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§8 · photoelectric energy and counts

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§8 · photoelectric energy and counts

A derivation

More electrons is not more energy per electron

What changes when frequency rises, and what changes when power rises?

The 9 printed paragraphs this passage explains
  • §8, paragraph 1: The usual view, that the energy of light is spread continuously, meets great difficulties in explaining the photoelectric effects, which Lenard described in detail.
  • §8, footnote 1: The footnote cites Lenard, Annalen der Physik, volume 8, pages 169 and 170, 1902.
  • §8, paragraph 2: If the exciting light consists of energy quanta, the production of cathode rays by light can be pictured simply: quanta enter the surface layer and give their energy, at least in part, to electrons, the simplest case being one quantum to one electron. An electron loses some energy on its way out and must do a work P to leave, so the fastest electrons leave with the energy (R/N)βν − P.
  • §8, paragraph 4: With E = 9.6 × 10³, Π × 10⁻⁸ is the potential in volts that the body reaches when irradiated in a vacuum.
  • §8, paragraph 5: As an order-of-magnitude check, with P′ = 0 and the frequency at the ultraviolet end of the solar spectrum, the formula gives about 4.3 volts, the same order as Lenard's results.
  • §8, footnote 3: The footnote cites Lenard, Annalen der Physik, volume 8, pages 165 and 184, plate I, figure 2, 1902.
  • §8, paragraph 6: If the formula is right, Π plotted against the frequency of the exciting light must be a straight line whose slope does not depend on the substance.
  • §8, footnote 4: The footnote cites the same paper by Lenard, pages 150 and 166 to 168.
  • §8, paragraph 7: As far as Einstein can see, the view does not contradict what Lenard observed: if each quantum acts independently, the speeds of the electrons do not depend on the intensity of the light, while the number of electrons leaving is proportional to it.

The most energetic electron receives a complete quantum and escapes with the least modeled energy loss. Subtracting the escape work Φ\Phi gives the maximum kinetic energy, provided emission is energetically allowed.

Kmax=h ν−ΦK_{\mathrm{max}} = h\,\nu - \Phi
ν0=Φh\nu_0 = \frac{\Phi}{h}

Maximum kinetic energy equals h frequency minus escape work, with threshold frequency Phi over h.

For a hypothetical work function of 2 electron volts and a frequency of 600 terahertz, the maximum is about 0.4814 electron volts using modern SI constants. Doubling optical power while retaining that frequency and escape work leaves the maximum unchanged.

Power is energy arriving per second. At fixed frequency, dividing it by hνh\nu gives the incoming quantum rate. Under a fixed yield, twice the power can therefore produce twice the electron count per second. Below threshold, negative hν−Φh\nu - \Phi is an energy deficit, not a negative kinetic energy of an emitted electron.

Show every step here: More electrons is not more energy per electron

Letters: the paper takes the exciting light to consist of energy quanta of size RNβν\frac{R}{N}\beta\nu, writes P for the work an electron must do to leave the body (Φ here), and writes ε for the electron's charge. This explanation writes the quantum as hν, with h a later name for Rβ/N.

  1. The simplest picture, which the paper assumes occurs: a light quantum gives its whole energy to a single electron. The paper also leaves open that some electrons take up only part of a quantum's energy.
  2. An electron excited inside the body loses part of its kinetic energy before it reaches the surface. The fastest electrons are those excited right at the surface and moving straight out.
  3. Each electron must do a work P, characteristic of the body, to leave it. So the kinetic energy of the fastest electrons is the quantum minus that work: RNβν−P\frac{R}{N}\beta\nu-P.
  4. In the explanatory letters, with hν for the quantum and Φ for P, that is the first half of the formula below. Setting it to zero gives the lowest frequency at which the fastest electron can still escape, the threshold ν0=Φ/h\nu_0=\Phi/h.
Kmax=h ν−ΦK_{\mathrm{max}} = h\,\nu - \Phi
ν0=Φh\nu_0 = \frac{\Phi}{h}

Maximum kinetic energy equals h frequency minus escape work, with threshold frequency Phi over h.

