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Special relativity: from clock operations to electrodynamics: §10 · electron force, work, and closing scope

Zur Elektrodynamik bewegter Körper

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§10 · electron force, work, and closing scope

A force-to-acceleration ratio needs two frame labels

Why are there two transverse coefficients?

Fxax=mγ3,Fy′ay=mγ2,Fyay=mγ\frac{F_x}{a_x}=m\gamma^3,\qquad\frac{F_y'}{a_y}=m\gamma^2,\qquad\frac{F_y}{a_y}=m\gamma

Longitudinal laboratory force over acceleration is m gamma cubed. Rest-frame transverse force over laboratory acceleration is m gamma squared. Laboratory transverse force over laboratory acceleration is m gamma.

For an electron moving along xx, a force across the motion is γ\gamma times larger in the electron’s momentary rest frame than in the laboratory. Einstein divides the rest-frame force by the laboratory acceleration and gets mγ2m\gamma^2. Dividing the laboratory force by the same acceleration gives mγm\gamma.

At 0.6c0.6c, γ=1.25\gamma = 1.25. The longitudinal mass is mγ3=1.953125 mm\gamma^3 = 1.953125\,m, Einstein’s transverse mass is mγ2=1.5625 mm\gamma^2 = 1.5625\,m, and the all-laboratory transverse ratio is mγ=1.25 mm\gamma = 1.25\,m. The electron-dynamics laboratory shows each number with the frames it uses, and leaves Einstein’s result as he printed it.

Return to why there are two transverse coefficients. (included in this file)

Along the motion: m gamma cubed

Modern teaching equation, not the equation as printed.

Fxax=m γ3\frac{F_x}{a_x} = m\,\gamma^{3}

Longitudinal laboratory force over acceleration gives m gamma cubed.

Pushing along the motion, the ratio of force to acceleration is m times gamma cubed. At 0.6c that is 1.953125 m.

Across the motion, both in the laboratory: m gamma

Modern teaching equation, not the equation as printed.

Fyay=m γ\frac{F_y}{a_y} = m\,\gamma

Laboratory transverse force over acceleration gives m gamma.

With force and acceleration both measured in the laboratory, the sideways ratio is m times gamma: 1.25 m at 0.6c. Changing the frame of the force changes the ratio by gamma.

Across the motion, the paper's convention: m gamma squared

Modern teaching equation, not the equation as printed.

Fy′ay=m γ2\frac{F_y'}{a_y} = m\,\gamma^{2}

Comoving transverse force over laboratory acceleration gives m gamma squared.

With the sideways force measured in the electron's own frame and the acceleration in the laboratory, the ratio is m times gamma squared: 1.5625 m at 0.6c. This is the paper's transverse mass.

Assumptions

  • In its momentary rest frame the electron obeys ordinary mechanics for slow motion.
  • Every force and every acceleration is labelled with the frame it is measured in.

Limits

  • The two masses are ratios of force to acceleration under stated conventions; the electron’s own mass does not change with the observer’s speed.
  • The electron is treated as a point driven slowly, without the effects of its own radiation or field.

The work integral has an observable endpoint

What energy is required to accelerate an electron?

K=∫0vmγ(u)3u du=mc2(γ−1)K=\int_0^v m\gamma(u)^3u\,du=mc^2(\gamma-1)

Integrating the longitudinal work from rest gives m c squared times gamma minus one.

The integral follows from one derivative, dγ/du=γ3u/c2d\gamma/du = \gamma^3 u/c^2: the integrand mγ3um\gamma^3 u is mc2mc^2 times it, so the integral is mc2(γ−1)mc^2(\gamma - 1). At low speed this approaches the familiar mv2/2mv^2/2. At 0.6c0.6c the exact value is 0.25 mc20.25\,mc^2 and the low-speed formula gives 0.18 mc20.18\,mc^2, a difference large enough to see.

