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Introduction General considerations Occurrence and importance The electromagnetic spectrum Generation of electromagnetic radiation Properties and behaviour Cosmic background electromagnetic radiation Effect of gravitation The greenhouse effect of the atmosphere
Forms of electromagnetic radiation Radio waves Microwaves
Relation between electricity and magnetism As early as 1760 the Swiss-born mathematician Leonhard Euler suggested that the same ether that propagates light is responsible for electrical phenomena. In comparison with both mechanics and optics, however, the science of electricity was slow to develop. Magnetism was the one science that made progress in the Middle Ages, following the introduction from China into the West of the magnetic compass, but electromagnetism played little part in the scientific revolution of the 17th century. It was, however, the only part of physics in which very significant progress was made during the 18th century. By the end of that century the
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Visible radiation
laws of electrostatics—the behaviour of charged particles at rest—were
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Ultraviolet radiation
well known, and the stage was set for the development of the elaborate
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X-rays
mathematical description first made by the French mathematician
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light
Siméon-Denis Poisson. There was no apparent connection of electricity
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luminescence
with magnetism, except that magnetic poles, like electric charges, attract
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James Clerk Maxwell
and repel with an inverse-square law force.
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photoelectric effect
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photovoltaic effect
Following the discoveries in electrochemistry (the chemical effects of
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ultraviolet radiation
electrical current) by the Italian investigators Luigi Galvani, a physiologist,
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X-ray
and Alessandro Volta, a physicist, interest turned to current electricity. A
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Herschel
Infrared radiation
Gamma rays
Historical survey Development of the classical radiation theory Development of the quantum theory of radiation
search was made by the Danish physicist Hans Christian Ørsted for some connection between electric currents and magnetism, and during the winter of 1819–20 he observed the effect of a current on a magnetic needle. Members of the French Academy learned about Ørsted’s discovery in September 1820, and several of them began to investigate it further. Of these, the most thorough in both experiment and theory was the physicist André-Marie Ampère, who may be called the father of electrodynamics. The list of four fundamental empirical laws of electricity and magnetism was made complete with the discovery of electromagnetic induction by Faraday in 1831. In brief, a change in magnetic flux through a conducting circuit produces a current in the circuit. The observation that the induced current is in a direction to oppose the change that produces it, now known as Lenz’s law, was formulated by a Russian-born physicist, Heinrich Friedrich Emil Lenz, in 1834. When the laws were put into mathematical form by Maxwell, the law of induction was generalized to include the production of electric force in space, independent of actual conducting circuits, but was otherwise unchanged. On the other hand, Ampère’s law describing the magnetic effect of a current required amendment in order to be consistent with the conservation of charge (the total charge must remain constant) in the presence of changing electric fields, and Maxwell introduced the idea of “displacement current” to make the set of equations logically consistent. As a result, he found on combining the equations that he arrived at a wave equation, according to which transverse electric and
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magnetic disturbances were propagated with a velocity that could be
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calculated from electrical measurements. These measurements were
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available to Maxwell, having been made in 1856 by the German physicists
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Rudolph Hermann Arndt Kohlrausch and Wilhelm Eduard Weber, and his
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calculation gave him a result that was the same, within the limits of error,
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as the speed of light in vacuum. It was the coincidence of this value with the velocity of the waves predicted by his theory that convinced Maxwell of the electromagnetic nature of light. Melba Phillips Hellmut Fritzsche
The electromagnetic wave and field concept Faraday introduced the concept of field and of field lines of force that exist outside material bodies. As he explained it, the region around and outside a magnet or an electric charge contains a field that describes at any location the force experienced by another small magnet or charge placed there. The lines of force around a magnet can be made visible by iron filings sprayed on a paper that is held over the magnet. The concept of field, specifying as it does a certain possible action or force at any location in space, was the key to understanding electromagnetic phenomena. It should be mentioned parenthetically that the field concept also plays (in varied forms) a pivotal role in modern theories of particles and forces. Besides introducing this important concept of electric and magnetic field lines of force, Faraday had the extraordinary insight that electrical and
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magnetic actions are not transmitted instantaneously but after a certain lag in time, which increases with distance from the source. Moreover, he
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realized the connection between magnetism and light after observing that
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a substance such as glass can rotate the plane of polarization of light in the presence of a magnetic field. This remarkable phenomenon is known
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as the Faraday effect.