  1. Worked case with modern SI constants, for a hypothetical work function of 2 electron volts at a frequency of 600 terahertz: hν=6.62607×10−34×6.00×1014=3.97564×10−19h\nu=6.62607\times10^{-34}\times6.00\times10^{14}=3.97564\times10^{-19} joule, which divided by 1.602177×10−191.602177\times10^{-19} joule per electron volt is 2.4814 electron volts. Subtract 2: the maximum kinetic energy is 0.4814 electron volts.
  2. The threshold for that work function is ν0=2\nu_0=2 electron volts divided by h, about 484 terahertz.
  3. Below the threshold, hν−Φh\nu-\Phi is negative. That is a shortfall of energy: no electron escapes by this route, and there is no negative kinetic energy to report.
  4. The paper's own check, in its letters: charge the body to a positive potential Π that just prevents it from losing electricity. Then Π times the electron's charge ε equals the kinetic energy RNβν−P\frac{R}{N}\beta\nu-P.
  5. Multiply by N: the charge becomes E, the charge of one gram-equivalent of a monovalent ion, and the right side becomes Rβν minus the escape work for that amount of charge. The paper sets that work to zero for an estimate, takes E=9,6⋅103E=9{,}6\cdot10^{3} in electromagnetic units, ν=1,03⋅1015\nu=1{,}03\cdot10^{15}, the limit of the solar spectrum toward the ultraviolet, and β=4,866⋅10−11\beta=4{,}866\cdot10^{-11}.
  6. Then Π = Rβν/E: 8.31×107×4.866×10−11×1.03×1015/(9.6×103)=4.34×1088.31\times10^{7}\times4.866\times10^{-11}\times1.03\times10^{15}/(9.6\times10^{3})=4.34\times10^{8} electromagnetic units, with R the standard value of 1905. One volt is 10810^{8} of those units, so Π is about 4.34 volts. The page gives 4,3 volts and says the result agrees in order of magnitude with Lenard's.
  7. The paper's further prediction: Π, plotted against the frequency of the exciting light, must be a straight line whose slope does not depend on the substance. In the explanatory letters the slope of KmaxK_{\mathrm{max}} against ν is h for every metal, and only the intercept, set by Φ, changes.
  8. Power sets the count, not the energy of each electron. Optical power is energy per second; divided by hν it gives quanta per second. At 600 terahertz, one milliwatt carries 2.5×10152.5\times10^{15} quanta per second, and two milliwatts carry twice as many, each still of 2.4814 electron volts.
  9. So, if each quantum gives up its energy independently of all the others, the speeds of the electrons do not depend on the intensity of the light, while the number leaving the body is proportional to it, other things being equal (p. 147). Twice the power can give twice the electrons per second; it cannot raise the maximum energy of one.
  10. The laboratory's straight line follows from the equation it is programmed with. It shows a consequence of the model; only measurements made independently can test the model.
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The most an escaping electron can keep

Kmax=h ν−ΦK_{\mathrm{max}} = h\,\nu - \Phi

is times , less .

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The largest kinetic energy equals h times the frequency, minus the escape work.

One quantum pays the escape work, and what is left is the most energy of motion an electron can carry away. The frequency sets it; the light's power does not appear.

Model assumptions and every term’s meaning
  • One electron receives the whole of one quantum, h times the frequency, and nothing from a second quantum.
  • Escaping costs the electron at least the escape work; any further loss on the way out is not negative.
  • These are modern teaching equations in SI notation, not a transcription of the printed section 8.
Largest kinetic energy
The energy of motion of the fastest electron to leave. Electrons that lose energy inside the metal leave with less, so this is a ceiling, not every electron's energy. Read the prerequisite
Planck's constant
Multiplied by the frequency it gives one quantum's energy. The 1905 paper writes the same quantum as R beta nu over N. Read the prerequisite
Frequency of the light
Raising it raises the energy of each quantum, and so the largest kinetic energy, along a straight line of slope h. Read the prerequisite
Escape work
The energy spent getting out of the metal, subtracted from the quantum. Einstein's section 8 calls it P. Read the prerequisite
An energy budget for one electron
What one quantum brings, less what escaping costs, is the most that can be left as motion. The light's power is not in it, so brighter light at the same frequency gives more electrons, not faster ones. Read the prerequisite

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The frequency below which no electron escapes

ν0=Φh\nu_0 = \frac{\Phi}{h}

is divided by .

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The threshold frequency equals the escape work divided by h.

Setting the largest kinetic energy to zero gives the frequency whose quantum only just pays the escape work. Below it the model emits nothing, however bright the light.

