Physics · Ch 7 — Dual Nature of Radiation and Matter
Particle nature of light: Einstein's explanation
Particle nature of light: Einstein's explanation
In 1905, Einstein extended Planck's quantum idea from the atomic oscillators that emit or absorb light to light itself. Rather than picturing the energy in a light wave as spread out continuously over its wavefront, Einstein proposed that light of frequency from any source should be thought of as a stream of discrete energy packets, or quanta, each carrying energy . Each such quantum of light behaves, in every relevant respect, like a genuine particle, and is called a photon. Einstein further proposed that a photon carries a definite linear momentum of magnitude .
From this single reconception of light, the following characteristic properties of photons follow. (i) A photon of frequency and wavelength carries energy . (ii) A photon's energy is set entirely by the frequency of the radiation, never by its intensity -- intensity instead reflects only how many photons per second are arriving, with each individual photon's energy unaffected. (iii) Photons travel at the speed of light and carry momentum . (iv) Being electrically neutral, photons are completely unaffected by electric and magnetic fields. (v) In any photon-electron interaction, total energy, total linear momentum and total angular momentum are all conserved, though the number of photons itself need not be conserved, since a photon can be absorbed entirely or a new one produced in the interaction.
Applying the photon picture to the photoelectric effect: when a single photon of energy strikes a metal surface, it is completely absorbed by one single electron. Part of this absorbed energy, equal to the photoelectric work function , is used up ejecting the electron from the metal, and the remainder becomes the ejected electron's kinetic energy. Conservation of energy for this one photon-one electron interaction gives Einstein's photoelectric equation,
If an electron loses no energy to internal collisions on its way out, it emerges with the maximum possible kinetic energy , and equation (7.6) rearranges to the most commonly used form,
At the threshold frequency , the photoelectron is emitted with essentially zero kinetic energy, so equation (7.6) reduces to (7.7 combines these as ). Plotting against from equation (7.8) gives a straight line whose slope is and whose -intercept, extended back to zero frequency, is ; this is exactly the graph R. A. Millikan produced experimentally for several metals (caesium, potassium, sodium, calcium), finding that although each metal's line sits at its own characteristic height (fixed by that metal's own work function), every line has the identical slope -- Millikan's precise experimental route to Planck's constant, Js.
Einstein's equation explains every one of the five experimental laws at once. (i) Since each absorbed photon liberates exactly one electron, more photons per second (higher intensity) simply means more electrons emitted per second, i.e. more photocurrent -- exactly as observed. (ii) From , the maximum kinetic energy depends only on frequency, never on intensity -- resolving the first puzzle from section 7.2.6. (iii) Since a photon needs at least energy to free an electron at all, there must exist a minimum (threshold) frequency below which no photoelectron can ever be emitted, however many photons arrive -- resolving the second puzzle. (iv) Because each photon's energy is transferred to a single electron in one complete, instantaneous absorption event rather than being slowly accumulated, there is no time lag between the light striking the surface and the electron being ejected -- resolving the third puzzle. …
What this figure shows. Two small panels each show a metal surface being struck by an incoming photon of energy , with an electron shown leaving the surface in panel (a) carrying maximum kinetic energy , corresponding to light above the threshold frequency, while panel (b) shows the special case at exactly the threshold frequency , where the photon's energy is just enough to free the electron and it leaves the surface with essentially zero kinetic energy, . The two panels together are the pictorial version of Einstein's photoelectric equation: as the incident frequency is reduced toward , the emitted electron's kin …
What this figure shows. A graph with frequency of the incident light along the horizontal axis and maximum kinetic energy of the photoelectrons along the vertical axis, drawn as a single straight line that crosses the frequency axis at the threshold frequency and has a y-intercept of when extended back to zero frequency. The line's slope is explicitly labelled -- Planck's constant -- making this graph the direct experimental route to measuring : it is exactly the straight-line form that Einstei …
What this figure shows. The same kind of -versus- straight-line graph as Figure 7.14, but now drawn simultaneously for four different metals -- caesium, potassium, sodium and calcium -- as four parallel lines, each starting from its own y-intercept marked with that metal's own negative work function value (-2.14 eV, -2.30 eV, -2.75 eV and -3.20 eV respectively) but all sharing the identical slope, explicitly labelled 'Slope = h'. This is exactly the graph Robert Millikan produced to experimentally verify Einstein's equation: the four lines' common slope, independent of which metal is used, gave Millikan his precise measurement of Planck's constant, Js, wh …
Worked out. A radiation of wavelength 300 nm is incident on a silver surface, and the task is to determine whether photoelectrons will be observed at all. Computing the incident photon's energy using (expressed in eV) with the standard constants gives eV. Comparing this against silver's work function, listed in Table 7.1 as 4.7 eV, shows the photon energy (4.14 eV) is less than the work function (4.7 eV) required to free even the most weakly bound surface electron -- so no photoelectrons are observed for this radiation on silver, however long or brightly it is shone, illustrating the strict quantum threshold-energy condition that a …
Worked out. When light of wavelength 2200 Å falls on copper (work function eV), photoelectrons are emitted, and the task is to find both the threshold wavelength and the stopping potential. The threshold wavelength follows directly from , giving Å -- the longest wavelength (lowest frequency) copper can still respond to. The incident photon's own energy at 2200 Å works out to J eV, so applying Einstein's equation gives the photoelectrons' maximum kinetic energy as eV. Since , the corresponding stopping potential is simply V -- a clean numerical illustration of how a single incident wavelength, together with a metal's tabulated work function, pins down both the thresho …
Worked out. UV light of wavelength 3000 Å and intensity is incident on a potassium surface (work function 2.30 eV) of area , and the task has two parts. First, the incident photon's energy works out to J eV, so by Einstein's equation the maximum kinetic energy of the ejected photoelectrons is eV. Second, assuming 40% of the incident photons actually succeed in producing a photoelectron, the number of photons striking the surface per second is found from the incident power divided by the single-photon energy, photons per second, so the rate of photoelectron emission is photoelectrons per second -- showing how a photon-counting argument …
Worked out. Light of wavelength 390 nm directed at a metal electrode is found to be completely stopped by an opposing potential difference of 1.10 V, and the task is to find both the metal's work function and its threshold wavelength for ejecting electrons. Since at the stopping potential, Einstein's equation can be rewritten as ; substituting the given wavelength and stopping potential gives J eV. The threshold wavelength then follows from , giving Å (about 5963-5969 Å depending on rounding) -- demonstrating that a single stopping-potential measurement at one known wavelength is, by itself, enough to fully characterise …