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As noted above, Maxwell formulated a quantitative theory that linked the fundamental phenomena of electricity and magnetism and that predicted electromagnetic waves propagating with a speed, which, as well as one could determine at that time, was identical with the speed of light. He concluded his paper “On the Physical Lines of Force” (1861–62) by saying that electricity may be disseminated through space with properties
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identical with those of light. In 1864 Maxwell wrote that the numerical factor linking the electrostatic and the magnetic units was very close to the speed of light and that these results “show that light and magnetism are affections of the same substance, and that light is an electromagnetic disturbance propagated through the field according to [his] electromagnetic laws.” What more was needed to convince the scientific community that the mystery of light was solved and the phenomena of electricity and magnetism were unified in a grand theory? Why did it take 25 more years for Maxwell’s theory to be accepted? For one, there was little direct proof of the new theory. Furthermore, Maxwell not only had adopted a complicated formalism but also explained its various aspects by unusual mechanical concepts. Even though he stated that all such phrases are to be considered as illustrative and not as explanatory, the French mathematician Henri Poincaré remarked in 1899 that the “complicated structure” which Maxwell attributed to the ether “rendered his system
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strange and unattractive.”
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The ideas of Faraday and Maxwell that the field of force has a physical
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existence in space independent of material media were too new to be
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accepted without direct proof. On the Continent, particularly in Germany,
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matters were further complicated by the success of Carl Friedrich Gauss and Wilhelm Eduard Weber in developing a potential field theory for the
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phenomena of electrostatics and magnetostatics and their continuing effort to extend this formalism to electrodynamics.
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It is difficult in hindsight to appreciate the reluctance to accept the
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Faraday–Maxwell theory. The impasse was finally removed by Hertz’s
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work. In 1884 Hertz derived Maxwell’s theory by a new method and put its fundamental equations into their present-day form. In so doing, he clarified the equations, making the symmetry of electric and magnetic fields apparent. The German physicist Arnold Sommerfeld spoke for most of his learned colleagues when, after reading Hertz’s paper, he remarked, “the shades fell from my eyes,” and admitted that he understood electromagnetic theory for the first time. Four years later, Hertz made a second major contribution: he succeeded in generating electromagnetic radiation of radio and microwave frequencies, measuring their speed by a
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standing-wave method and proving that these waves have the properties
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of reflection, diffraction, refraction, and interference common to light. He
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showed that such electromagnetic waves can be polarized, that the
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electric and magnetic fields oscillate in directions that are mutually
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perpendicular and transverse to the direction of motion, and that their
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velocity is the same as the speed of light, as predicted by Maxwell’s theory. Hertz’s ingenious experiments not only settled the theoretical misconceptions in favour of Maxwell’s electromagnetic field theory but also opened the way for building transmitters, antennas, coaxial cables, and detectors for radio-frequency electromagnetic radiation. In 1896 Marconi received the first patent for wireless telegraphy, and in 1901 he achieved transatlantic radio communication. The Faraday–Maxwell–Hertz theory of electromagnetic radiation, which is commonly referred to as Maxwell’s theory, makes no reference to a medium in which the electromagnetic waves propagate. A wave of this kind is produced, for example, when a line of charges is moved back and forth along the line. Moving charges represent an electric current. In this back-and-forth motion, the current flows in one direction and then in another. As a consequence of this reversal of current direction, the magnetic field around the current (discovered by Ørsted and Ampère) has to reverse its direction. The time-varying magnetic field produces perpendicular to it a time-varying electric field, as discovered by Faraday (Faraday’s law of induction). These time-varying electric and magnetic fields spread out from their source, the oscillating current, at the speed of light in free space. The oscillating current in this discussion is the oscillating current in a transmitting antenna, and the time-varying electric and magnetic fields that are perpendicular to one another propagate at the speed of light and constitute an electromagnetic wave. Its frequency is that of the oscillating charges in the antenna. Once generated, it is selfpropagating because a time-varying electric field produces a time-varying magnetic field, and vice versa. Electromagnetic radiation travels through space by itself. The belief in the existence of an ether medium, however, was at the time of Maxwell as strong as at the time of Plato and Aristotle. It was impossible to visualize ether because contradictory properties had
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to be attributed to it in order to explain the phenomena known at any given time. In his article ETHER in the ninth edition of the Encyclopædia Britannica, Maxwell described the vast expanse of the substance, some of it possibly even inside the planets, carried along with them or passing through them as the “water of the sea passes through the meshes of a net when it is towed along by a boat.” If one believes in the ether, it is, of course, of fundamental importance to measure the speed of its motion or the effect of its motion on the speed of light. One does not know the absolute velocity of the ether, but, as Earth moves through its orbit around the Sun, there should be a difference in ether velocity along and perpendicular to Earth’s motion equal to its speed. If such is the case, the velocity of light and of any other electromagnetic radiation along and perpendicular to Earth’s motion should, predicted Maxwell, differ by a fraction that is equal to the square of the ratio of Earth’s velocity to that of light. This fraction is one part in 100 million. Michelson set out to measure this effect and, as noted above, designed for this purpose the interferometer sketched in Figure 4. If it is assumed that the interferometer is turned so that half beam A is oriented parallel to Earth’s motion and half beam B is perpendicular to it, then the idea of using this instrument for measuring the effect of the ether motion is best explained by Michelson’s words to his children: Two beams of light race against each other, like two swimmers, one struggling upstream and back, while the other, covering the same distance, just crosses the river and returns. The second swimmer will always win, if there is any current in the river.
