|
way our two observers view a particular event. First, let me note that
|
|
with what we have discussed we cannot make a complete comparison of the
|
|
two observers' coordinate systems. You see, we have not seen how the
|
|
lengths which represents one unit of space and time in the reference
|
|
frame of O compares with the lengths representing the same units in O'.
|
|
I will tell you that the lengths are in fact different; however, I will
|
|
not take up any more of your time by going into exactly how they
|
|
compare. Also, to do this comparison one would use the fact that for
|
|
the observers we have defined, if an event occurs at a point (x,t) for O
|
|
and (x',t') for O', then x^2 - t^2 = x'^2 - t'^2. The best way to show
|
|
this on the diagram is to draw hyperbolas represented by these
|
|
equations, and I don't even want to consider how to do this with my
|
|
limited experience with ASCII graphics.
|
|
There is, however, one comparison that we can make, and it will
|
|
be of importance in later discussions. In Diagram 8, in addition to the
|
|
O and O' space and time axes, I have also marked a particular event with
|
|
a star, "*". Recall that for O, any event on the x axis occurs at the
|
|
same time as the origin (the place and time that the two observers pass
|
|
each other). Since the marked event appears under the x axis, then O
|
|
must believe that the event occurs before the observers pass each other.
|
|
Also recall that for O', those events on the x' axis are the ones that
|
|
occur at the same time the observers are passing. Since the marked
|
|
event appears above the x' axis, O' must believe that the event occurs
|
|
after the observers pass each other. So, when and where events occur
|
|
with respect to other events is completely dependent on who is observing
|
|
the events. Now, how can this make sense? How can one event be both in
|
|
the future for one observer and in the past to another observer. To
|
|
better understand why this situation doesn't contradict itself, we need
|
|
to look at one other construction typically shown on a space-time
|
|
diagram.
|
|
In Diagram 11 I have drawn two light rays, one which travels in
|
|
the +x direction and another which travels in the -x direction. At some
|
|
negative time, the two rays were headed towards x = 0. At t = 0, the
|
|
two rays finally get to x = 0 and cross paths. As time progresses, the
|
|
two then speed away from x = 0. This construction is known as a light
|
|
cone.
|
|
A light cone divides a space-time diagram into two major
|
|
sections: the area inside the cone and the area outside the cone (as
|
|
shown in Diagram 11). Let me mention here that specifically I will call
|
|
the cone I have drawn a light cone centered at the origin, because that
|
|
is where the two beams meet. Now, consider an observer who has been
|
|
sitting at x = 0 (like our O observer) and is receiving and sending
|
|
signals at the moment marked by t = 0. Obviously, if he sends out a
|
|
signal, it proceeds away from x = 0 into the future, and the event
|
|
marked by someone receiving the signal would be above the x axis (in his
|
|
future). Also, if he is receiving signals at t = 0, then the event
|
|
marked by someone sending the signal would have to be under the x axis
|
|
(in his past). Now, if it is impossible for anything to travel faster
|
|
than light, then the only events occurring before t = 0 that the observer
|
|
can know about at the moment are those that are inside the light cone.
|
|
Also, the only future events (those occurring after t = 0) that he can
|
|
influence are, again, those inside the light cone.
|
|
Now, one of the most important things to note about a light cone
|
|
is that it's position is the same for all observers (because the speed of
|
|
light is the same for all observers). For example, picture taking the
|
|
skewed coordinate system of the moving observer and superimposing it on
|
|
the light cone I have drawn. If you were to move one unit "down" the x'
|
|
axis (a distance that represents one light second for our moving
|
|
observer), and you move one unit "up" the t' axes (one second for our
|
|
moving observer), then the point you end up at should lie somewhere on
|
|
the light cone. In effect, a light cone will always look the same on
|
|
our diagram reguardless of which observer is drawing the cone.
|
|
This fact has great importance. Consider different observers who
|
|
are all passing by one another at some point in space and time. In
|
|
general, they will disagree with each other on when and where different
|
|
events have and will occur. However, if you draw a light cone centered
|
|
at the point where they are passing each other, then they will ALL agree
|
|
as to which events are inside the light cone and which events are
|
|
outside the light cone. So, reguardless of the coordinate system for
|
|
any of these observers, the following facts remain: The only events
|
|
that any of these observers can ever hope to influence are those which
|
|
lie inside the upper half of the light cone. Similarly, the only events
|
|
that any of these observers can know about as they pass by one another
|
|
are those which lie inside the lower half of the cone.
