Physics

The Photoelectric Effect

The photoelectric effect refers to the phenomenon where electrons are emitted from a material's surface when it is exposed to light. This effect provided evidence for the particle-like behavior of light, as described by Albert Einstein in 1905. The energy of the emitted electrons is directly proportional to the frequency of the incident light, rather than its intensity.

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12 Key excerpts on "The Photoelectric Effect"

  • Light
    eBook - ePub
    Planck’s original theory was concerned only with the interaction of radiation and matter. He hoped that it would involve only minor modifications of the classical electromagnetic theory of light and the classical electron theory of matter. This expectation was not fulfilled and it became necessary to modify the theory of light to include the fact that energy of the radiation field which represents a beam of light can change only by an integral number of quanta. It is also necessary to assume that an atom can change its energy only by discrete amounts, and hence that atoms can exist only in certain states separated by finite differences of energy. Nothing in the classical laws of electromagnetism, which are based on experiments with static fields or alternating fields of low frequency, would lead us to expect this effect.
    The quantum theory thus becomes both a theory of radiation and a theory of matter instead of being merely a special hypothesis concerning their interaction. The theory is a connected whole and we cannot deal with a section of the theory concerning radiation without referring extensively to atomic structure. In this chapter we discuss the experimental basis of the quantum theory, giving special prominence to experiments on light and on electromagnetic radiation of shorter wavelength. The order is chosen for convenience of exposition and does not follow the historical order.
    17.2. The Photo-electric Effect.
    It is found that electrons are ejected from the surfaces of metals by light and by radiation of shorter wavelength (X-rays and y-rays). If the radiation is able to penetrate the substance, electrons in the interior may be removed from their equilibrium positions. In this paragraph we are concerned with the emission of electrons from surfaces, and we shall call this the photo-electric effect, although, strictly, it should be called the surface photo-electric effect. The number and velocities of electrons emitted have been measured for different metals and for different wavelengths. Fig. 17.1 shows in a diagrammatic way a simple apparatus. Fig. 17.2 shows a more elaborate experiment in which the surface of the metal is freshly cut in vacuo immediately before the measurements are made. The results of the experiments in which monochromatic light is incident normally upon the surface of a metal may be summarized as follows:
    Fig. 17.1.—Photo-electric effect. Diagram of simplified apparatus
  • Physics in the Modern World
    17

    ELECTRONS AND PHOTONS

    Publisher Summary

    This chapter explains the phenomenon of photoelectric effect. The Photoelectric Effect exhibits a frequency limit, and if the frequency is too low, the effect cannot be produced even if the light intensity is made very large. The chapter describes the qualitative aspects of The Photoelectric Effect. According to classical electromagnetic theory, the energy transferred by a wave is proportional to its intensity and does not depend on the frequency. The chapter discusses the fundamental principles governing the interaction of radiation and matter at the atomic level. It illustrates the interference pattern produced by electrons. Electrons have wave properties and exhibit interference effects. Electron wavelengths tend to be considerably smaller than the wavelengths of visible light. The chapter explains the accumulation of single-photon events on a diffraction screen. A photon can exhibit both wavelike and particlelike properties. The chapter discusses the concept of wave packet and describes quantum theory.
    At about the time that Einstein was formulating his ideas concerning space and time which were to lead to the development of relativity theory, scientists were also investigating the nature of light and electrons. Electrons were known to be particles and light was acknowledged to be a wave phenomenon.
    We all have rather clear intuitive ideas about waves and particles. We know that a wave is an extended propagating disturbance in a medium. We know that a particle is an object that can be located at a particular point in space whereas a wave cannot. And we have come to accept the existence of atomic particles–electrons, protons, and neutrons. What could be simpler? A wave is a wave, and a particle is a particle; the distinction is clear.