An improved version of the interferometer, in which each half beam traversed its path eight times before both were reunited for interference, was built in 1887 by Michelson in collaboration with Morley. A heavy sandstone slab holding the interferometer was floated on a pool of mercury to allow rotation without vibration. Michelson and Morley could not detect any difference in the two light velocities parallel and perpendicular to Earth’s motion to an accuracy of one part in four billion. This negative result did not, however, shatter the belief in the existence of an ether because the ether could possibly be dragged along with Earth and thus be stationary around the Michelson-Morley apparatus. Hertz’s formulation of Maxwell’s theory made it clear that no medium of any sort was needed for the propagation of electromagnetic radiation. In spite of this, ether-drift experiments continued to be conducted until about the mid-1920s. All such tests confirmed Michelson’s negative results, and scientists finally came to accept the idea that no ether medium was needed for electromagnetic radiation.
Speed of light Much effort has been devoted to measuring the speed of light, beginning with the aforementioned work of Rømer in 1676. Rømer noticed that the orbital period of Jupiter’s first moon, Io, is apparently slowed as Earth and Jupiter move away from each other. The eclipses of Io occur later than expected when Jupiter is at its most remote position. This effect is understandable if light requires a finite time to reach Earth from Jupiter. From this effect, Rømer calculated the time required for light to travel from the Sun to Earth as 11 minutes. In 1728 James Bradley, an English astronomer, determined the speed of light from the apparent orbital motion of stars that is produced by Earth’s orbital motion. He computed the time for light to reach Earth from the Sun as 8 minutes 12 seconds. The first terrestrial measurements were made in 1849 by Fizeau and a year later by Foucault. Michelson improved on Foucault’s method and obtained an accuracy of one part in 100,000. Any measurement of velocity requires, however, a definition of the measure of length and of time. Current techniques allow a determination of the velocity of electromagnetic radiation to a substantially higher degree of precision than permitted by the unit of length that scientists had applied earlier. In 1983 the value of the speed of light was fixed at exactly 299,792,458 metres per second, and this value was adopted as a new standard. As a consequence, the metre was redefined as the length of the path traveled by light in a vacuum over a time interval of 1/299,792,458 of a second. Furthermore, the second—the international unit of time—has been based on the frequency of electromagnetic radiation emitted by a cesium-133 atom.
Development of the quantum theory of radiation After a long struggle electromagnetic wave theory had triumphed. The Faraday-Maxwell-Hertz theory of electromagnetic radiation seemed to be able to explain all phenomena of light, electricity, and magnetism. The understanding of these phenomena enabled one to produce electromagnetic radiation of many different frequencies which had never been observed before and which opened a world of new opportunities. No one suspected that the conceptional foundations of physics were about to change again.