|
|
Now let's apply this to the observers and event in Diagram 8. As
|
|
you can see, the event in question is indeed outside the light cone.
|
|
Because of this, even though the event is in one observers past, he
|
|
cannot know about the event at this time. Also, even though the event
|
|
is in the other observer's future, he can never have an effect on the
|
|
event. In essence, the event (when it happens, where it happens, how it
|
|
happens, etc.) is of absolutely no consequence for these two observers at
|
|
this time. As it turns out, any time you find two observers who are
|
|
passing by one another and an event which one observer's coordinate
|
|
system places in the past and the other observer's coordinate system
|
|
places in the future, then the event will always be outside of the light
|
|
cone for the observers.
|
|
But doesn't this relativistic picture of the universe still
|
|
present an ambiguity in the concepts of past and future? Perhaps
|
|
philosophically it does, but not physically. You see, the only time you
|
|
can see these ambiguities is when you are looking at the whole space-
|
|
time picture at once. If you were one of the observers who is actually
|
|
viewing space and time, then as the other observer passes by you, your
|
|
whole picture of space and time can only be constructed from events that
|
|
are inside the lower half of the light cone. If you wait for a while,
|
|
then eventually you can get all of the information from all of the events
|
|
that were happening around the time you were passing the other observer.
|
|
From this information, you can draw the whole space-time diagram, and
|
|
then you can see the ambiguity. But by that time, the ambiguity that
|
|
you are considering no longer exists. So the ambiguity can never
|
|
actually play a part in any physical situation. Finally, remember that
|
|
this is only true if nothing can travel faster than the speed of light.
|
|
|
|
Diagram 11
|
|
t
|
|
^
|
|
| light
|
|
\ + /
|
|
\ inside /
|
|
\ + /
|
|
outside \ | / outside
|
|
---+---+---o---+---+---> x
|
|
/ | \
|
|
/ + \
|
|
/ inside \
|
|
/ + \
|
|
|
|
|
|
|
|
|
Well, that concludes our look at relativity and space-time
|
|
diagrams. Now, we can use these concepts to discuss the problems
|
|
presented by FTL travel.
|
|
|
|
|
|
|
|
|
|
|
|
III. The First Problem: The Light Speed Barrier
|
|
|
|
In this section we discuss the first thing (and in some cases the
|
|
only thing) that comes to mind for most people who consider the problem
|
|
of faster than light travel. I call it the light speed barrier. As we
|
|
will see by considering ideas from the first section, light speed seems
|
|
to be a giant, unreachable wall standing in our way. I also introduce a
|
|
couple of fictional ways to get around this barrier; however, part of my
|
|
reason for introducing these solutions is to show that they do not solve
|
|
the problem discussed in the next section.
|
|
|
|
Consider two observers, A and B. Let A be here on Earth and be
|
|
considered at rest for now. B will be speeding past A at highly
|
|
relativistic speeds. If B's speed is 80% that of light with respect to
|
|
A, then gamma for him (as defined in the first section) is
|
|
1.6666666... = 1/0.6
|
|
So from A's point of view B's clock is running slow and B's lengths in
|
|
the direction of motion are shorter by a factor of 0.6. If B were
|
|
traveling at 0.9 c, then this factor becomes about 0.436; and at 0.99 c,
|
|
it is about 0.14. As the speed gets closer and closer to the speed of
|
|
light, A will see B's clock slow down infinitesimally slow, and A will
|
|
see B's lengths in the direction of motion becoming infinitesimally
|
|
small.
|
|
In addition, If B's speed is 0.8 c with respect to A, then A will
|
|
see B's observed mass as being larger by a factor of gamma (which is
|
|
1.666...). At 0.9 c and 0.99 c this factor is about 2.3 and 7.1
|
|
respectively. As the speed gets closer and closer to the speed of
|
|
light, A will see B's observed mass (and thus his energy) become
|
|
infinitely large.
|
|
Obviously, from A's point of view, B will not be able to reach
|
|
the speed of light without stopping his own time, shrinking to
|
|
nothingness in the direction of motion, and taking on an infinite amount
|
|
of energy.