∣q∣U=K,rB=γmv∣q∣B|q|U=K,\qquad r_B=\frac{\gamma mv}{|q|B}

For acceleration from rest, charge magnitude times voltage magnitude supplies kinetic energy; in a transverse magnetic field the circular radius is gamma m v over charge magnitude B.

The third relation compares bending by the two kinds of field. In an electric field across the motion the path curves with radius γmv2/(∣q∣Ey)\gamma mv^2/(|q|E_y) at that instant; the field also speeds the electron up as the path turns, so the radius keeps changing. In a magnetic field the speed stays constant and the path is a circle of radius γmv/(∣q∣B)\gamma mv/(|q|B). The electron-dynamics laboratory keeps the two cases apart.

Return to the energy it takes to accelerate an electron. (included in this file)

The voltage supplies the energy

Modern teaching equation, not the equation as printed.

∣q∣ U=K|q|\,U = K

Charge magnitude times voltage magnitude supplies kinetic energy.

Accelerated from rest through a voltage U, the electron gains energy |q| times U, and all of it is energy of motion. With K = mc²(γ − 1) this fixes the electron's speed.

Add up the work from rest

Modern teaching equation, not the equation as printed.

K=∫0vm γ(u)3 u duK = \int_{0}^{v} m\,\gamma\left(u\right)^{3}\,u\,\mathrm{d}u

Integrating the longitudinal work from rest gives the kinetic energy.

The work done on the electron as it speeds up from rest to v: the longitudinal mass m gamma cubed times the speed, added up over every speed on the way.

The result: m c squared times gamma minus one

Modern teaching equation, not the equation as printed.

K=m c2 (γ−1)K = m\,c^{2}\,\left(\gamma - 1\right)

Integrating the longitudinal work from rest gives m c squared times gamma minus one.

Because the rate of change of gamma with speed is gamma cubed u over c squared, the integral is m c squared times the change in gamma, from 1 at rest to gamma at v. At 0.6c that is 0.25 m c squared; the familiar one half m v squared gives 0.18 m c squared, so at this speed the difference is plain.

The circle in a magnetic field

Modern teaching equation, not the equation as printed.

rB=γ m v∣q∣ Br_B = \frac{\gamma\,m\,v}{|q|\,B}

In a transverse magnetic field the circular radius is gamma m v over charge magnitude B.

In a uniform magnetic field across its motion the electron goes round a circle. Its radius is gamma m v over |q| B: larger than m v over |q| B, the value without gamma, by gamma. At 0.6c that is 25 per cent.

Assumptions

  • The electron has a fixed mass m and moves slower than light, and force is defined as stated.
  • For the voltage relation, the electron starts at rest and all the work of the field becomes its energy of motion.

Limits

  • Losses by radiation and interactions with matter are left out.
  • The kinetic energy formula alone does not give the September paper’s result that a body’s mass changes with its energy.

Foundations included in this file

Adding and averaging

What does an average keep, and what does it lose?

Four jars hold 3, 1, 1 and 3 marbles. Pour them together and there are 8. Share the 8 equally between the four jars and each holds 2. Two is the average, although no jar held 2 to begin with.

The average keeps the total and the count and nothing else, so 3, 1, 1, 3 and 2, 2, 2, 2 have the same average. Listing every value twice doubles both the total and the count, and the average stays at 2.

Worked example: Three mornings with the same average

  1. One morning the four jars hold 3, 1, 1 and 3 marbles. Add them: 8. Divide by the four jars: an average of 2.
  2. Another morning they hold 8, 0, 0 and 0. Add them: 8 again. Divide by four: 2 again, and now three jars are empty.
  3. A third morning every jar holds 2, which is the average itself. Add them: 8. Divide by four: 2.
  4. Write any of those three lists out twice over. The total doubles to 16 and the count doubles to 8 jars, and 16 divided by 8 is still 2.
  5. Four descriptions and one average. It keeps the total and the count, and the differences between the mornings are what it leaves behind.