Radiation laws and Planck’s light quanta The quantum theory of absorption and emission of radiation announced in 1900 by Planck ushered in the era of modern physics. He proposed that all material systems can absorb or give off electromagnetic radiation only in “chunks” of energy, quanta E, and that these are proportional to the frequency of that radiation E = h. (The constant of proportionality h is, as noted above, called Planck’s constant.) Planck was led to this radically new insight by trying to explain the puzzling observation of the amount of electromagnetic radiation emitted by a hot body and, in particular, the dependence of the intensity of this incandescent radiation on temperature and on frequency. The quantitative aspects of the incandescent radiation constitute the radiation laws. The Austrian physicist Josef Stefan found in 1879 that the total radiation energy per unit time emitted by a heated surface per unit area increases as the fourth power of its absolute temperature T (Kelvin scale). This means that the Sun’s surface, which is at T = 6,000 K, radiates per unit area (6,000/300)4 = 204 = 160,000 times more electromagnetic energy than does the same area of Earth’s surface, which is taken to be T = 300 K. In 1889 another Austrian physicist, Ludwig Boltzmann, used the second law of thermodynamics to derive this temperature dependence for an ideal substance that emits and absorbs all frequencies. Such an object that absorbs light of all colours looks black, and so was called a blackbody. The Stefan-Boltzmann law is written in quantitative form W = T 4, where W is the radiant energy emitted per second and per unit area and the constant of proportionality is = 0.136 calories per metre2-secondK4 . The wavelength or frequency distribution of blackbody radiation was studied in the 1890s by Wilhelm Wien of Germany. It was his idea to use as a good approximation for the ideal blackbody an oven with a small hole. Any radiation that enters the small hole is scattered and reflected from the inner walls of the oven so often that nearly all incoming radiation is absorbed and the chance of some of it finding its way out of the hole again can be made exceedingly small. The radiation coming out of this hole is then very close to the equilibrium blackbody electromagnetic radiation corresponding to the oven temperature. Wien found that the radiative energy dW per wavelength interval d has a maximum at a certain wavelength m and that the maximum shifts to shorter wavelengths as the temperature T is increased, as illustrated in Figure 8. He found that the product mT is an absolute constant: mT = 0.2898 cm-K.
Figure 8: Electromagnetic energy dW emitted per unit area and per second into a wavelength interval, d =one angstrom, by a blackbody at various temperatures between 3,000 and 6,000 K as a function of wavelength. The range of visible light is between the vertical dashed lines. Encyclopædia Britannica, Inc.
Wien’s law of the shift of the radiative power maximum to higher frequencies as the temperature is raised expresses in a quantitative form commonplace observations. Warm objects emit infrared radiation, which is felt by the skin; near T = 950 K a dull red glow can be observed; and the colour brightens to orange and yellow as the temperature is raised. The tungsten filament of a lightbulb is T = 2,500 K hot and emits bright light, yet the peak of its spectrum is still in the infrared according to Wien’s law. The peak shifts to the visible yellow when the temperature is T = 6,000 K, like that of the Sun’s surface. It was the shape of Wien’s radiative energy distribution as a function of frequency that Planck tried to understand. The decrease of the radiation output at low frequency had already been explained by Lord Rayleigh in terms of the decrease, with lowering frequency, in the number of modes of electromagnetic radiation per frequency interval. Rayleigh, following the principle of equipartition of energy, assumed that all possible frequency modes could radiate with equal probability. Since the number of frequency modes per frequency interval continues to increase without limit with the square of the frequency, Rayleigh’s formula predicted an ever-increasing amount of radiation of higher frequencies instead of the observed maximum and subsequent fall in radiative power. A possible way out of this dilemma was to deny the high-frequency modes an equal chance to radiate. To achieve this, Planck postulated that the radiators or oscillators can emit electromagnetic radiation only in finite amounts of energy of size E = h. At a given temperature T, there is then not enough thermal energy available to create and emit many large radiation quanta h . More large energy quanta h can be emitted, however, when the temperature is raised. Quantitatively the probability of emitting at temperature T an electromagnetic energy quantum h is
where k is Boltzmann’s constant, well known from thermodynamics. With c = , Planck’s radiation law then becomes
This is in superb agreement with Wien’s experimental results when the value of h is properly chosen to fit the results. It should be pointed out that Planck’s quantization refers to the oscillators of the blackbody or of heated substances. These oscillators of frequency are incapable of absorbing or emitting electromagnetic radiation except in energy chunks of size h . To explain quantized absorption and emission of radiation, it seemed sufficient to quantize only the energy levels of mechanical systems. Planck did not mean to say that electromagnetic radiation itself is quantized, or, as Einstein later put it, “The sale of beer in pint bottles does not imply that beer exists only in indivisible pint portions.” The idea that electromagnetic radiation itself is quantized was proposed by Einstein in 1905, as described in the subsequent section.