|
|
|
|
Now let's look at the situation from B's point of view, so we
|
|
will consider him to be at rest. First, notice that the sun, the other
|
|
planets, the nearby stars, etc. are not moving very relativistically
|
|
with respect to the Earth; so we will consider all of these to be in the
|
|
same frame of reference. Let B be traveling past the earth and toward
|
|
some nearby star. In his point of view, the earth, the sun, the other
|
|
star, etc. are the ones traveling at highly relativistic velocities with
|
|
respect to him. So to him the clocks on Earth are running slow, the
|
|
energy of all those objects becomes greater, and the distances between
|
|
the objects in the direction of motion become smaller.
|
|
Let's consider the distance between the Earth and the star to
|
|
which B is traveling. From B's point of view, as the speed gets closer
|
|
and closer to that of light, this distance becomes infinitesimally
|
|
small. So from his point of view, he can get to the star in practically
|
|
no time. (This explains how A seems to think that B's clock is
|
|
practically stopped during the whole trip when the velocity is almost
|
|
c.) If B thinks that at the speed of light that distance shrinks to
|
|
zero and that he is able to get there instantaneously, then from his
|
|
point of view, c is the fastest possible speed.
|
|
|
|
So from either point of view, it seems that the speed of light
|
|
cannot be reached, much less exceeded. However, through some inventive
|
|
imagination, it is possible to come up with fictional ways around this
|
|
problem. Some of these solutions involve getting from point A to point
|
|
B without traveling through the intermittent space. For example,
|
|
consider a forth dimension that we can use to bend two points in our
|
|
universe closer together (sort of like connecting two points of a "two
|
|
dimensional" piece of paper by bending it through a third dimension and
|
|
touching the two points directly). Then a ship could travel between two
|
|
points without moving through the space in between, thus bypassing the
|
|
light speed barrier.
|
|
Another idea involves bending the space between the points to
|
|
make the distance between them smaller. In a way, this is what highly
|
|
relativistic traveling looks like from the point of view of the
|
|
traveler; however, we don't want the associated time transformation. So
|
|
by fictionally bending the space to cause the space distortion without
|
|
the time distortion, one can imagine getting away from the problem.
|
|
|
|
Again I remind you that these solutions only take care of the
|
|
"light speed barrier" problem. They do not solve the problem discussed
|
|
in the next section, as we shall soon see.
|
|
|
|
|
|
|
|
|
|
IV. The Second Problem: FTL Implies The Violation of Causality
|
|
|
|
In this section we explore the violation of causality involved
|
|
with faster than light travel. First I will explain what we mean here
|
|
by causality and why it is important that we do not simply throw it
|
|
aside without a second thought. I will then try to explain why any
|
|
faster than light method that allows you to travel faster than light in
|
|
any frame you wish will also allow you to violate causality.
|
|
|
|
When I speak of causality, I have the following particular idea
|
|
in mind. Consider an event A which has an effect on another event B.
|
|
Causality would require that event B cannot in turn have an effect on
|
|
event A. For example, let's say that event A is a murderer making a
|
|
decision to shoot and kill his victim. Let's then say that event B is
|
|
the victim being shot and killed by the murderer. Causality says that
|
|
the death of the victim cannot then have any effect on the murderer's
|
|
decision. If the murderer could see his dead victim, go back in time,
|
|
and then decide not to kill him after all, then causality would be
|
|
violated. In time travel "theories," such problems are reasoned with
|
|
the use of multiple time lines and the likes; however, since we do not
|
|
want every excursion to a nearby star to create a new time line, we
|
|
would hope that FTL travel could be done without such causality
|
|
violations. As I shall now show, this is not a simple problem to get
|
|
around.
|
|
|
|
I refer you back to the diagrams in the second section so that I
|
|
can demonstrate the causality problem involved with FTL travel. In
|
|
Diagram 8, two observers are passing by one another. At the moment
|
|
represented by the principle axes shown, the two observers are right
|
|
next to one another an the origin. The x' and t' axes are said to
|
|
represent the K-prime frame of reference (I will call this Kp for
|
|
short). The x and t axes are then the K frame of reference. We define
|
|
the K system to be our rest system, while the Kp observer passes by K at
|
|
a relativistic speed. As you can see, the two observers measure space
|
|
and time in different ways. For example, consider again the event
|
|
marked "*". Cover up the x and t axis and look only at the Kp system.
