The Cosmic Landscape Page 6

  The Fine Structure Constant

  The various equations and formulas of physics contain a variety of different numerical constants. Some of these constants are numbers derived from pure mathematics. An example is the number 3.14159… , better known by its Greek name, π. We know the value of π to billions of decimal places, not by measuring it, but from its purely mathematical definition: π is defined to be the ratio of the circumference of a circle to its diameter. Other purely mathematical numbers, such as the square root of 2 and the number called e, may also be computed to endless precision if anyone were motivated to do it.

  But other numbers that appear in physics equations have no special mathematical significance. We might call them empirical numbers. An example that is important in nuclear physics is the ratio of the proton mass to the neutron mass. Its numerical value is known to seven figures—1.001378. The next digit cannot be obtained by mathematics alone. One must go into the lab and measure it. The most fundamental of these empirical numbers are crowned with the title “constants of nature.” The fine structure constant is one of the most important constants of nature.13 Like π, the fine structure is named for a Greek letter, in this case α (alpha). It is often approximated by the fraction 1/137. Its precise value is known to a limited number of decimal places—0.007297351—but it is, nonetheless, one of the most accurately known physical constants.

  The fine structure constant is an example of a quantity that physicists call coupling constants. Each coupling constant is associated with one of the basic events—the vertex diagrams—of quantum field theory. The coupling constant is a measure of the strength, or potency, of the event depicted by the vertex. In QED the sole vertex diagram is the emission of a photon by an electron. Let’s consider more closely what happens when a photon is emitted.

  One might begin by asking what determines the precise point at which an electron, as it moves through space-time, emits a photon. The answer is that nothing does—physics at the microscopic level is capricious. Nature has a random element that drove Einstein in his later years to distraction. He protested, “God does not play dice.”14 But whether Einstein liked it or not, nature is not deterministic. Nature has an element of randomness that is built into the Laws of Physics at the deepest level. Even Einstein couldn’t change that. But if nature is not deterministic, neither is it completely chaotic. Here is where the principles of quantum mechanics enter. Unlike Newtonian physics, quantum mechanics never predicts the future in terms of the past. Instead, it provides very precise rules for computing the probability for various alternative outcomes of an experiment. Just as there is no way to predict the final location of a photon that has gone through a slit, there is also no way to predict exactly where along its path an electron will launch a photon or where another electron may absorb it. But there is a definite probability for these events.

  The operation of a television screen provides a good illustration of such probabilities. The light coming from a TV screen is composed of photons that are created when electrons strike the screen. The electrons are ejected from an electrode at the rear of the set and are guided to the screen by electric and magnetic fields. But not every electron that hits the screen emits a photon. Some do. Most don’t. Roughly speaking the probability that any particular electron will radiate a quantum of light is given by the fine structure constant α. In other words, only one lucky electron out of 137 emits a photon. That is the meaning of α: it is the probability that an electron, as it moves along its trajectory, will capriciously emit a photon.

  Feynman didn’t just draw pictures. He invented a set of rules for working out the probabilities of the complex processes depicted in the pictures. In other words, he discovered a precise mathematical calculus that predicts the probabilities for any process in terms of the simplest events—propagators and vertices. The probabilities for all processes in nature ultimately trace back to coupling constants like a.

  The fine structure constant also controls the strength of the exchange diagrams, which in turn, determine the strength of electric forces among charged particles. It controls how tightly the atomic nucleus pulls the electrons toward it. As a consequence it determines how big the atom is, how fast the electrons move in their orbits, and ultimately controls the forces between different atoms that allow them to form molecules. But as important as it is, we don’t know why its value is 0.007297351 and not something else. The Laws of Physics that were discovered during the twentieth century are very accurate and useful, but the underlying origin of those laws remains a mystery.

  The theory of this simplified world of electrons, photons, and point nuclei is Quantum Electrodynamics, and Feynman’s version of it was incredibly successful. Using his methods the properties of electrons, positrons, and photons were understood with astonishing accuracy. Moreover, if the simplified version of the nucleus was added, the properties of the simplest atom—hydrogen—could also be calculated to incredible precision. In 1965 Feynman, Julian Schwinger, and the Japanese physicist Sin-Itero Tomanaga won the Nobel Prize for their work on Quantum Electrodynamics. That was Act I.

  If Act I was theater in the small, with only two characters, the play became an epic with hundreds of players in Act II. New particles were discovered throughout the 1950s and 1960s that eventually required an unruly cast including electrons, neutrinos, muons, tau particles, up-quarks, down-quarks, strange-quarks, charmed-quarks, bottom-quarks, top-quarks, photons, gluons, W- and Z-bosons, Higgs bosons, and a good deal more. Don’t ever believe anyone who tells you that elementary-particle physics is elegant. This hodgepodge of particle names reflects an equally unwieldy jumble of masses, electric charges, spins, and other properties. But as messy as it is, we know how to describe it with enormous precision. The Standard Model is the name of the mathematical structure—a particular quantum field theory—that describes the modern theory of elementary particles. Although it is far more complicated than Quantum Electrodynamics, Feynman’s methods are so powerful that, once again, they can be used to express everything in terms of simple pictures. The principles are exactly the same as those of QED: everything is built out of propagators, vertex diagrams, and coupling constants. But there are new actors and whole new plot lines, including one called QCD.