    17-1 The Photoelectric Effect

    The Ejection of Electrons from Metals

    But it is not all this simple. As the 20th century began, scientists were confronted with new questions concerning waves and particles. It had been discovered, for example, that if a piece of clean zinc is exposed to ultraviolet (UV) radiation, the zinc acquires a positive charge. The radiation can carry no charge to the zinc, so this result must mean that electrons (the carriers of negative charge) are literally knocked off the zinc by the action of the UV radiation (Fig. 17-1 ). The removal of electrons causes the zinc to become charged positively. This phenomenon is called the photoelectric effect and the ejected electrons are called photoelectrons.
  • The Manual of Photography
    • Elizabeth Allen, Sophie Triantaphillidou(Authors)
    • 2012(Publication Date)
    • Routledge
      (Publisher)
    The existence of a threshold frequency for each metal can be explained by the work function of the material; the minimum photon energy capable of causing The Photoelectric Effect will eject the electron with zero kinetic energy. The photoelectric equation becomes:
    where v0 is the threshold frequency.
    The existence of light in quantities called photons provided solutions to the problems raised by The Photoelectric Effect that classical wave theory had failed to explain. Einstein’s work was a theoretical treatment and caused much controversy at the time, appearing as it did to contradict the wave theory of light based upon Maxwell’s equations for electromagnetic waves and, perhaps more fundamentally, the idea that energy was not something that could be divided into infinitely small units, i.e. continuous in nature.
    It was not until 1915, with the work of Robert Andrews Millikan, that Einstein’s theory was shown to be correct: Einstein had predicted that the energy of the ejected electrons would increase linearly with the frequency of the radiating light and Millikan was able to demonstrate this linear relationship experimentally. The work on The Photoelectric Effect had turned the world of physics on its head, resulting in the introduction of the concept of the duality of light: that it exhibited the characteristics of both waves and particles in different circumstances. Wavee particle duality would eventually be extended to other elementary particles such as the electron.

    THE PHOTON

    A photon is a single quantum of energy that can only exist at the speed of light. It is the fundamental element carrying all electromagnetic radiation. It is indivisible, it cannot be split into smaller units, and is a stable, elementary particle. Photons differ from other elementary particles such as electrons in that they have zero mass or electric charge and consist purely of energy. When many photons are present, for example in a light beam, their numbers are so large that the inherent discontinuity or granularity of the light beam disappears and it appears as a continuous phenomenon. The photon can exhibit wave-like behaviour, resulting in phenomena such as refraction or diffraction, described earlier in this chapter. It also behaves as a particle when interacting with matter at a subatomic level, exchanging energy in discrete amounts. The amount of energy E (from Planck’s Law) exchanged during such an interaction is dependent on the frequency of light, and is known as the photon energy
  • Quantum Mechanics for Electrical Engineers
    1.1 ) according to:
    FIGURE 1.1 The Photoelectric Effect. (a) If certain materials are irradiated with light, electrons within the material can absorb energy and escape the material. (b) It was observed that the KE of the escaping electron depends on the frequency of the light.
    where, ϕ , the work function, is the minimum energy that the particle needs to leave the material.
    Planck postulated that energy is contained in discrete packets called quanta, and this energy is related to frequency through what is now known as Planck’s constant, where h = 6.625 × 10−34 J·s,
    (1.1)
    Einstein suggested that the energy of the light is contained in discrete wave packets called photons. This theory explains why the electrons absorbed specific levels of energy dictated by the frequency of the incoming light and became known as The Photoelectric Effect.
    1.1.2 Wave–Particle Duality
    Another famous experiment suggested that particles have wave properties. When a source of particles is accelerated toward a screen with a single opening, a detection board on the other side shows the particles centered on a position right behind the opening as expected (Fig. 1.2 a). However, if the experiment is repeated with two openings, the pattern on the detection board suggests points of constructive and destructive interference, similar to an electromagnetic or acoustic wave (Fig. 1.2 b).
    FIGURE 1.2 The wave nature of particles. (a) If a source of particles is directed at a screen with one opening, the distribution on the other side is centered at the opening, as expected. (b) If the screen contains two openings, points of constructive and destructive interference are observed, suggesting a wave.
    Based on observations like these, Louis De Broglie postulated that matter has wave-like qualities. According to De Broglie, the momentum of a particle is given by:
  • Atoms, Radiation, and Radiation Protection
    • James S. Bogard, Darryl J. Downing, Robert L. Coleman, Keith F. Eckerman, James E. Turner(Authors)
    • 2022(Publication Date)
    • Wiley-VCH
      (Publisher)
    Raleigh scattering of a photon results from the combined, coherent action of an atom as a whole. The scattering angle is usually very small. There is no appreciable loss of energy by the photon to the atom, which, however, does “recoil” enough to conserve momentum. We shall not consider Thomson or Raleigh scattering further.
    The principal mechanisms of energy deposition by photons in matter are photoelectric absorption, Compton scattering, pair production, and photonuclear reactions. We treat these processes in some detail.