Where this lesson stops

An average is the total shared equally among the observations, and two very different lists can have the same one.

Return to the chapter

Density is not probability

What does the height of a probability curve mean?

Mark where 100 particles end up on a ruler divided into 2 μm bins. If 30 land in one bin, that bin holds a probability of about 0.3, and the density there is 0.3 divided by 2 μm, or 0.15 per micrometre. Measured in metres the same density is 150,000 per metre, while the bin still holds 0.3: the height depends on the unit of length, and the probability does not.

P(a≤X≤b)=∫abp(x) dxP(a\le X\le b)=\int_a^b p(x)\,dx

The probability of the interval from a to b is the integral of the density over that interval.

Under a smooth curve, any single exact position has probability zero, since an interval of zero width has no area. At the starting instant of the Brownian problem every particle sits at one point. No curve can draw that: the whole probability, 1, sits on the single point, and a curve appears only once the particles have begun to spread.

Worked example: A flat density across four micrometres

  1. Spread the probability evenly over 4 μm. The density is 1 divided by 4 μm, or 0.25 per micrometre.
  2. The area over the whole 4 μm is 0.25 per μm × 4 μm = 1.
  3. A 1 μm piece has probability 0.25 × 1 = 0.25, and a 2 μm piece has 0.5.
  4. Squeeze the same probability into 2 μm and the height doubles to 0.5 per micrometre, while the total stays 1. The height was never a probability.

Where this lesson stops

The height of the curve is a density, a probability per unit length. Only the area over an interval is a probability.

This lesson builds on

Return to the chapter

Adding continuously

How do you add up something that varies continuously?

Chance spread along a line is measured per unit length: a density. Where the density is the same all along a stretch, the chance of the stretch is the density times its length. A particle equally likely to be anywhere in a 4 µm stretch has density 0.25 per micrometre, and the chance of finding it in the first 1.5 µm is 0.25 × 1.5 = 0.375.

Where the density changes from place to place, cut the line into narrow strips. Each strip contributes its height times its width, as if the density were flat across it. Add the strips, then cut them narrower and add again. For a smooth curve the totals settle on one value, and that value is the integral:

∫abp(x) dx=lim⁡Δx→0∑ip(xi) Δx\int_a^b p(x)\,dx = \lim_{\Delta x \to 0} \sum_i p(x_i)\,\Delta x

The integral of p of x from a to b is the value that the sum of p of x i times delta x settles on as delta x shrinks.

The units multiply. A probability density is a probability per metre, so a strip of it, times a width in metres, is a plain probability. For a density the whole area must be 1, because the particle has to be somewhere. The Brownian paper's §4 writes exactly that for the chances of a jump Δ, ∫φ(Δ) dΔ = 1, and the light-quanta paper's §3 adds entropy over every frequency, S = v∫φ dν.

One more tool recurs in the papers: integration by parts. It is the product rule for derivatives added up over an interval, and it moves a derivative from one factor to the other at the price of an endpoint term:

∫abudvdx dx=[uv]ab−∫abvdudx dx\int_a^b u\frac{dv}{dx}\,dx = [uv]_a^b - \int_a^b v\frac{du}{dx}\,dx

The integral of u times the derivative of v equals u v at b minus u v at a, minus the integral of v times the derivative of u.

The endpoint term, uv at b minus uv at a, is part of the answer. It disappears only when uv is zero at both ends, as it is for a density that falls to zero far out on both sides.

Worked example: A rising density, added up in narrower strips

  1. A particle's density rises steadily across a 4 µm stretch, from 0 at the left end to 0.5 per micrometre at the right. The whole area is a triangle, ½ × 4 × 0.5 = 1.
  2. Four strips 1 µm wide, each taking the height at its left edge: 0 + 0.125 + 0.25 + 0.375 = 0.75.
  3. Eight strips 0.5 µm wide: the heights add to 1.75, and times 0.5 that is 0.875.
  4. Sixteen strips 0.25 µm wide: 0.9375. The shortfall halves each time the strips do: 0.25, then 0.125, then 0.0625.
  5. The totals settle on 1, the area of the triangle. That settled value is the integral.