Model assumptions and every term’s meaning
  • One electron receives the whole of one quantum, h times the frequency, and nothing from a second quantum.
  • Escaping costs the electron at least the escape work; any further loss on the way out is not negative.
  • These are modern teaching equations in SI notation, not a transcription of the printed section 8.
Threshold frequency
The lowest frequency at which one quantum can free an electron. It depends on the metal, through the escape work, and on nothing about the light but its frequency. Read the prerequisite
Escape work
The same escape work as in the energy budget. A metal that holds its electrons more tightly has a higher threshold. Read the prerequisite
Planck's constant
Dividing an energy by h turns it into the frequency whose quantum carries that energy. Read the prerequisite
Where the budget reaches zero
Put zero for the largest kinetic energy in the budget and solve for the frequency. This threshold is a consequence of the one-quantum assumption, not an independent measurement of it. Read the prerequisite

Every term’s units were checked when this page was built. That checks the units, not the model. This equation is written for this edition in modern notation, not transcribed from the paper.

Modern qualifications

The source discusses the potential attained by an illuminated body; a later collector apparatus is a distinct arrangement. Later measurements such as Millikan’s 1916 work are not premises available in 1905, and agreement with the energy relation alone does not prove the complete light-quantum picture.

Assumptions and limits: More electrons is not more energy per electron

Assumed here

  • One electron can receive one quantum of energy hν.
  • Escape requires positive work Φ, with any additional loss nonnegative.
  • Frequency, work function and yield stay fixed when the power changes.

What this does not establish

  • In the laboratory the threshold and the straight line follow from the model’s assumptions; they are not experimental proof.
  • The work function used in a hypothetical example is not a sourced value for a named metal.
  • Real collection and emission rates require additional material and apparatus assumptions.

Earlier step: A coefficient suggests an energy element

Source context: German source · English · Interlinear gloss · Facsimile

A qualification

Einstein's own limits on the photoelectric laws

Where does Einstein expect his photoelectric regularities might stop holding?

The printed paragraph this passage explains
  • §8, paragraph 8: Einstein adds that the likely limits of validity of these laws call for remarks like those he made about deviations from Stokes's rule.

After working out how the escaping electrons should behave, Einstein adds one sentence of caution: about the presumable limits of validity of these regularities, remarks would have to be made like those about the presumable deviations from Stokes's rule. His word, 'mutmaßlich', means presumable: he expects limits, and he does not locate them.

The regularities are those of the paragraph before. If each energy quantum gives its energy to electrons independently of all the others, the speeds of the escaping electrons do not depend on the intensity of the exciting light, while their number is proportional to it. The energy relation behind them assumes one quantum for one electron:

ΠE=Rβν−P′ΠE=R\beta\nu-P'

Pi times E equals R beta nu minus P prime.

The remarks on Stokes's rule, in §7, named two conditions. First, so many quanta are being transformed at once in each unit of volume that one produced quantum can take its energy from several exciting quanta. Second, the light is not of the kind black radiation has within the range of Wien's law, for instance light from a body so hot that Wien's law no longer holds at the wavelength concerned.

Carried over, as the sentence invites: in very intense light an electron might gather energy from more than one quantum, and then its energy is no longer bounded by one quantum's (R/N)βν less the work P it spends leaving. For light outside Wien's range, the entropy argument of §6 that gave quanta of size Rβν/N does not apply, so it does not secure the size of the energy portions. Einstein spells out neither case for the photoelectric effect; the caution stays a caution.

Show every step here: Einstein's own limits on the photoelectric laws

Letters: Π is the potential the illuminated body reaches, E the charge of a gram-equivalent of a univalent ion, P′P' the work for a gram-equivalent of electrons to leave the body, R the gas constant, N the number of real molecules in a gram-equivalent, β the constant from Planck's formula in §2, and ν the frequency. (R/N)βν is the energy of one quantum; later physics writes it hν.

  1. The regularities being qualified come from the paragraph before: each quantum gives its energy to electrons independently of all the others.
  2. Consequence one: the speeds of the escaping electrons, the quality of the cathode rays, do not depend on the intensity of the light, because each electron still receives the energy of a single quantum.
  3. Consequence two: the number of electrons leaving is proportional to the intensity, other things equal, because doubling the intensity doubles the number of quanta arriving.
  4. Both rest on one quantum for one electron, which gives the stopping condition, for a gram-equivalent of electrons:
ΠE=Rβν−P′ΠE=R\beta\nu-P'

Pi times E equals R beta nu minus P prime.