    8.2 Photoelectric Effect

    The ejection of electrons from a surface as a result of light absorption is called The Photoelectric Effect. The arrangement in Fig. 8.1 can be used to study this process experimentally. Monochromatic light passes into an evacuated glass tube through a quartz window (which allows ultraviolet light to be used) and strikes an electrode 1 causing photoelectrons to be ejected. Electrode 1 can be made of a metal to be studied or have its surface covered with such a metal. The current I that flows during illumination can be measured as a function of the variable potential difference V21 applied between the two electrodes, 1 and 2, of the tube. Curves (a) and (b) represent data obtained at two different intensities of the incident light. With the surface illuminated, there will be some current even with V21 = 0. When V21 is made positive and increased, the efficiency of collecting photoelectrons at electrode 2 increases; the current rises to a plateau when all of the electrons are being collected. The ratio of the plateau currents is equal to the relative light intensity used for curves (a) and (b).
    Figure 8.1
    Experiment on photoelectric effect. With electrode 1 illuminated with monochromatic light of constant intensity, the current I is measured as a function of the potential difference V21 between electrodes 2 and 1. Curves (a) and (b) represent data at two different intensities of the incident light.
    When the polarity of the potential difference is reversed (V21 < 0), photoelectrons ejected from the illuminated electrode 1 now experience an attractive force back toward it. Making V21 more negative allows only the most energetic photoelectrons to reach electrode 2, thus causing the current I to decrease. Independently of the light intensity, the photoelectric current drops to zero when the reversed potential difference reaches a magnitude V0 , called the stopping potential. The potential energy eV0 , where e is the magnitude of the electronic charge, is equal to the maximum kinetic energy, Tmax
  • Introduction to Quantum Mechanics 1
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    Introduction to Quantum Mechanics 1

    Thermal Radiation and Experimental Facts of the Quantization of Matter

    • Ibrahima Sakho(Author)
    • 2019(Publication Date)
    • Wiley-ISTE
      (Publisher)
    Figure 2.7 .
    A freshly etched zinc plate amalgamated with mercury is placed on a negatively charged electroscope. The plate is lighted by a halogen lamp with quartz crystal envelope (UV-rich light). Rapid discharge of the electroscope can be noted, which proves that electrons are removed from the lighted zinc plate: this is referred to as photoelectric effect.
    Figure 2.7.
    Experimental setup for the observation of The Photoelectric Effect
    If light passes through a glass plate that fully absorbs ultraviolet radiations, the electroscope does not discharge; this proves that the removal of electrons due to photoelectric effect requires short wavelength light. By definition, p-hotoelectric effect is the extraction of electrons from a metal exposed to adequate (UV-rich) light. Electrons removed by light are known as photoelectrons.

    2.2.2. Interpretation, photon energy

    The Photoelectric Effect is explained within Einstein’s photon theory. Light is a set of particles called photons. Therefore, The Photoelectric Effect results from a collision between a photon of light radiation and an electron of the lighted metal. Two outcomes are possible:
    Figure 2.8.
    Interpretation of The Photoelectric Effect: photonelectron collision
    • – if photon energy is not sufficient (long wavelength light), the photon rebounds off the metal and the electron is not removed (Figure 2.8(a) );
    • – if photon energy is sufficient (short wavelength light), the photon is absorbed by the metal, which absorbs all its energy: one electron is then removed and set in motion with maximal speed υ (Figure 2.8(b) ).
    In conclusion, The Photoelectric Effect supports the particle nature of light.