Photoelectric effect Hertz discovered the photoelectric effect (1887) quite by accident while generating electromagnetic waves and observing their propagation. His transmitter and receiver were induction coils with spark gaps. He measured the electromagnetic field strength by the maximum length of the spark of his detector. In order to observe this more accurately, he occasionally enclosed the spark gap of the receiver in a dark case. In doing so, he observed that the spark was always smaller with the case than without it. He concluded, correctly, that the light from the transmitter spark affected the electrical arcing of the receiver. He used a quartz prism to disperse the light of the transmitter spark and found that the ultraviolet part of the light spectrum was responsible for enhancing the receiver spark. Hertz took this discovery seriously because the only other effect of light on electrical phenomena known at that time was the increase in electrical conductance of the element selenium with light exposure.
Explanation of the photoelectric effect. Encyclopædia Britannica, Inc.
A year after Hertz’s discovery, it became clear that ultraviolet radiation caused the emission of negatively charged particles from solid surfaces. Thomson’s discovery of electrons (1897) and his ensuing measurement of the ratio m/e (the ratio of mass to charge) finally made it possible to identify the negative particles emitted in the photoelectric effect with electrons. This was accomplished in 1899 by J.J. Thomson and independently by Philipp Lenard, one of Hertz’s students. Lenard discovered that for a given frequency of ultraviolet radiation the maximum kinetic energy of the emitted electrons depends on the metal used rather than on the intensity of the ultraviolet light. The light intensity increases the number but not the energy of emitted electrons. Moreover, he found that for each metal there is a minimum light frequency that is needed to induce the emission of electrons. Light of a frequency lower than this minimum frequency has no effect regardless of its intensity. In 1905 Einstein published an article entitled “On a Heuristic Point of View about the Creation and Conversion of Light.” Here he deduced that electromagnetic radiation itself consists of “particles” of energy h . He arrived at this conclusion by using a simple theoretical argument comparing the change in entropy of an ideal gas caused by an isothermal change in volume with the change in entropy of an equivalent volume change for electromagnetic radiation in accordance with Wien’s or Planck’s radiation law. This derivation and comparison made no references to substances and oscillators. At the end of this paper, Einstein concluded that if electromagnetic radiation is quantized, the absorption processes are thus quantized too, yielding an elegant explanation of the threshold energies and the intensity dependence of the photoelectric effect. He then predicted that the kinetic energy of the electrons emitted in the photoelectric effect increases with light frequency proportional to h − P, where P is “the amount of work that the electron must produce on leaving the body.” This quantity P, now called work function, depends on the kind of solid used, as discovered by Lenard. LEARN MORE
Einstein’s path-breaking idea of light quanta was not widely accepted by his peers. Planck himself stated as late as 1913 in his recommendation for admitting Einstein to the Prussian Academy of Sciences “the fact that he [Einstein] may occasionally have missed the mark in his speculations, as, for example, with his hypothesis of light quanta, ought not to be held too much against him, for it is impossible to introduce new ideas, even in the exact sciences, without taking risks.” In order to explain a quantized absorption and emission of radiation by matter, it seemed sufficient to quantize the possible energy states in matter. The resistance against quantizing the energies of electromagnetic radiation itself is understandable in view of the incredible success of Maxwell’s theory of electromagnetic radiation and the overwhelming evidence of the wave nature of this radiation. Moreover, a formal similarity of two theoretical expressions, in Einstein’s 1905 paper, of the entropy of an ideal gas and the entropy of electromagnetic radiation was deemed insufficient evidence for a real correspondence. Einstein’s prediction of the linear increase of the kinetic energy of photoemitted electrons with the frequency of light, h − P, was verified by Arthur Llewelyn Hughes, Owen Williams Richardson, and Karl Taylor Compton in 1912. In 1916 Robert Andrews Millikan measured both the frequency of the light and the kinetic energy of the electron emitted by the photoelectric effect and obtained a value for Planck’s constant h in close agreement with the value that had been arrived at by fitting Planck’s radiation law to the blackbody spectrum obtained by Wien.
Compton effect Convincing evidence of the particle nature of electromagnetic radiation was found in 1922 by the American physicist Arthur Holly Compton. While investigating the scattering of X-rays, he observed that such rays lose some of their energy in the scattering process and emerge with slightly decreased frequency. This energy loss increases with the scattering angle, , measured from the direction of an unscattered X-ray. This socalled Compton effect can be explained, according to classical mechanics, as an elastic collision of two particles comparable to the collision of two billiard balls. In this case, an X-ray photon of energy h and momentum h /c collides with an electron at rest. The recoiling electron was observed and measured by Compton and Alfred W. Simon in a Wilson cloud chamber. If one calculates the result of such an elastic collision by using the relativistic formulas for the energy and momentum of the scattered electron, one finds that the wavelength of an X-ray after ( ¢) and before () the scattering event differs by ¢ − = ( h/mc)(1 − cos ). Here m is the rest mass of the electron and h/mc is called Compton wavelength. It has the value 0.0243 angstrom. The energy h of a photon of this wavelength is equal to the rest mass energy mc2 of an electron. One might argue that electrons in atoms are not at rest, but their kinetic energy is very small compared with that of energetic X-rays and can be disregarded in deriving Compton’s equation.
