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Lawrence Krauss - The Greatest Story Ever Told--So Far

Page 9

by Why Are We Here (pdf)


  original interference pattern to the originally expected pattern—with

  a bright region behind each of the two slits, just as if one were

  shooting billiard balls or bullets and not waves toward the screen.

  In other words, in attempting to verify your classical intuition,

  you changed the behavior of the electrons. Or, as more commonly

  asserted in quantum mechanics, measurement of a system can alter

  its behavior.

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  One of the many seemingly impossible aspects of quantum

  mechanics is that there is no experiment you can perform that

  demonstrates that in the absence of measurement the electrons

  behave in a sensible classical way.

  This strange wavelike nature of objects that would otherwise be

  considered to be particles—such as electrons—is mathematically

  expressed by assigning to each electron a “wave function,” which

  describes the probability of finding that electron at any given point.

  If the wave function takes on non-zero values at many different

  points, then the electron’s position cannot be isolated in advance of

  accurately measuring its position. In other words there is a non-zero

  probability that the electron is not actually localized at just some

  specific point in space in advance of making a measurement.

  While you might imagine that this is a simple problem of not

  having access to all the information we need to locate the particle

  until we make a measurement, Young’s double-slit experiment,

  when updated for electrons, demonstrated that this is most certainly

  not the case. Any “sensible” classical picture of what is happening

  between measurements is inconsistent with the data.

  • • •

  The strange behavior of electrons was not the first evidence that the

  microscopic world could not be understood by intuitive classical

  logic. Once again, in keeping with the revolutionary developments in

  our understanding of nature since Plato, the discovery of quantum

  mechanics began with a consideration of light.

  Recall that if we perform Young’s double-slit experiment in

  Plato’s cave with light rays, we get the interference pattern on the

  wall that Young discovered, which demonstrated that light was

  indeed a wave. So far, so good. However, if the light source is

  sufficiently weak, then if we try to detect the light as it passes

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  through either of the slits, something strange happens. We will

  measure the light beam as traveling through one slit or the other,

  not both. And as with electrons, in this case the pattern on the wall

  will now change, looking as it would if light were particles and not

  waves.

  In fact, light also behaves like both a particle and a wave,

  depending on the circumstances under which you choose to

  measure it. The individual particles of light, which we now call

  photons, were first labeled quanta by the German theoretical

  physicist Max Planck, who suggested in 1900 that light might be

  emitted or absorbed in some smallest bundle (although the idea that

  light might come in discrete packets had earlier been floated by the

  great Ludwig Boltzmann in 1877).

  I have come to admire Planck even more as I have learned about

  his life. Like Einstein, he was an unpaid lecturer and was not offered

  an academic position after completing his thesis. During this time he

  spent his career trying to understand the nature of heat and

  developed several important pieces of work in thermodynamics. Five

  years after defending his thesis, he was finally offered a university

  position, and he then quickly rose up the ranks and became a full

  professor at the prestigious University of Berlin in 1892.

  In 1894 he turned to the question of the nature of light emitted by

  hot objects, in part driven by commercial considerations (the first

  example I know of in the story I have been telling where

  fundamental physics was commercially motivated). He was

  commissioned to explore how to get the maximum amount of light

  out of the newly invented lightbulbs while using the minimum

  amount of energy.

  We all know that when we heat up an oven element it first glows

  red, and then, when it gets hotter, it begins to glow blue. But why?

  Surprisingly, the conventional approaches to this problem were

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  unable to reproduce these observations. After struggling with the

  problem for six years, Planck presented a revolutionary proposal

  about radiation that agreed with observations.

  Originally there was nothing revolutionary about his derivation,

  but within two months he had revised his analysis to accommodate

  ideas about what was happening at a fundamental level. In a quote

  that has endeared him to me since I first read it, he wrote that his

  new approach arose as “an act of despair. . . . I was ready to sacrifice

  any of my previous convictions about physics.”

  This reflects to me the fundamental quality that makes the

  scientific process so effective, and which is so clearly represented in

  the rise of quantum mechanics. “Previous convictions” are just

  convictions waiting to be overturned—by empirical data, if

  necessary. We throw out cherished old notions like yesterday’s

  newspaper if they don’t work. And they didn’t work in explaining the

  nature of radiation emitted by matter.

  Planck derived his law of radiation from the fundamental

  assumption that light, which was a wave, nevertheless was emitted

  only in “packets” of some minimum energy—proportional to the

  frequency of the radiation in question. He labeled the constant that

  related the energy to the frequency the “action quantum,” which is

  now called Planck’s constant.

