Einstein's two theories of relativity have shown us that when things move very fast or when objects get massive, the universe exhibits very strange properties. The same is also true of the microscopic world of quantum interactions. The deeper we delve into the macrocosm and the microcosm, the further we get away from the things that make sense to us in our everyday world.
At the heart of relativity theory is the idea that what you experience is real for you but not necessarily for someone else—it depends on your frame of reference. This can also be said of the quantum world, but with less certainty. Because what we find within the framework of quantum mechanics is that events are based on probability and not certainty. And the probable outcome of any event often depends on what you're looking for.
In “The Dual Nature of Light,” I discussed the wave/particle duality of light and touched on some aspects of the quantum. This section will extend that discussion by inquiring into just why energy has to come in chunks, or quanta, and how this would lead in the next section into the bizarre nature of quantum interactions where everything is so uncertain. We'll also look at the key theories of some of the great physicists who helped to define this weird quantum landscape. Next stop, the quantum zone.
There are many physicists who have contributed to the development of quantum mechanics. For our purposes we're going to look at the handful whose theories laid the foundation that others would build upon. Here's a list of those that we'll be taking a look at. If I omit any, it's not because their contributions weren't significant, it's only because I can only cover so much as an introduction to this huge body of material.
A few years before the outbreak of World War I, the Belgian industrialist Ernest Solvay (1838-1922) sponsored the first of a series of international physics meetings in Brussels called the Solvay Conference. Attendance at these meetings was by special invitation, and participants, usually limited to around 30, were asked to concentrate on a pre-arranged topic. The first five meetings held between 1911 and 1927 chronicled the development of twentieth-century physics. The 1927 gathering was devoted to quantum theory and attended by nine of the most brilliant theoretical physicists. Each of the nine would eventually be awarded the Nobel Prize for their contributions.
These six physicists along with three others—Wolfgang Pauli, Max Born, and Paul Dirac—were all together in 1927 at the Solvay Conference. It was during this conference that the essential concepts of quantum theory were formulated. What I will do for the rest of this section is to discuss each of the founding fathers listed above and explain some of the basic concepts of their contributions. Let's begin with a little overview of just what quantum mechanics is all about.
A quantum leap is a discontinuous transition between quantum states. What this means is that an electron in one energy level in an atom jumps instantly into another energy level, emitting or absorbing energy as it does so. There is no in-between state, and it doesn't take any time for the leap to occur. The leaps also occur at random, selecting from the options available to the quantum entity in accordance with the strict rules of probability. So a quantum leap is a sudden change in a system that occurs on a very small scale and is made at random.
What is quantum mechanics? Well, essentially it's the mechanics of quantized things. Okay, so what does that mean? In physics, mechanics is not about fixing your car, but is the explanation of the way things work in terms of energy, forces, and motion. And anything that is quantized is simply expressed in multiples of some small measurable unit. As you already know, before the turn of the century, the way things worked was explained by Newtonian mechanics or classical physics. And the central feature of Newtonian mechanics was that everything was continuous; things flowed smoothly through space; energy could come in an infinite range of amounts; light undulated in a continuous wave; there was no minimum amount of anything.
Quantum mechanics changed all that. Now energy, light, force, and motion all came to be quantized. For something to be quantized, you can't have just any old amount; you can only have multiples of certain minimum quantities. Quantum mechanics meant that all the qualities of subatomic things, and by extension, all things, were precisely quantifiable. Nature revealed herself to be somewhat grainy or jerky, jumping from one quantum amount to the other, never traversing the area in between. This leads to an uneasy uncertainty about what is going on between those quantum states, or to put it into a popular phrase, quantum leaps. In fact, as it turns out, there is no way of knowing the exact state of things between quantum states. In our perception (and that is a key ingredient), there is no transition between quantum states. You can have one or two or three units of energy or momentum or light or force or matter or whatever, but there is no such thing as one and one-half or two and three-quarters units.
An example of this might help you understand. Imagine that a child is jumping up the stairs. A quantum leap is the transition from one state to the next state, the same as a child jumping from the first stair to the second stair. Depending on the amount of energy she has, she can also jump up to the third stair, the fourth, or the sixth. But she can't jump in between the stairs and land safely.
Everything in the quantum mechanical universe, which is the universe we live in, happens in quantum leaps. The uncertainty associated with these leaps will be explained when we get to Werner Heisenberg in “Chunks of Uncertainty.” The important point I want to mention is that all of this comes into acute focus when we actually set out to measure things as small as atoms and try to describe them in language of typical Newtonian systems. Lost? Don't worry, it will become quantumly clear shortly.
Excerpted from The Complete Idiot's Guide to Theories of the Universe © 2001 by Gary F. Moring. All rights reserved including the right of reproduction in whole or in part in any form. Used by arrangement with Alpha Books, a member of Penguin Group (USA) Inc.