|
|
In this system, the event is above the x' axis. If the Kp observer at
|
|
the origin could look left and right and see all the way down his space
|
|
axis instantaneously, then he would have to wait a while for the event
|
|
to occur. Now cover up the Kp system and look only at the K system. In
|
|
this system, the event is below the x axis. So to the observer in the K
|
|
system, the event has already occurred.
|
|
Normally, this fact gives us no trouble. If you draw a light
|
|
cone (as discussed in the second section) through the origin, then the
|
|
event will be outside of the light cone. As long as no signal can
|
|
travel faster than the speed of light, then it will be impossible for
|
|
either observer to know about or influence the event. So even though it
|
|
is in one observer's past, he cannot know about it, and even though it is
|
|
in the other observer's future, he cannot have an effect on it. This is
|
|
how relativity saves its own self from violating causality.
|
|
Now consider what would happen if a signal could be sent
|
|
arbitrarily fast. From K's frame of reference, the event has already
|
|
occurred. For example, say the event occurred a year ago and 5 light
|
|
years away. As long as a signal can be sent at 5 times the speed of
|
|
light, then obviously K can receive a signal from the event. However,
|
|
from Kp's frame of reference, the event is in the future. So as long as
|
|
he can send a signal sufficiently faster than light, he can get a signal
|
|
out to the place where the event will occur before it occurs. So, in
|
|
the point of view of one observer, the event can be known about. This
|
|
observer can then tell the other observer as they pass by each other.
|
|
Then the second observer can send a signal out that could change that
|
|
event. This is a violation of causality.
|
|
Basically, when K receives a signal from the event, Kp sees the
|
|
signal as coming from the future. Also, when Kp sends a signal to the
|
|
event, K sees it as a signal being sent into the past. In one frame of
|
|
reference the signal is moving faster than light, while in the other
|
|
frame it is going backwards in time. Also notice that in this example I
|
|
never mentioned anything about how the signal gets between two points.
|
|
I didn't even require that the signal be "in our universe" when it is
|
|
traveling. The only thing I required is that the signal starts and ends
|
|
as events in our universe. As long as this is true, and as long as
|
|
either observer (K or Kp) can send any faster than light signal in their
|
|
own frame of reference, then the causality problem can be produced.
|
|
As a short example of this, consider the following. Instead of
|
|
sending a message out, let's say that Kp sends out a bullet that travels
|
|
faster than the speed of light. This bullet can go out and kill someone
|
|
light-years away in only a few hours (for example) in Kp's frame of
|
|
reference. Now, say he fires this bullet just as he passes by K. Then
|
|
we can call the death of the victim the event (*). Now, in K's frame of
|
|
reference, the victim is already dead when Kp passes by. This means
|
|
that the victim could have sent a signal just after he was shot that
|
|
would reach K before Kp passed by. So K can know that Kp will shoot his
|
|
gun as he passes, and K can stop him. But then the victim is never hit,
|
|
so he never sends a message to K. So K doesn't know to stop Kp and Kp
|
|
does shoot the bullet. Obviously, causality is not very happy about
|
|
this logical loop that develops.
|
|
|
|
If this argument hasn't convinced you, then let me try one more
|
|
thought experiment to convince you of the problem. Here, to make
|
|
calculations easy, we assume that a signal can be sent infinitely fast.
|
|
|
|
Person A is on earth, and person B speeds away from earth at a
|
|
velocity v. To make things easy, let's say that v is such that for an
|
|
observer on Earth, person B's clock runs slow by a factor of 2. Now,
|
|
person A waits one hour after person B has passed earth. At that time
|
|
person A sends a message to person B which says "I just found a bomb
|
|
under my chair that will take 10 minutes to defuse, but goes off in 10
|
|
seconds ... HELP" He sends it instantaneously from his point of view...
|
|
well, from his point of view, B's clock has moved only half an hour. So
|
|
B receives the message half an hour after passing earth in his frame of
|
|
reference.
|
|
Now we must switch to B's point of view. From his point of view,
|
|
A has been speeding away from him at a velocity v. So, to B, it is A's
|
|
clock that has been running slow. Therefore, when he gets the message
|
|
half an hour after passing earth, then in his frame of reference, A's
|
|
clock has moved only 1/4 an hour. So, B sends a message to A that says:
|
|
"There's a bomb under your chair." It gets to A instantaneously, but
|
|
this time it is sent from B's frame of reference, so instantaneously
|
|
means that A gets the message only 1/4 of an hour after B passed Earth.