  This may not sound so revolutionary, and as Faraday did with

  electric fields, Planck viewed his assumption as merely a formal

  mathematical crutch to aid in his analysis. He later stated, “Actually I

  did not think much about it.” Nevertheless, this proposal that light

  was emitted in particle-like packets is clearly difficult to reconcile

  with the classical picture of light as a wave. The energy carried by a

  wave is simply related to the magnitude of its oscillations, which can

  change continuously from zero. However, according to Planck, the

  amount of energy that could be emitted in a light wave of a given

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  frequency had an absolute minimum. This minimum was termed an

  “energy quantum.”

  Planck subsequently tried to develop a classical physical

  understanding of these energy quanta, but failed—causing him, as he

  put it, “much trouble.” Still, unlike a number of his colleagues, he

  recognized that the universe didn’t exist to make his life easier.

  Referring to the physicist and astronomer Sir James Jeans, who was

  unwilling to give up classical notions in the face of the evidence

  provided by radiation, Planck stated, “I am unable to understand

  Jeans’s stubbornness—he is an example of a theoretician as should

  never be existing, the same as Hegel was for philosophy. So m
uch

  the worse for the facts if they don’t fit.” (Just to be clear, in case

  readers are moved to write me letters, Planck cast this aspersion on

  Hegel, not me!)

  Planck later became friends with another physicist who had let

  the facts drive him toward another revolutionary idea, Albert

  Einstein. In 1914, when Planck had become dean at Berlin

  University, he established a new professorship for Einstein there. At

  first Planck could not accept Einstein’s remarkable proposal—made

  in 1905, the same year in which he proposed the Special Theory of

  Relativity—that not only was light emitted by matter in quantum

  packets, but that light beams themselves existed as bunches of these

  quanta—that light itself was made up of particle-like objects, which

  we now call photons.

  Einstein was driven to this proposal to explain a phenomenon

  called the photoelectric effect, discovered by Philipp Lenard in 1902

  —a physicist whose anti-Semitism would later play a key role in

  delaying Einstein’s Nobel Prize, and ensuring, curiously, if perhaps

  poetically, that it would be not for Einstein’s work on relativity, but

  rather on the photoelectric effect. In the photoelectric effect, light

  shining on a metal surface can knock electrons out of atoms and

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  produce a current. However, no matter how intense the light, no

  electrons would be emitted if the frequency of the light was below

  some threshold. The moment the frequency was raised above that

  threshold, a photoelectric current would be generated.

  Einstein realized, correctly, that this could be explained if the light

  came in minimum packets of energy, with the energy proportional

  to the frequency of light—as Planck had postulated for light emitted

  by matter. In this case, only light with frequencies greater than some

  threshold frequency could contain quanta energetic enough to kick

  electrons out of atoms.

  Planck could accept the quantized emission of radiation as

  explaining his radiation law, but the assumption that light itself was

  quantum-like (i.e., particle-like) was so foreign to the common

  understanding of light as an electromagnetic wave that Planck

  balked. Only six years later, at a conference in Belgium, the Solvay

  Conference, which later became famous, was Einstein finally able to

  convince Planck that the classical picture of light had to be

  abandoned, and that quanta—aka photons—were real.

  Einstein was also the first to actually use a fact that he later

  denounced in his famous statement deriding the probabilistic

  essence of quantum mechanics and reality: “God does not play dice

  with the universe.” He showed that if atoms spontaneously (i.e.,

  without direct cause) absorb and emit finite packets of radiation as

  electrons jump between discrete energy levels in atoms, then he

  could rederive the Planck radiation law.

  It is ironic that Einstein, who started the quantum revolution but

  never joined it, was also perhaps the first to use probabilistic

  arguments to describe the nature of matter—a strategy that the

  subsequent physicists who turned quantum mechanics into a full

  theory would place front and center. As a result, Einstein was one of

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  the first physicists to demonstrate that God does play dice with the

  universe.

  To take the analogy a little further, Einstein was one of the first

  physicists to demonstrate that the classical notion of causation

  begins to break down in the quantum realm. Many people have

  taken exception to my proposal that the universe needed no cause

  but simply popped into existence from nothing. Yet this is precisely

  what happens with the light you are using to read this page.

  Electrons in hot atoms emit photons—photons that didn’t exist

  before they were emitted—which are emitted spontaneously and

  without specific cause. Why is it that we have grown at least

  somewhat comfortable with the idea that photons can be created

  from nothing without cause, but not whole universes?