    Box 2.2. Hertz (1857–1894)

    Heinrich Rudolf Hertz
  • Surfaces and Interfaces of Electronic Materials
    • Leonard J. Brillson(Author)
    • 2012(Publication Date)
    • Wiley-VCH
      (Publisher)

    Chapter 7

    Photoemission Spectroscopy

    7.1 The Photoelectric Effect

    Photoelectron spectroscopy is one of the most widely used surface science techniques. Its utility stems from the discrete or quantized nature of light, first explained by Albert Einstein in 1905 [1] and for which he received the Nobel Prize in Physics in 1921. At the turn of the century, researchers had noticed that light incident on clean metal surfaces resulted in electrons being ejected from the metal surface into vacuum. Significantly, these electrons appeared only for incident wavelengths that were shorter than a critical wavelength. Furthermore, the kinetic energies of these ejected electrons appeared to increase with decreasing wavelength. Finally, this wavelength dependence appeared to be independent of light intensity. Einstein recognized that light could deliver its energy in quantized amounts, analogous to the quantized energies of lattice vibrations in a solid that had been proposed earlier by Planck [2] to account for black body radiation (and for which Planck received a Nobel Prize in 1918). These quantized packets of energy, termed photons, could have an energy
    (7.1)
    where h is Planck’s constant, equal to 6.626 × 10−34 J-s, and ν is the frequency of light, equal to the speed of light c divided by wavelength λ. Thus, as wavelength decreases, frequency ν and energy hν increase.
    Figure 7.1 illustrates these features of the photoelectric effect. In Figure 7.1a , electrons absorb photon energy hν and some are ejected into vacuum. The kinetic energy of these electrons can be measured with a plate biased to retard the collection of electrons leaving the illuminated metal. Here the kinetic energy is just equal to the minimum retarding potential needed to cut off collection of these electrons. Figure 7.1b shows the dependence of the maximum kinetic energy Emax versus photon frequency ν. The kinetic energy is linearly proportional to ν with slope h. The minimum energy required to eject an electron is shown as the extrapolated dashed line and defined as the work function, qΦ
    W
  • Let There Be Light
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    Let There Be Light