|
|
You see that A as received an answer to his message before he even sent
|
|
it. Obviously, there is a causality problem, no matter how you get the
|
|
message there.
|
|
OK, what about speeds grater than c but NOT instantaneous?
|
|
Whether or not you can use the above argument to find a causality
|
|
problem will depend on how fast you have B traveling. If you have a
|
|
communication travel faster than c, then you can always find a velocity
|
|
for B (v < c) such that a causality problem will occur. However, if you
|
|
send the communication at a speed that is less than c, then you cannot
|
|
create a causality problem for any velocity of B (as long as B's
|
|
velocity is also less that c).
|
|
|
|
So, it seems that if you go around traveling faster than the
|
|
speed of light, causality violations are sure to follow you around.
|
|
This causes some very real problems with logic, and I for one would like
|
|
to find a way around such problems. This next section intends to do just
|
|
that.
|
|
|
|
|
|
|
|
|
|
V. A Way Around the Second Problem
|
|
|
|
Now we can discuss my idea for getting around the causality
|
|
problem produced by FTL travel. I will move through the development of
|
|
the idea step by step so that it is clear to the reader. I will then
|
|
explain how the idea I pose completely gets rid of causality violations.
|
|
Finally, I will discuss the one "bad" side effect of my solution which
|
|
involves the fundamentals of relativity, and I will mention how this
|
|
might not be so bad after all.
|
|
|
|
Join me now on a science fictional journey of the imagination.
|
|
Picture, if you will, a particular area of space about one square light-
|
|
year in size. Filling this area of space is a special field which is
|
|
sitting relatively stationary with respect to the earth, the sun, etc.
|
|
(By stationary, I mean relativistically speaking. That means it could
|
|
still be moving at a few hundreds of thousands of meters per second with
|
|
respect to the earth. Even at that speed, someone could travel for a
|
|
few thousand years and their clock would be off by only a day or two
|
|
from earth's clocks.) So, the field has a frame of reference that is
|
|
basically the same as ours on earth. In our science fictional future, a
|
|
way is found to manipulate the very makeup (fabric, if you will) of this
|
|
field. When this "warping" is done, it is found that the field has a
|
|
very special property. An observer inside the warped area can travel at
|
|
any speed he wishes with respect to the field, and his frame of
|
|
reference will always be the same as that of the field. This means that
|
|
x and t axes in a space time diagram will be the same as the ones for
|
|
the special field, reguardless of the observer's motion. In our
|
|
discussion of relativity, we saw that in normal space a traveler's frame
|
|
of reference depends on his speed with respect to the things he is
|
|
observing. However, for a traveler in this warped space, this is no
|
|
longer the case.
|
|
To help you understand this, let's look at a simple example.
|
|
Consider two ships, A and B, which start out sitting still with respect
|
|
to the special field. They are in regular space, but in the area of
|
|
space where the field exists. At some time, Ship A warps the field
|
|
around him to produce a warped space. He then travels to the edge of
|
|
the warped space at a velocity of 0.999 c with respect to ship B. That
|
|
means that if they started at one end of the field, and A traveled to
|
|
the other end of the field and dropped back into normal space, then B
|
|
says the trip took 1.001001... years. (That's 1 light-year divided by
|
|
0.999 light-years per year.) Now, if A had traveled in normal space,
|
|
then his clock would have been moving slow by a factor of 22.4 with
|
|
respect to B's clock. To observer A, the trip would have only taken
|
|
16.3 days. However, by using the special field, observer A kept the
|
|
field's frame of reference during the whole trip. So he also thinks it
|
|
took 1.001001... years to get there.
|
|
Now, let's change one thing about this field. Let the field
|
|
exist everywhere in space that we have been able to look. We are able
|
|
to detect its motion with respect to us, and have found that it still
|
|
doesn't have a very relativistic speed with respect to our galaxy and
|
|
its stars. With this, warping the field now becomes a means of travel
|
|
within all known space.