  Quantum Chromodynamics

  Many years ago I was invited to a famous university to give a series of lectures on a brand-new subject called Quantum Chromodynamics (QCD). As I was walking through the halls of the Physics Department on my way to the first lecture, I overheard a pair of graduate students discussing the title. One, who was looking at the lecture announcement on the bulletin board, said, “What’s this all about? What is Quantum Chromodynamics?” The other fellow thought for a moment, then looked up and said, “Hmmm, it must be a new way to use quantum mechanics to develop your photographs.”

  Quantum Chromodynamics has nothing to do with photography or even light. QCD is the modern version of nuclear physics. Conventional nuclear physics begins with protons and neutrons (nucleons), but QCD goes a step deeper. It’s been known for forty years that nucleons are not elementary particles. They are more like atoms or molecules except on a much smaller scale. If one could look into a proton with a sufficiently powerful microscope, one would see three quarks tied together by a string of particles called gluons. The theory of quarks and gluons—QCD—is a more complicated theory than QED, and I won’t really be able to do it justice in a few pages. But the basic facts are not too difficult. Here is the cast of characters.

  The Six Quarks

  First there are the quarks: there are six distinct types of them. In order to distinguish one from another, physicists gave them meaningless, whimsical names: up-quark, down-quark, strange-quark, charmed-quark, bottom-quark, and top-quark, or more concisely, u-, d-, s-, c-, b-, and t-quarks. There is, of course, nothing stranger about the strange-quark or more charming about the charmed-quark, but the silly names give them a bit of personality.

  Why are there six quark types and not four or
two? Who knows? A theory with four or two types of quarks is every bit as consistent as one with six types. What we do know is that the mathematics of the Standard Model requires the quarks to come in pairs—up with down, charmed with strange, and top with bottom. But the reason for the threefold replication of the simplest theory—one with only up- and down-quarks—is a complete mystery. To make matters worse, only the up- and down-quarks play any essential role in ordinary nuclei.15 If QCD were an engineering project, the rest of the quarks would be considered an extravagant squandering of resources.

  Quarks are in some ways similar to electrons, although somewhat heavier, and they have peculiar electric charges. In order to have a basis for comparison, the charge of the proton is traditionally taken to be one (+1). The electron’s charge is equally big but opposite in sign (–1). Quarks, on the other hand, have charges that are fractions of the proton charge. In particular, the charges of the u-, c-, and t-quarks are positive like the proton’s but only two-thirds as big (2/3). The d-, s-, and b-quarks have negative charges equal to one-third the electron charge (–1/3).

  Both protons and neutrons contain three quarks. In the case of the proton, there are two u-quarks and a single d-quark. Adding up the electric charges of these three quarks, the result is the charge of the proton:

  The neutron is very similar to the proton, the difference being that the up- and down-quarks are interchanged. Thus, the neutron contains two d-quarks and one u-quark. Again adding the three charges, we find the neutron has (as expected) no electric charge:

  What would happen if we tried to build a proton, or something like a proton, by substituting a strange-quark for the down-quark? Such objects do exist—they are called strange particles—but they don’t exist anywhere except in physics laboratories. Even in such laboratories strange particles are fleeting occurrences that last for no more than a tiny fraction of a second before disintegrating by a kind of radioactivity. The same is true of particles containing charmed-, bottom-, or top-quarks. Only up- and down-quarks can be assembled into stable, long-lasting objects. As I said, if the strange-, charmed-, bottom-, and top-quarks were suddenly removed from the list of elementary particles, hardly anyone would notice.

  What about quarks that go backward in time? Like electrons, each kind of quark has its antiparticle. They can be assembled into antiprotons and antineutrons. At one time very early in the history of the universe, when the temperature was billions of degrees, antinucleons were about as abundant as ordinary nucleons. But as things cooled, the antiparticles almost entirely disappeared, leaving only the ordinary protons and neutrons to form the nuclei of atoms.

  The Gluon

  Nucleons are like tiny atoms made of quarks. But quarks alone would be powerless to bind themselves into nucleons. Like the atom, they require another ingredient to create the forces of attraction that “glue” them together. In the case of the atom, we know exactly what the glue is. The atom is held from flying apart by photons continuously being juggled back and forth between electrons and nuclei. But the force generated by photon exchange is far too weak to bind quarks into the tightly knit structure of a nucleon (remember that nucleons are 100,000 times smaller than atoms). Another particle with more potent properties is needed to pull quarks together that tightly. That particle is the aptly named gluon.

  The basic events in any quantum field theory are always the same: the emission of particles by other particles. The Feynman diagrams describing these events always have the same form: vertex diagrams shaped like the letter Y. The basic vertex diagram for QCD looks exactly like the photon-emission vertex with a quark replacing the electron and a gluon taking the place of the photon.