    The Story of Light from Atoms to Galaxies

    • Ann Breslin, Alex Montwill(Authors)
    • 2013(Publication Date)
    • ICP
      (Publisher)
    Experimental data giving the value of the cut-off potential as a function of the light frequency. The points lie on a straight line, exactly as predicted by Einstein’s equation.
    The figure above shows a graph in which measured values of the stopping potential are plotted as a function of the frequency. This, and all the other experimental data on The Photoelectric Effect agree with the predictions of one simple equation! As a bonus, the slope of the graph provides an independent measurement of Planck’s constant, h.
    Abandoning his former scepticism, Millikan conceded, ‘this is a bullet-like, not a wave-like effect’.
    Note that momentum does not come into play, because the electron is basically attached to the lattice, which is much heavier, and absorbs all the momentum.
    The photoelectric work function
    The work function is a measure of the minimum amount of work required to draw an electron out of the metal. It varies from metal to metal, and determines the minimum photon energy required for The Photoelectric Effect to take place at that metallic surface.
    Photoelectric work functions of some elements.
    The most energetic photons of visible light are at the violet end of the spectrum. It can be seen by comparing the data in the tables above and below that such photons have enough energy to liberate electrons from caesium, potassium and sodium, but not from aluminium, copper, mercury or lead.
    Energies of some visible photons. Practical applications
    Quite apart from its theoretical importance, The Photoelectric Effect has numerous practical applications. It makes it possible to convert a light signal into an electric current. Television cameras, burglar alarms, barcode readers and light sensors of every description are based on The Photoelectric Effect.
    Perhaps the most remarkable practical example is the photomultiplier, which amplifies the electrical signal to such an extent that it is possible to detect the arrival of a single photon. The use of this instrument in some fascinating fundamental experiments with individual photons will be discussed in Chapter 14
  • The History of the Laser
    • Mario Bertolotti(Author)
    • 2004(Publication Date)
    • CRC Press
      (Publisher)
    Annalen der Physik in 1902. In this paper he reported two important facts: the first one was that in order to obtain electrons from a given metal surface only light of certain frequencies was effective; the second fact regarded the velocity (kinetic energy) of the emitted electrons that did not depend on the intensity of the incident radiation.
    Einstein in his work provided an explanation of The Photoelectric Effect as an example of the application of his theory of light quanta. According to him, the energy of the light wave does not propagate as a wave, but rather as a particle (Einstein called it a ‘quantum of energy’) that has an energy inversely proportional to the wavelength of the light. The number of quanta is proportional to the light intensity. The more intense a wave is, the more quanta it contains. When a quantum of light collides with an electron in the metal, it gives the electron all its energy and disappears. The electron spends part of this energy escaping from the metal, and keeps what remains as kinetic energy. The intensity of the light beam, being proportional to the number of quanta, has no effect on the energy of the electrons, but determines their total number.
    In a letter to his friend Conrad Habicht (1876–1958), Einstein wrote of his paper:
    ‘It deals with radiation and the energy characteristics of light and is very revolutionary, as you will see.’
    Notwithstanding this declaration, in discussing the physical interpretation of Wien’s law and enouncing the concept of a quantum of light, Einstein did not consider that he had broken with tradition. By introducing the quantum of light he applied in a coherent way the statistical methods associated with the theory of radiating heat. However, he called his introduction of the hypothesis of light quanta a ‘revolutionary’ step because he thought it contradicted Maxwell’s electrodynamics that required that radiation to be a continuously radiating energy flow in space.
  • Exploring Quantum Physics through Hands-on Projects
    • David Prutchi(Author)
    • 2012(Publication Date)
    • Wiley
      (Publisher)
    Einstein thus proposed that each particle of light carries a quantum of energy according to the color of its light. He named the light particles quanta. We now call them photons. Putting it in terms of light that we can see, red light is composed of individual particles (also called quanta, or photons), where each individual particle (quantum, or photon) has less energy than a particle of violet light. According to Einstein, red light is composed of low-energy quanta, so no one quantum would be energetic enough to knock electrons out of the electrode from Figure 24a. Increasing the intensity of the light does nothing more than increase the number of light quanta showering on this electrode, all of them too weak in energy to liberate an electron from the metal. Beyond a certain threshold frequency, the individual light quantum is energetic enough on its own to liberate a single photoelectron. Above this frequency threshold, a change in intensity would change the number of photoelectrons that are released. However, since only one light quantum of sufficient energy is needed to liberate one photoelectron, the photoelectric emission with high-frequency light will happen no matter how weak the intensity of the light. In 1921, Einstein won the Nobel Prize for his discovery of the law of the photo-electric effect. From now on, to keep things consistent, we’ll call particles of light by their modern name: photons. This name applies whether we talk about a photon corresponding to the very low frequencies of radio and microwaves, the visible spectrum, or the extremely high frequencies of cosmic gamma rays. You can experiment with The Photoelectric Effect using a phototube, such as that shown in Figure 25. The device is a gas-filled or vacuum tube that has an electrode (the photocathode) which expels electrons when illuminated by a light source. The photo-electrons can be collected by a thin wire electrode (the anode), causing a current to flow through a closed circuit
  • Let There Be Light
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    Let There Be Light