  1. Worked case, with the paper's own check: P′=0P'=0, R=8.31×107R=8.31\times10^{7}, β=4.866×10−11\beta=4.866\times10^{-11}, ν=1.03×1015\nu=1.03\times10^{15} and E=9.6×103E=9.6\times10^{3}. Then Rβν=8.31×107×4.866×10−11×1.03×1015≈4.16×1012R\beta\nu=8.31\times10^{7}\times4.866\times10^{-11}\times1.03\times10^{15}\approx4.16\times10^{12}, and Π=Rβν/E≈4.3×108Π=R\beta\nu/E\approx4.3\times10^{8}, which the paper converts to about 4.3 volts. One quantum, one electron.
  2. The first condition from §7, carried over: if so many quanta are being transformed at once in each unit of volume that one electron could take energy from two quanta, the energy available to it could reach twice (R/N)βν, and the equation above would no longer bound it. The paper names no intensity at which that begins.
  3. The second condition from §7, carried over: the quantum picture came from the entropy of radiation within the range of Wien's law (§6). Light well outside that range, such as light from a very hot source at the wavelength used, is not covered by that argument, so the argument does not fix the size of its energy portions.
  4. What Einstein asserts is only that such remarks would have to be made. He calls the limits presumable and leaves their details open, so neither carried-over case is a prediction of the paper.

Modern qualifications

In 1905 the photoelectric data were Lenard's, and the paper claims only that its view does not contradict them, as far as Einstein can see. Millikan's measurements of 1916 later tested the straight-line relation between stopping potential and frequency; that is later evidence, not a premise available in 1905. Emission in which one electron takes the energy of two light quanta at once was observed only after lasers made such intensities available, decades later; it is one concrete form of the first condition, and the paper does not anticipate it in any detail.

Assumptions and limits: Einstein's own limits on the photoelectric laws

Assumed here

  • The regularities in question are those of the paragraph before: the speeds of the escaping electrons do not depend on the intensity of the light, and their number is proportional to it.
  • In §7 Einstein named two conditions under which Stokes's rule might fail.
  • §8 says only that similar remarks would apply to the photoelectric laws; it does not spell them out.

What this does not establish

  • The two conditions are carried over from §7 by the analogy Einstein's sentence invites; §8 does not state them itself, so this passage marks them as a reading of his remark.
  • The paper gives no intensity and no temperature at which the laws fail, and neither does this passage.

Earlier step: More electrons is not more energy per electronAn energy budget has conditions

Source context: German source · English · Interlinear gloss · Facsimile

A qualification

A stopping voltage is a magnitude with a sign convention

Why does retarding an electron not make its charge positive?

The 6 printed paragraphs this passage explains
  • §8, paragraph 2: If the exciting light consists of energy quanta, the production of cathode rays by light can be pictured simply: quanta enter the surface layer and give their energy, at least in part, to electrons, the simplest case being one quantum to one electron. An electron loses some energy on its way out and must do a work P to leave, so the fastest electrons leave with the energy (R/N)βν − P.
  • §8, paragraph 3: If the body is charged to the positive potential Π that just stops it losing charge, Π times the electron's charge equals (R/N)βν − P; for a gram-equivalent of electrons this reads ΠE = Rβν − P′.
  • §8, footnote 2: The footnote says the relation is unchanged if the electron must first be freed from a neutral molecule; P′ is then the sum of two works.
  • §8, paragraph 9: The argument assumed that at least some quanta give all their energy to a single electron; without that assumption the equation becomes an inequality, ΠE + P′ ≤ Rβν.
  • §8, paragraph 10: For cathode luminescence, the reverse process, a similar argument gives ΠE + P′ ≥ Rβν. In Lenard's experiments the electrons had fallen through hundreds or thousands of volts to make visible light, so one electron's energy must go into many light quanta.
  • §8, footnote 5: The footnote cites Lenard, Annalen der Physik, volume 12, page 469, 1903.
e Vs=Kmax=h ν−Φe\,V_{\mathrm{s}} = K_{\mathrm{max}} = h\,\nu - \Phi

The positive charge magnitude times the stopping-voltage magnitude equals maximum kinetic energy, h frequency minus escape work.

VsV_s is a nonnegative magnitude. The sign of a laboratory electrode voltage must also specify which electrode is the reference. Using ee for a positive magnitude does not change the negative charge of the electron.

If the electron receives only part of the available energy or loses energy inside matter, its outgoing kinetic energy is at most hν−Φh\nu - \Phi. These losses do not reverse the frequency dependence or turn extra intensity into extra energy for one electron.