|
|
|
|
The most important reason for considering this as a means of
|
|
travel in a science fiction story is that it does preserve causality, as
|
|
I will now attempt to show. Again, I will be referring to Diagram 8 in
|
|
the second section. In order to demonstrate my point, I will be doing
|
|
two things. First, I will assume that the frame of reference of the
|
|
field (let's call it the S frame) is the same as that of the x and t
|
|
system (the K system) shown in Diagram 8. Assuming that, I will show
|
|
that the causality violation discussed in the previous section will not
|
|
occur using the new method of travel. Second, I will show that we can
|
|
instead assume that the S frame is the same as that of the x' and t'
|
|
system (the K-prime--or Kp for short--system), and again causality will
|
|
be preserved.
|
|
Before I do this, let me remind you of how the causality
|
|
violation occurred. The event (*) in the diagram will again be focused
|
|
on to explore causality. This event is in the past of the K system, but
|
|
it is in the future of the Kp system. Since it is in the past according
|
|
to the K observer, an FTL signal could be sent from the event to the
|
|
origin where K would receive the signal. As the Kp observer passed by,
|
|
K could tell him, "Hay, here is an event that will occur x number of
|
|
light years away and t years in your future." Now we can switch over to
|
|
Kp's frame of reference. He sees a universe in which he now knows that
|
|
at some distant point an event will occur some time in the future. He
|
|
can then send a FTL signal that would get to that distant point before
|
|
the event happens. So he can influence the event, a future that he
|
|
knows must exist. That is a violation of causality. But now we have a
|
|
specific frame of reference in which any FTL travel must be done, and
|
|
this will save causality.
|
|
First, we consider what would happen if the frame of the special
|
|
field was the same as that of the K system. That means that the K
|
|
observer is sitting relatively still with respect to the field. So, in
|
|
the frame of reference of the field, the event "*" IS in the past. That
|
|
means that someone at event "*" can send a message by warping the field,
|
|
and the message will be able to get to origin. Again, the K observer
|
|
has received a signal from the event. So, again he can tell the Kp
|
|
observer about the event as the Kp observer passes by. Again, we switch
|
|
to Kp's frame of reference, and again he is in a universe in which he
|
|
now knows that at some distant point an event will occur some time in
|
|
the future. But here is where the "agains" stop. Before it was
|
|
possible for Kp to then send a signal out that would get to that distant
|
|
point before the event occurs. But NOW, to send a signal faster than
|
|
light, you must do so by warping the field, and the signal will be sent
|
|
in the field's frame of reference. But we have assumed that the field's
|
|
frame of reference is the same as K's frame, and in that frame, the
|
|
event has already occurred. So, as soon as the signal enters the warped
|
|
space, it is in a frame of reference in which the event is over with,
|
|
and it cannot get to the location of the event before it happens. What
|
|
Kp basically sees is that no matter how fast he tries to send the
|
|
signal, he can never get it to go fast enough to reach the event. In
|
|
K's frame, it is theoretically possible to send any signal, even an
|
|
instantaneous one in any direction; but in Kp's frame, some signals
|
|
which would appear to him to be FTL cannot be sent (specifically,
|
|
signals which would go back in time in the K frame). So we see that
|
|
under this first consideration, causality is preserved.
|
|
To further convince you of my point, I will now consider what
|
|
would happen if the frame of the special field was the same as that of
|
|
the Kp system instead of the K system. Again, consider an observer at
|
|
the event "*" who wishes to send a signal to K before Kp passes by K.
|
|
The event of K and Kp passing one another has the position of the origin
|
|
in our diagram. In order to send this signal, the observer at "*" must
|
|
warp the field and thus enter the system of the Kp observer. But in the
|
|
frame of reference of Kp, when he passes by K, the event "*" is in the
|
|
future. Another way of saying this is that in the Kp frame of
|
|
reference, when the event "*" occurs, Kp will have already passed K and
|
|
gone off on his merry way. So when the signal at "*" enters the warped
|
|
space, it's frame of reference switches to one in which K and Kp have
|
|
already passed by one another. That means that it is impossible for "*"
|
|
to send a signal that would get to K before Kp passes by. The
|
|
possibility of creating a causality violation thus ends here.
|
|
Let me summarize the two above scenarios. In the first
|
|
situation, K could know about the event before Kp passes. So Kp can
|
|
know about the event after he passes K, but Kp could not send a signal
|
|
that would then influence the event. In the second situation, Kp can
|
|
send a signal that would influence the event after he passed by K.
|
|
However, K could not know about the event before Kp passed, so Kp cannot
|
|
have previous knowledge of the event before he sends a signal to the
|
|
event. In either case, causality is safe. Also notice that only one
|
|
case can be true. If both cases existed at the same time, then
|
|
causality would be no safer than before. Therefore, only one special
|
|
field can exist, and using it must be the only way that FTL travel can
|
|
be done.