Resonance absorption and recoil During the mid-1800s the German physicist Gustav Robert Kirchhoff observed that atoms and molecules emit and absorb electromagnetic radiation at characteristic frequencies and that the emission and absorption frequencies are the same for a given substance. Such resonance absorption should, strictly speaking, not occur if one applies the photon picture due to the following argument. Since energy and momentum have to be conserved in the emission process, the atom recoils to the left as the photon is emitted to the right, just as a cannon recoils backward when a shot is fired. Because the recoiling atom carries off some kinetic recoil energy ER, the emitted photon energy is less than the energy difference of the atomic energy states by the amount ER. When a photon is absorbed by an atom, the momentum of the photon is likewise transmitted to the atom, thereby giving it a kinetic recoil energy ER. The absorbing photon must therefore supply not only the energy difference of the atomic energy states but the additional amount ER as well. Accordingly, resonance absorption should not occur because the emitted photon is missing 2ER to accomplish it. Nevertheless, ever since Kirchhoff’s finding, investigators have observed resonance absorption for electronic transitions in atoms and molecules. This is because for visible light the recoil energy ER is very small compared with the natural energy uncertainty of atomic emission and absorption processes. The situation is, however, quite different for the emission and absorption of gamma-ray photons by nuclei. The recoil energy ER is more than 10,000 times as large for gamma-ray photons as for photons of visible light, and the nuclear energy transitions are much more sharply defined because their lifetime can be one million times longer than for electronic energy transitions. The particle nature of photons therefore prevents resonance absorption of gamma-ray photons by free nuclei. In 1958 the German physicist Rudolf Ludwig Mössbauer discovered that recoilless gamma-ray resonance absorption is, nevertheless, possible if the emitting as well as the absorbing nuclei are embedded in a solid. In this case, there is a strong probability that the recoil momentum during absorption and emission of the gamma photon is taken up by the whole solid (or more precisely by its entire lattice). This then reduces the recoil energy to nearly zero and thus allows resonance absorption to occur even for gamma rays.
Wave-particle duality How can electromagnetic radiation behave like a particle in some cases while exhibiting wavelike properties that produce the interference and diffraction phenomena in others? This paradoxical behaviour came to be known as the wave-particle duality. Bohr rejected the idea of light quanta, and he searched for ways to explain the Compton effect and the photoelectric effect by arguing that the momentum and energy conservation laws need to be satisfied only statistically in the time average. In 1923 he stated that the hypothesis of light quanta excludes, in principle, the possibility of a rational definition of the concepts of frequency and wavelength that are essential for explaining interference. The following year the conceptual foundations of physics were shaken by the French physicist Louis de Broglie, who suggested in his doctoral dissertation that the wave-particle duality applies not only to light but to a particle as well. De Broglie proposed that any object has wavelike properties. In particular, he showed that the orbits and energies of the hydrogen atom, as described by Bohr’s atomic model, correspond to the condition that the circumference of any orbit precisely matches an integral number of wavelengths of the matter waves of electrons. Any particle such as an electron moving with a momentum p has, according to de Broglie, a wavelength = h/p. This idea required a conceptual revolution of mechanics, which led to the wave and quantum mechanics of Erwin Schrödinger, Werner Heisenberg, and Max Born. De Broglie’s idea of the wavelike behaviour of particles was quickly verified experimentally. In 1927 Clinton Joseph Davisson and Lester Germer of the United States observed diffraction and hence interference of electron waves by the regular arrangement of atoms in a crystal of nickel. That same year S. Kikuchi of Japan obtained an electron diffraction pattern by shooting electrons with an energy of 68 keV through a thin mica plate and recording the resultant diffraction pattern on a photographic plate. The observed pattern corresponded to electron waves having the wavelength predicted by de Broglie. The diffraction effects of helium atoms were found in 1930, and neutron diffraction has today become an indispensable tool for determining the magnetic and atomic structure of materials. The interference pattern that results when a radiation front hits two slits in an opaque screen is often cited to explain the conceptual difficulty of the wave-particle duality. Consider an opaque screen with two openings A and B, called a double slit, and a photographic plate or a projection screen, as shown in Figure 9. A parallel wave with a wavelength passing through the double slit will produce the intensity pattern on the plate or screen as shown at the right of the figure. The intensity is greatest at the centre. It falls to zero at all locations x0, where the distances to the openings A and B differ by odd-number multiples of a half wavelength, as, for instance, /2, 3/2, and 5/2. The condition for such destructive interference is the same as for Michelson’s interferometer illustrated in Figure 4. Whereas a half-transparent mirror in Figure 4 divides the amplitude of each wave train in half, the division in Figure 9 through openings A and B is spatial. The latter is called division of wave front. Constructive interference or intensity maxima are observed on the screen at all positions whose distances from A and B differ by zero or an integer multiple of . This is the wave interpretation of the observed double-slit interference pattern.