A flat density gives the same total for every cut, which is why the uniform stretch above needed no strips. A curved one, such as the Brownian bell curve, does, and the integral is the value the totals settle on.

Where this lesson stops

An integral is a total of height times width over a range, in the units of both. The widths and any endpoint term are part of the calculation, not decoration on the integral sign.

This lesson builds on

Return to the chapter

Energy of motion and inertia

If a body moves at the same speed but carries less energy of motion, what has changed?

A force that pushes a body through a distance does work on it, and the work becomes the body's energy of motion, its kinetic energy. That is separate from energy stored inside the body, as heat or in its chemistry.

For one body at everyday speeds, doubling the speed multiplies the energy of motion by four. At a fixed speed, doubling the mass doubles it. The mass-energy paper's title asks about a body's Trägheit, its inertia: its resistance to a change in its motion, which is measured by pushing it, not by weighing it.

K=12mv2K=\frac{1}{2}mv^2

In Newtonian mechanics, kinetic energy is one half times inertial mass times speed squared.

This formula holds at speeds small compared with the speed of light, and it is not exact close to that speed. So the mass-energy argument works with the exact expression and reads the mass from its low-speed limit, where it takes this form.

Worked example: Two bodies at the same speed, different masses

  1. Two bodies move at 2 metres per second.
  2. The 3 kg body has ½ × 3 × 2² = 6 joules of energy of motion; the 2 kg body has ½ × 2 × 2² = 4 joules.
  3. The speed is the same, and the energies differ by 2 joules because the masses differ by 1 kg.
K0−K1=12(m0−m1)v2K_0-K_1=\frac{1}{2}(m_0-m_1)v^2

At the same low speed, the kinetic-energy drop equals one half times the mass decrease times the squared speed.

Here the two masses are given, so the example proves nothing about mass and energy. The 1905 argument runs the other way: it computes the energy difference from the light the body gives off, finds that it has this form, and reads the mass difference from the coefficient of ½v².

Where this lesson stops

At the same low speed, less energy of motion means less mass. The comparison gives only a difference in mass, never the total energy stored inside the body.

This lesson builds on

Return to the chapter

Static laboratory examples

sr-13: a built-in worked result

Static host-calculated example, not a running experiment or an observation. Canonical units and owner-supplied statuses are retained. Open sr-13 online

Build-time scalar readouts
QuantityValueUnitStatus
longitudinalMass1.7791765066210937e-30kgvalue
transverseMassComoving1.423341205296875e-30kgvalue
transverseMassLaboratory1.1386729642375e-30kgvalue
kineticEnergy2.0467764469921127e-14Jvalue
kineticEnergyNewtonian1.473679041834321e-14Jvalue
acceleratingPotential127749.7376729383Vvalue
acceleratingPotentialNewtonian91979.81112451557Vvalue
radiusCurvatureMagneticNo numeric valuemoutside-domain
radiusCurvatureElectric2.299495278112889mvalue
lorentzFactor1.251value
speedRatio0.61value

1 array outputs are not reproduced. This table does not claim to reproduce the interactive plot.

Settings (canonical units)

customCharge
-1.602176634e-19
customMass
9.1093837139e-31
datasetOverlay
none
electricFieldX
0
electricFieldY
100000
electricFieldZ
0
forceConvention
source
initialDirectionDeg
0
initialSpeed
0.6
integrationInterval
2e-9
magneticFieldX
0
magneticFieldY
0
magneticFieldZ
0
massLanguage
1905
particle
electron

Evaluator: source:sha256:3ec9af5c69ff8a2d46951101875199420576c8728aa55f2a49da1a2794f8a214

Source references

  1. A. Einstein, Zur Elektrodynamik bewegter Körper. Annalen der Physik (4), 17, 891–921 (1905).
  2. 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.