|
|
Many scenarios like the one above can be conceived using
|
|
different events and observers, and (under normal situations) FTL
|
|
travel/communication can be shown to violate causality. However, in all
|
|
such cases the same types of arguments are used that I have used here,
|
|
and the causality problem is still eliminated by using the special
|
|
field. In general, this is because no observer can ever send a signal
|
|
which goes backward in time in the frame of the special field.
|
|
I thus see warp travel in Star Trek like this: Subspace is a
|
|
field which defines a particular frame of reference at all points in
|
|
known space. When you enter warp, you are using subspace such that you
|
|
keep its frame of reference reguardless of your speed. Not only does
|
|
this mean that normal warp travel cannot be used to grossly violate
|
|
causality, but since your frame of reference does not depend on your
|
|
speed as it does in relativity, relativistic effects in general do not
|
|
apply to travelers using warp. Since relativistic effects don't apply,
|
|
you also have a general explanation as to why you can exceed the speed
|
|
of light in the first place.
|
|
|
|
So, is this the perfect solution where FTL travel exists without
|
|
any side effects that make it logically impossible? Does this mean that
|
|
FTL travel in Star Trek lives, and all we have to do is accept the idea
|
|
that subspace/warped space involves a special frame of reference? Well,
|
|
not quite.
|
|
You see, there is one problem with all of this which involves the
|
|
basic ideas which helped form relativity. We said that an observer
|
|
using our special mode of transportation will always have the frame of
|
|
reference of the field. This means that his frame of reference does not
|
|
change with respect to his speed, and that travel within the warped
|
|
field does not obey Einstein's Relativity. At first glance, this
|
|
doesn't seem too bad, it just sounds like good science fiction. But
|
|
what happens when you observe the outside world while in warp? To
|
|
explore this, let's first look back at why it is necessary for the frame
|
|
of reference to change with respect to speed. We had assumed that the
|
|
laws of physics don't simply change for every different inertial
|
|
observer. It had been found that if the laws of electrodynamics look
|
|
the same to all inertial observers, then the speed of an electromagnetic
|
|
wave such as light must be the same for all observers. This in turn
|
|
made it necessary for different observers to have different frames of
|
|
reference. Now, let's go backwards through this argument. If different
|
|
observers using our special mode of transportation do not have different
|
|
frames of reference, then the speed of light will not look the same to
|
|
all observers. This in turn means that if you are observing an
|
|
electromagnetic event occurring in normal space while you are within the
|
|
warped space, the laws governing that occurrence will look different to
|
|
you than they would to an observer in normal space.
|
|
Perhaps this is not that big of a problem. One could assume that
|
|
what you see from within warped space is not actually occurring in real
|
|
space, but is caused by the interaction between the warped space and the
|
|
real universe. The computer could then compensate for these effects and
|
|
show you on screen what is really happening. I do not, however, pretend
|
|
that this is a sound explanation. This is the one part of the
|
|
discussion that I have not delved into very deeply. Perhaps I will look
|
|
further into this in the future, but it seems as if science fiction
|
|
could take care of this problem.
|
|
|
|
|
|
|
|
|
|
VI. Conclusion.
|
|
|
|
I have presented to you some major concepts of relativity and the
|
|
havoc they play with faster than light travel. I have shown you that the
|
|
violation of causality alone is a very powerful deterrent to faster than
|
|
light travel of almost any kind. So powerful are its effects, in fact,
|
|
that I have found only one way to get around them if we wish to have
|
|
faster than light travel readily available. I hope I have convinced you
|
|
that (1) causality is indeed very hard to get around, and (2) my idea
|
|
for a special field with a particular frame of reference does get around
|
|
it. For the moment, I for one see this as the only way that I would
|
|
ever want to consider the possibility of faster than light travel.
|
|
Though I do not expect you to be so adamant about the idea, I do hope
|
|
that you see it as a definite possibility with some desirable outcomes.
|
|
If nothing else, I hope that I have at least educated you to some extent
|
|
on the problems involved when considering the effects of relativity on
|
|
faster than light travel.
|
|
|
|
|
|
|
|
|
|
Jason Hinson
|
|
|
|
|
|
-Jay
|
|
|