A footnote to the stopping condition allows that the light may also have to free each electron from a neutral molecule, at the cost of some work, before the electron can leave. The paper says nothing in the derived relation changes: its P′P', which it defines as the potential of a gram-equivalent of negative electricity with respect to the body, is then read as a sum of two terms, the work to free the electron and the work to leave the body. In the letters used here, Φ\Phi stands for that sum, and the stopping potential still rises in a straight line with frequency, with the same slope.

An inverse energy-budget question asks for the smallest accelerating-potential magnitude capable of supplying a quantum hνh\nu. Within that idealized conversion, eVacceV_{\mathrm{acc}} must be at least hνh\nu. This is an energetic lower bound, not a promise that every collision produces light.

Show every step here: A stopping voltage is a magnitude with a sign convention

Letters: the paper charges the illuminated body to a positive potential Π and writes ε for the electron's charge. This explanation writes VsV_s for the size of the stopping potential and e for the positive size of the electron's charge; the electron's charge itself is −e.

  1. Set the arrangement and the sign: the body is at the potential VsV_s above the conductors around it, which are at zero. An electron leaving the body is pulled back toward it, so the potential retards the electron.
  2. An electron moving from the body out to the surroundings, across a potential difference VsV_s, loses kinetic energy eVseV_s. If it had kinetic energy K at the surface, it arrives with K−eVsK-eV_s, or is turned back if that would be negative.
  3. The body stops losing electricity when even the fastest electron is turned back, that is, when eVseV_s equals the largest kinetic energy KmaxK_{\mathrm{max}}.
  4. Insert the one-quantum budget of the previous passage for KmaxK_{\mathrm{max}}.
e Vs=Kmax=h ν−Φe\,V_{\mathrm{s}} = K_{\mathrm{max}} = h\,\nu - \Phi

The positive charge magnitude times the stopping-voltage magnitude equals maximum kinetic energy, h frequency minus escape work.

  1. Divide by e: Vs=(hν−Φ)/eV_s=(h\nu-\Phi)/e. Worked with the previous passage's hypothetical numbers: KmaxK_{\mathrm{max}} is 0.4814 electron volts, so VsV_s is 0.4814 volts, since one electron volt is e times one volt.
  2. Keep sizes and signs apart. VsV_s is a size, zero or positive. The electron's charge is negative, and writing e for its size does not change that. A voltage read from an instrument also needs its reference electrode named.
  3. The paper's gram-equivalent form of the stopping condition is ΠE=Rβν−P′ΠE=R\beta\nu-P', with P′P' the potential of a gram-equivalent of negative electricity with respect to the body: the work for that much electricity to leave it. A footnote attached to it takes up one more possibility.
  4. Suppose the light must first free each electron from a neutral molecule, at the cost of a certain work, before the electron can make its way out. The footnote says nothing in the derived relation changes; P′P' is then to be read as a sum of two terms.
  5. Why nothing changes: one quantum's energy, (R/N)βν per electron (hνh\nu in the explanatory letters), now pays two works in turn, freeing the electron from its molecule and taking it out of the body. Both come out of the same quantum, so the fastest electron keeps the quantum's energy less their sum. Write Φ\Phi for the sum, and eVs=hν−ΦeV_s=h\nu-\Phi stands as before.
  6. Worked case, with hypothetical numbers: freeing the electron costs 1.0 electron volt and leaving the body 2.0, so Φ\Phi is 3.0 electron volts. A quantum of 3.5 electron volts leaves the fastest electron 3.5 − 1.0 − 2.0 = 0.5 electron volts, and VsV_s is 0.5 volts. A quantum of 2.5 electron volts releases no electron from the body.
  7. What stays: the frequency enters only through the quantum's energy, so the stopping potential plotted against frequency is still a straight line whose slope does not depend on the substance. The two works together only move the frequency at which the line reaches zero.
  8. Partial transfer and losses: if an electron receives only part of a quantum, or loses energy inside the body, it reaches the surface with less than hν−Φh\nu-\Phi. The paper then replaces the equation by an inequality: in its letters, Π times E, plus the escape work for a gram-equivalent, is at most Rβν.
  9. In the explanatory letters: eVs≤hν−ΦeV_s\le h\nu-\Phi. Losses can only lower the stopping potential; they cannot give one electron more than the quantum it received.
  10. The inverse process, cathode luminescence: electrons that have fallen through a potential produce light. Reversing the budget, the energy supplied per electron must be at least the energy of the quantum produced, eVacc≥hνeV_{\mathrm{acc}}\ge h\nu in the explanatory letters.
  11. Worked scale from the paper: in the substances Lenard examined, the cathode rays had to fall through several hundred, in some cases several thousand, volts to produce visible light, far more than the few volts one quantum of visible light needs. The paper concludes that the kinetic energy of one electron is used to produce many light quanta.
  12. A bound is not a promise: eVacc≥hνeV_{\mathrm{acc}}\ge h\nu states what is needed in energy, not that every collision produces light.
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What the stopping potential measures