  Not surprisingly, the origin of the forces that bind quarks into protons and neutrons is the exchange of gluons. But there are two big differences between QED and QCD. The first is a quantitative difference: the numerical constant governing the emission of gluons is not as small as the fine structure constant. It is called αQCD (alpha-QCD) and is about one hundred times larger than the fine structure constant. This is the reason that the force between quarks is much stronger than the electric force that acts in the atom. QCD is sometimes called the theory of the strong interactions.

  The second difference is qualitative. It causes gluons to become a sticky substance that always reminds me of the tale of the tar baby. Once upon a time, according to southern folklore, Brer Rabbit16 came upon a tar baby sitting in the road, minding his own business. Brer Rabbit said, “Mornin’.” The tar baby said nothing. Brer Rabbit got offended. One thing led to another, and soon an altercation ensued—Brer Rabbit got mad and punched tar baby, but that was a huge mistake. Stuck with his fist in the tar, Brer Rabbit pulled and pulled, but the tar just stretched and pulled him back. As hard as he struggled to free him himself, tar baby just wouldn’t let go.

  Why the tar baby story? Because quarks are miniature tar babies, but only to other quarks. They are permanently glued together by a tarlike, stringy substance made of gluons. The origin of this strange behavior is one extra vertex that has no analog in QED. Any electrically charged particle can emit a photon. But photons themselves are not charged. They are electrically neutral and, therefore, will not emit another photon. In this respect gluons are very different from photons. The laws of QCD require a vertex in which a gluon splits into two gluons, each proceeding on one of the paths of the fork.

  This is the big difference between QCD and QED that makes QCD a far more complicated theory than its electric counterpart. Among other things, it implies that gluons can exchange gluons and bind into objects called glueballs—particles with no quarks or electrons at all. In fact gluons don’t stick together only in pairs. They can form long chains of stringy glue. Earlier I likened the electrons in an atom to balls being swung on ropes. In that case the rope was entirely metaphorical. But in the case of quarks, the strings holding them together are quite real. They are strings of gluons strung out between the quarks. In fact when a quark is forcibly ejected from a nucleon, a long string of gluons forms and eventually prevents the quark’s escape.

  The Weak Interactions

  If you are getting weary of learning particle physics, I don’t blame you. It’s too complicated with too many things to remember. There are too many particles to keep track of and no good reason that we know of for their existence. QCD and QED hardly exhaust the pieces that make up the Standard Model. The whole thing is a very far cry from the elegant simple theory that physicists expected to find “at the bottom of it all.” It’s a good deal more like zoology or botany. But that’s just the way it is. We can’t change the facts.

  I am going to guide you through one more piece of the Standard Model: that part known as the weak interactions. Like QED and QCD the weak interactions play an important role in explaining our own existence, although the reasons are subtler and won’t become clear until later chapters.

  The history of the weak interactions dates back to the very end of the nineteenth century, when the French physicist Antoine-Henri Becquerel discovered radioactivity. Becquerel’s discovery preceded J. J. Thomson’s discovery of the electron by one year.

  Radioactivity comes in three different kinds, called alpha, beta, and gamma. They correspond to three very different phenomena, only one of which (beta) has to do with the weak interactions. Today we know that the beta rays coming from Becquerel’s uranium sample were actually electrons emitted by neutrons in the uranium nucleus. Upon emitting the electron, the neutron immediately turns into a proton.

  Nothing in either QED or QCD explains how a neutron can emit an electron and become a proton. The simplest explanation, which may already have occurred to you, is that there is an additional vertex diagram to add to our list of fundamental events. The vertex would involve an initial neutron coming to a fork in the road, whereupon a proton would continue on one path and an electron on the other. But this is not the correct explanation. The fact is that a new character is about to make its entrance—the neutrino. What Becquere
l didn’t know was that another particle flew off when the neutron decayed, namely, the antiparticle of the ghostly neutrino.

  The Neutrino

  The neutrino is similar to the electron but without electric charge. Think of it as an electron that has lost its electrical properties. In a way the relationship between the electron and the neutrino is similar to that between the proton and neutron.

  What’s left of the neutrino then? It has a tiny bit of mass but not much else. It doesn’t emit photons. It doesn’t emit gluons. This means it has none of the forces acting on it that electrically charged particles or quarks experience. It doesn’t bind itself to other particles to form more complex objects. It hardly does anything. In fact the neutrino is such a loner that it will pass through light-years of lead without even getting deflected. But it’s not a complete zero. To understand how the neutrino gets into the act, yet another actor has to be introduced—the W-boson.

  The W-Boson

  For the moment don’t worry about the word boson. For now, it simply denotes another particle, similar in its properties to the photon or gluon but electrically charged. It comes in two versions, the positively charged W and the negatively charged W. They are, of course, each other’s antiparticles.

  The W-boson is the key to the neutrino’s activities. Not only can electrons and quarks emit W-bosons—so, too, can the neutrino. Here is a (partial) list of the W-boson’s activities:

  Electrons emit W-bosons and turn into neutrinos

  Up-quarks emit W-bosons and become down-quarks

  Up-quarks emit W-bosons and become strange-quarks

  Charmed-quarks emit W-bosons and become strange-quarks

  Top-quarks emit W-bosons and become bottom-quarks