Figure 9: Double-slit interference. Encyclopædia Britannica, Inc.
The description of photons is necessarily different because a particle can obviously only pass through opening A or alternatively through opening B. Yet, no interference pattern is observed when either A or B is closed. Both A and B must be open simultaneously. It was thought for a time that one photon passing through A might interfere with another photon passing through B. That possibility was ruled out after the British physicist Geoffrey Taylor demonstrated in 1909 that the same interference pattern can be recorded on a photographic plate even when the light intensity is so feeble that only one photon is present in the apparatus at any one time. Another attempt to understand the dual nature of electromagnetic radiation was to identify the photon with a wave train whose length is equal to its coherence length c, where is the coherence time, or the lifetime of an atomic transition from a higher to a lower internal atomic energy state, and c is the light velocity. This is the same as envisioning the photon to be an elongated wave packet, or “needle radiation.” Again, the term “photon” had a different meaning for different scientists, and wave nature and quantum structure remained incompatible. It was time to find a theory of electromagnetic radiation that would fuse the wave theory and the particle theory. Such a fusion was accomplished by quantum electrodynamics (QED).
Quantum electrodynamics Among the most convincing phenomena that demonstrate the quantum nature of light are the following. As the intensity of light is dimmed further and further, one can see individual quanta being registered in light detectors. If the eyes were about 10 times more sensitive, one would perceive the individual light pulses of fainter and fainter light sources as fewer and fewer flashes of equal intensity. Moreover, a movie has been made of the buildup of a two-slit interference pattern by individual photons, such as shown in Figure 9. Photons are particles, but they behave differently from ordinary particles like billiard balls. The rules of their behaviour and their interaction with electrons and other charged particles, as well as the interactions of charged particles with one another, constitute QED. Photons are created by perturbations in the motions of electrons and other charged particles; in reverse, photons can disappear and thereby create a pair of oppositely charged particles, usually a particle and its antiparticle (e.g., an electron and a positron). A description of this intimate interaction between charged particles and electromagnetic radiation requires a theory that includes both quantum mechanics and special relativity. The foundations of such a theory, known as relativistic quantum mechanics, were laid beginning in 1929 by Paul A.M. Dirac, Heisenberg, and Wolfgang Pauli. The discussion that follows explains in brief the principal conceptual elements of QED. Further information on the subject can be found in subatomic particle: The development of modern theory and quantum mechanics. Many phenomena in nature do not depend on the reference scale of scientific measurements. For instance, in electromagnetism the difference in electrical potentials is relevant but not its absolute magnitude. During the 1920s, even before the emergence of quantum mechanics, the German physicist Hermann Weyl discussed the problem of constructing physical theories that are independent of certain reference bases or absolute magnitudes of certain parameters not only locally but everywhere in space. He called this property “Eichinvarianz,” which is the conceptual origin of the term “gauge invariance” that plays a crucial role in all modern quantum field theories. In quantum mechanics all observable quantities are calculated from socalled wave functions, which are complex mathematical functions that include a phase factor. The absolute magnitude of this phase is irrelevant for the observable quantities calculated from these wave functions; hence, the theory describing, for example, the motion of an electron should be the same when the phase of its wave function is changed everywhere in space. This requirement of phase invariance, or gauge invariance, is equivalent to demanding that the total charge is conserved and does not disappear in physical processes or interactions. Experimentally one does indeed observe that charge is conserved in nature. It turns out that a relativistic quantum theory of charged particles can be made gauge invariant if the interaction is mediated by a massless and chargeless entity which has all the properties of photons. Coulomb’s law of the force between charged particles can be derived from this theory, and the photon can be viewed as a “messenger” particle that conveys the electromagnetic force between charged particles of matter. In this theory, Maxwell’s equations for electric and magnetic fields are quantized. The range of a force produced by a particle with nonzero mass is its Compton wavelength h/mc, which for electrons is about 2 × 10−10 cm. Since this length is large