e Vs=Kmax=h ν−Φe\,V_{\mathrm{s}} = K_{\mathrm{max}} = h\,\nu - \Phi

times is , which the budget puts at times , less .

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The electron's charge times the stopping potential equals the largest kinetic energy, which equals h times the frequency minus the escape work.

A retarding potential that just stops the fastest electrons measures their energy: charge times potential. The one-quantum budget says what that energy should be.

Model assumptions and every term’s meaning
  • One electron receives the whole of one quantum, h times the frequency, and nothing from a second quantum.
  • Escaping costs the electron at least the escape work; any further loss on the way out is not negative.
  • These are modern teaching equations in SI notation, not a transcription of the printed section 8.
  • The stopping potential is taken as measured on the fastest electrons, with contact potentials between electrode materials ignored.
Charge of one electron
Charge times a potential difference is an energy: the work the field does on the electron as it crosses. Read the prerequisite
Stopping potential
The retarding potential at which the current of the fastest electrons just stops. It is read off the apparatus. Read the prerequisite
Largest kinetic energy
The energy the stopping potential measures, and the energy the one-quantum budget predicts. Read the prerequisite
Planck's constant
Sets one quantum's energy with the frequency. It is also the slope of stopping energy against frequency. Read the prerequisite
Frequency of the light
The one property of the light the stopping energy depends on in this model. Read the prerequisite
Escape work
On a plot of stopping energy against frequency the model's line crosses zero frequency at minus the escape work, so the line's intercept measures it. Read the prerequisite
A potential measures an energy
Charge times stopping potential is the energy the fastest electron had. This half is how the apparatus reads energy, not a claim about light. Read the prerequisite
The prediction to test
The one-quantum budget says that measured energy rises in a straight line with frequency, with slope h. An experiment can test that; restating the equation cannot. Read the prerequisite

Every term’s units were checked when this page was built. That checks the units, not the model. This equation is written for this edition in modern notation, not transcribed from the paper.

Modern qualifications

This modern voltage-magnitude convention does not silently replace the paper’s printed charge and potential symbols. The historical 4.3-volt check belongs to its separately identified constant and unit convention in the photoelectric laboratory. The footnote on P′P' leaves room for electrons bound in neutral molecules without giving that work a value; §9 applies the same one-quantum budget to freeing an electron from a gas molecule, which is ionization.

Assumptions and limits: A stopping voltage is a magnitude with a sign convention

Assumed here

  • e denotes a positive charge magnitude; the electron charge is −e.
  • A retarding potential removes kinetic energy, with the sign convention of the electrodes stated.

What this does not establish

  • No stopping endpoint for emitted electrons is supplied when emission is not allowed.
  • A negative energy deficit and a signed collector voltage are different quantities.
  • The footnote gives no size for the work of freeing an electron from a molecule; the passage's figures for it are hypothetical.

Earlier step: More electrons is not more energy per electron

Source context: German source · English · Interlinear gloss · Facsimile

References

A. Einstein, Über einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt. Annalen der Physik (4), 17, 132–148 (1905).

A. Einstein, On the motion of particles suspended in liquids at rest required by the molecular-kinetic theory of heat. Annalen der Physik (4), 17, 549–560 (1905), §§1–5. Bibliographic pointer; this preview is not a source transcription or translation.

A. Einstein, Zur Elektrodynamik bewegter Körper. Annalen der Physik (4), 17, 891–921 (1905).

A. Einstein, Does the inertia of a body depend upon its energy content? Annalen der Physik (4), 18, 639–641 (1905). External 1923 Perrett–Jeffery translation, electronically transcribed by John Walker; its notation was modernized. A reference for this explanatory preview, not this edition’s translation or its pinned facsimile.

R. A. Millikan, A Direct Photoelectric Determination of Planck's "h". Physical Review (2), 7 (3), 355–388 (1916).

26 foundation readings sit behind this argument.

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