    The Story of Light from Atoms to Galaxies

    • Alex Montwill, Ann Breslin(Authors)
    • 2008(Publication Date)
    • ICP
      (Publisher)
    photoelectric effect was first discovered, quite by accident, in 1887, by Heinrich Hertz (1857–1894), who was working on the production of radio waves by means of an electrical spark discharge between two metal spheres. He noticed that when he illuminated the spheres with ultraviolet light, the sparks which came across were bigger and brighter. At the time he did not realise that this was due to electrons liberated from the metal by the light. A year later Wilhelm Hallwachs (1859–1922) confirmed the phenomenon for various other metallic surfaces.
    There are ‘grains’ in the light beam
    The fact that The Photoelectric Effect works at all is already strong evidence for the particle-like nature of light. Bits of matter thrown out look more like the result of sandblasting! Particularly convincing is the fact that there is no measurable delay between exposure to light and the appearance of photoelectrons. Light of intensity as low as a few microwatts per square metre produces an immediate, detectable photoelectric current. The effect is practically instantaneous (the delay is less than 10–9 s).
    13.1.4 How long would we expect to wait? An order-of-magnitude calculation
    The minimum energy required to pull an electron out of the metal is of the order of 3 eV. (The electron volt, eV, is the unit of energy commonly used in atomic physics, equal to the energy of an electron which has been accelerated through a potential difference of 1 volt, and is equivalent to 1.60 ×10–19 J.) Let us assume that there is one free electron per atom and that the photoelectron comes from one of the ten layers of sodium atoms closest to the surface. Assuming a light beam is spread out evenly and smoothly with an intensity of 5 × 10–6 Wm-2 , we can estimate the time required for an electron to receive the necessary energy as follows:
    Estimating the time taken if the light energy is evenly divided
    Allowing for the very approximate nature of the above estimate, it is clear that the observed emission of photoelectrons is too fast by at least 16 orders of magnitude. The situation can be compared to the power of the sea which gradually erodes the shore. The energy of the waves is distributed over a large area, and over a long period of time. If this power were concentrated in quanta of analogous proportions, we might find the Rock of Gibraltar ejected suddenly and without warning.
  • Practical Fluorescence Spectroscopy
    • Zygmunt (Karol) Gryczynski, Ignacy Gryczynski(Authors)
    • 2019(Publication Date)
    • CRC Press
      (Publisher)
    CHAPTER 1

    Theory of Light and Light Interaction with Matter

    C ONVENTIONALLY, WE CALL LIGHT ” a small range of a broad spectrum of electromagnetic radiation that corresponds to the visible spectral range (400–700 nm) as shown in Figure 1.1 . Light is electromagnetic radiation which presents properties of both a wave and a particle. A “particle” of light is called a photon. The dual nature of light is often a source of confusion, but experiments confirming both interpretations exist. For example, experiments involving single-photon double-slit interference and The Photoelectric Effect have shown both the wave and particle nature of light, respectively. A photon is a quanta or the smallest possible amount/part of an electromagnetic energy/wave. Since we almost always refer to multiple photons, a photon can be referred to as a quantum of electromagnetic radiation. Both definitions will be used throughout this text. For example, a single chromophore (molecule) absorbs or emits a photon of a certain energy. It is important to remember that when discussing photons or electromagnetic waves, we are talking about light; both representations are equivalent, but one is often much easier applied to a particular scenario. For example, it is more natural to discuss a metal interacting with an oscillating electric wave rather than a stream of “particles” (photons) that never physically collide with the metal surface.
    FIGURE 1.1 Electromagnetic radiation. The expanded range of 400–700 nm represents visible light.

    1-1      BASICS OF LIGHT

    This section is meant as a review of the basics of light as electromagnetic waves or photons. More importantly, it should demonstrate that there are many different ways of looking at light from a mathematical perspective, but they all lead to the same interpretation. Various uses of light are presented across many different fields, especially biology, chemistry, physics, and engineering. Within each field, and indeed specializations within each individual field, the nomenclature and properties of interest vary. For example, in biology, spectra are frequently given in a wavelength scale (nanometers) but in the semiconductor field, they are typically presented on a scale in terms of energy (electron volts). However, any spectrum may be presented in wavelength or energy without a loss of information. By the end of this chapter, the reader should have a fluid understanding of the relationships between different notations.
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