compared with distances over which stronger nuclear forces act, QED is a very precise theory for electrons. Despite the conceptual elegance of the QED theory, it proved difficult to calculate the outcome of specific physical situations through its application. Richard P. Feynman and, independently, Julian S. Schwinger and Freeman Dyson of the United States and Tomonaga Shin’ichirō of Japan showed in 1948 that one could calculate the effects of the interactions as a power series in which the coupling constant is called the fine structure constant and has a value close to 1/137. A serious practical difficulty arose when each term in the series, which had to be summed to obtain the value of an observed quantity, turned out to be infinitely large. In short, the results of the calculations were meaningless. It was eventually found, however, that these divergences could be avoided by introducing “renormalized” couplings and particle masses, an idea conceived by the Dutch physicist Hendrik A. Kramers. Just as a ship moving through water has an enhanced mass due to the fluid that it drags along, so will an electron dragging along and interacting with its own field have a different mass and charge than it would without it. By adding appropriate electromagnetic components to the bare mass and charge— that is, by using renormalized quantities—the disturbing infinities could be removed from the theory. Using this method of renormalization and the perturbation theory, Feynman developed an elegant form for calculating the likelihood of observing processes that are related to the interaction of electromagnetic radiation with matter to any desired degree of accuracy. For example, the passage of an electron or a photon through the double slit illustrated in Figure 9 will, in this QED formalism, produce the observed interference pattern on a photographic plate because of the superposition of all the possible paths these particles can take through the slits. The success of unifying electricity, magnetism, and light into one theory of electromagnetism and then with the interaction of charged particles into the theory of quantum electrodynamics suggests the possibility of understanding all the forces in nature (gravitational, electromagnetic, weak nuclear, and strong nuclear) as manifestations of a grand unified theory (GUT). The first step in this direction was taken during the 1960s by Abdus Salam, Steven Weinberg, and Sheldon Glashow, who formulated the electroweak theory, which combines the electromagnetic force and the weak nuclear force. This theory predicted that the weak nuclear force is transmitted between particles of matter by three messenger particles designated W+, W−, and Z, much in the way that the electromagnetic force is conveyed by photons. The three new particles were discovered in 1983 during experiments at the European Organization for Nuclear Research (CERN), a large accelerator laboratory near Geneva. This triumph for the electroweak theory represented another stepping stone toward a deeper understanding of the forces and interactions that yield the multitude of physical phenomena in the universe.
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Microwaves
LEARN MORE in these related articles: radiation: Types of radiation …type constitutes the spectrum of electromagnetic radiation that includes radio waves, microwaves, infrared rays, visible light, ultraviolet rays, X rays, and gamma rays, as well as the neutrino (see below). These are all characterized by zero mass when (theoretically) at rest. The second type includes such particles as electrons, protons,… READ MORE
radiation: The field concept …propagate as what are called electromagnetic waves. In an assumed ideal free space (without intrusion from other fields or forces of any kind, devoid of matter, and, thus, in effect without any intrusions, demarcations, or boundaries), such waves propagate with the speed of light in the so-called transverse electromagnetic mode—one… READ MORE
spectroscopy: General principles …absorption or the emission of electromagnetic radiation as molecules undergo changes from one quantized energy state to another. The mechanisms involved are similar to those observed for atoms but are more complicated. The additional complexities are due to interactions of the various nuclei with each other and with the electrons,… READ MORE
spectroscopy: Basic features of electromagnetic radiation Electromagnetic radiation is composed of oscillating electric and magnetic fields that have the ability to transfer energy through space. The energy propagates as a wave, such that the crests and troughs of the wave move READ MORE
principles of physical science: Ensuing developments and their ramifications …his description of light as electromagnetic waves, brought the problem to a state of crisis. It became clear that if light waves were propagated in the hypothetical ether that filled all space and provided an embodiment of Newton’s absolute frame (see below), it would not be logically consistent to accept… READ MORE
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