  The realization that electromagnetic waves were also particles

  began a quantum revolution that would change everything about the

  way we view nature. To be a particle and a wave at the same time is

  impossible classically—as should be clear from the earlier discussion

  in this chapter—but it is possible in the quantum world. As should

  also be clear, this was just the beginning.

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  C h a p t e r 7

  A

  U N I V E R S E

  S T R A N G E R

  T H A N F I C T I O N

  Therefore do not throw away your confidence, which has a great

  reward.

  —HEBREWS 10:35

  Conventional wisdom might suggest that physicists love to

  invent crazy esoterica to explain the universe around us, either

  because we have nothing better to do, or because we are particularly

  perverse. However, as the unveiling of the quantum world

  demonstrates, more often than not it is nature that drags us

  scientists, kicking and screaming, away from the safety of what is

  familiar.

  Nevertheless, to say that the pioneers who pushed us forward into

  the quantum world lacked confidence would be a profound

  misstatement. The voyage they embarked upon was without

  precedent and without guides. The world they were entering defied

  all common sense, and classical logic, and they had to be prepared at

  every turn for a change in the rules.

  Imagine taking a road trip to another country, where the

  inhabitants all speak a foreign language, and the laws are not based

  on experiences that compare to any you have ever had in your life.

  Moreover imagine the traffic signals are hidden and can change

  from place to place. Then you can get a sense of where the young

  Turks who overturned our understanding of nature in the first half

  of the twentieth century were heading.

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  The analogy between exploring strange new quantum worlds and

  embarking on a trek through a new landscape may seemed strained,

  but exactly such a relationship between the two was paralleled in the

  life of none other than Werner Heisenberg, one of the founders of

  quantum mechanics, who once reminisced about an evening in the

  summer of 1925 on the island of Helgoland, a lovely oasis in the

  North Sea, when he realized he had discovered the theory:

  It was almost three o’clock in the morning before the final result of

  my computations lay before me. The energy principle had held for

  all the terms, and I could no longer doubt the mathematical

  consistency and coherence of the kind of quantum mechanics to

  which my calculations pointed. At first, I was deeply alarmed. I

  had the feeling that, through the surface of atomic phenomena, I

  was looking at a strangely beautiful interior and felt almost giddy

  at the thought that I now had to probe this wealth of

  mathematical structures nature had so generously spread out

  before me. I was far too excited to sleep, and so, as a new day

  dawned,
I made for the southern tip of the island, where I had

  been longing to climb a rock jutting out into the sea. I now did so

  without too much trouble and waited for the sun to rise.

  Heisenberg, fresh from obtaining his PhD, had moved to the

  distinguished German university in Göttingen to work with Max

  Born to try to come up with a consistent theory of quantum

  mechanics (a term first used in the paper “On Quantum Mechanics”

  by Born in 1924). However, spring hay fever had laid Heisenberg

  low, and he escaped the green countryside for the sea. There, he

  polished off his ideas about the quantum behavior of atoms and sent

  it off to Born, who submitted it for publication.

  You may be familiar with Heisenberg’s name, not least because of

  the famous principle associated with it. The Heisenberg uncertainty

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  principle has gained a New Age aura, providing fuel for many a

  charlatan to take advantage of people for whom quantum mechanics

  seems to offer hope of a world where any dream, no matter how

  outlandish, is realizable.

  Other familiar names, Bohr, Schrödinger, Dirac, and later

  Feynman and Dyson, each made great leaps into the unknown. But

  they weren’t alone. Physics is a collaborative discipline. Too often

  science stories are written as if the protagonists had a sudden Aha!

  experience alone late at night. Heisenberg had been working on

  quantum mechanics for several years with his PhD supervisor, the

  brilliant German scientist Arnold Sommerfeld (whose students

  would win four Nobel Prizes, and whose postdoctoral research

  assistants would win three), and later with Born (who was finally

  recognized with a Nobel almost thirty years later), as well as a young

  colleague, Pascual Jordan. Every major triumph we celebrate with a

  name and a prize is accompanied by a legion of hardworking, often

  less heralded, individuals, each of whom moves forward the line of

  scrimmage by a little bit. Baby steps are the norm, not the exception.

  The most remarkable leaps into the unknown are often not fully

  appreciated, even by their developers, until much later. Thus

  Einstein, for example, never trusted his beautiful General Relativity

  enough to believe its prediction that the universe cannot be static

  but must be expanding or contracting—until observations

  demonstrated the expansion. And the world didn’t stand on its head

 

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