Part C · the analytic toolkit · spine
The chain rule alone shows the wave operator breaks under x ↦ x − vt; asking which substitution does not break it produces the Lorentz transformation, with c supplied by the equation rather than by a postulate.
needs 24, 03~2 h slides + 4 h problemsproblems: ./mr problems 25
25 · overview
Every component of a light wave obeys $u_{tt} = c^2u_{xx}$. Galileo's $x' = x - vt$, $t' = t$ breaks it. Which linear change of frame does not?
1. The chain rule turns $\partial_t^2 - c^2\partial_x^2$ into a combination of $\partial_{t'}^2$, $\partial_{x'}\partial_{t'}$, $\partial_{x'}^2$ whose coefficients are read off the map. Galileo's leaves $-2v\,\partial_{x'}\partial_{t'}$, which no redefinition of the field removes.
2. Demand no cross term and the right ratio of the other two. The cross term dies only if $t'$ depends on $x$: $\ x' = A(x - vt)$, $t' = A(t - vx/c^2)$.
3. With $y' = sy$, $z' = sz$, the transverse terms force $A^2(1 - v^2/c^2) = s^2 \gt 0$: so $|v| \lt c$, and one scale $s(v)$ is left free.
4. The inverse must be the same rule at $-v$, and space is isotropic: so $s = 1$ — the Lorentz boost, whose invariant speed is the $c$ in the operator.
Galileo tilts only the time axis. The map that saves the operator also tilts $t' = 0$ (dashed), mirroring $x = vt$ in the light line.
Dotted: a glossary term, click it or press G. Solid: the running example, on hover. N: the notes.
The plan. 1 covariance · 2 the boost fails · 3 three ways out, and their experiments · 4 the right substitution · 5 a group.
section 1
Newton's laws cannot tell uniformly moving frames apart. Saying precisely what that means — for particles, and then for fields — is the definition this unit is built on.
25 · covariance
The maps of spacetime $\mathbb R\times\mathbb R^3$ $$(t, \vec x) \;\mapsto\; (t + \tau,\ R\vec x - \vec vt + \vec a),$$ $R \in SO(3)$ (unit 03), $\vec v, \vec a \in \mathbb R^3$, $\tau \in \mathbb R$: ten parameters. The case $R = I$, $\vec a = \vec 0$, $\tau = 0$ is a Galilean boost — the frame whose origin moves at $\vec v$.
It is a group: the composite of two such maps is another, and each has an inverse of the same form (notes).
If $m_i\ddot{\vec x}_i = \sum_{j\ne i}\vec F_{ij}(\vec x_i - \vec x_j,\ \dot{\vec x}_i - \dot{\vec x}_j)$ holds in one frame, the same equations hold in every boosted frame.
Proof. $\vec x_i' = \vec x_i - \vec vt$ gives $\ddot{\vec x}_i' = \ddot{\vec x}_i$, and differences of positions and of velocities are unchanged. $\square$
The laws of physics take the same form in every inertial frame. Newton's mechanics satisfies it for the Galilean group, which is how unit 03 could say "an" inertial frame.
25 · covariance
Let a group $G$ act on spacetime $U$ by bijections $y \mapsto \varphi_g(y)$, with $\varphi_{gh} = \varphi_g\circ\varphi_h$, and let $\rho : G \to GL(V)$ be a homomorphism. For a field $u : U \to V$ put $$(g\cdot u)(y) = \rho(g)\,u\big(\varphi_g^{-1}(y)\big).$$ This is an action: $(gh)\cdot u = g\cdot(h\cdot u)$.
A linear system $Pu = 0$ is $G$-covariant if $g\cdot u$ is a solution whenever $u$ is, for every $g \in G$. The operator $P$ is invariant up to a factor if $P(g\cdot u) = \lambda(g)\,g\cdot(Pu)$ for scalars $\lambda(g) \ne 0$.
$\big(g\cdot(h\cdot u)\big)(y) = \rho(g)\rho(h)\,u\big(\varphi_h^{-1}\varphi_g^{-1}y\big) = \rho(gh)\,u\big(\varphi_{gh}^{-1}y\big)$. $\square$
Here $y = (t, \vec x)$, $g$ is a change of frame, and $u$ is a scalar field or the six components of $(\vec E, \vec B)$. The matrix $\rho(g)$ says how the components mix: a scalar has $\rho = 1$; for $(\vec E, \vec B)$, working out $\rho$ is part of the problem.
The principle of relativity for a field theory is: the equations are covariant under the group relating inertial frames. Invariance of $P$ implies covariance, since $Pu = 0$ gives $P(g\cdot u) = \lambda\,g\cdot 0 = 0$.
25 · covariance
Let a group $H$ act on fields, and $S$ be the solution set of $Pu = 0$. Then $$\mathrm{Sym}(P) = \{\,g\in H : g\cdot S = S\,\}$$ is a subgroup of $H$. A subgroup $G \le H$ has $G\cdot S \subseteq S$ if and only if $G \le \mathrm{Sym}(P)$.
If $g\cdot S = S$ and $h\cdot S = S$ then $(gh)\cdot S = g\cdot(h\cdot S) = S$, and applying $g^{-1}$ to $g\cdot S = S$ gives $S = g^{-1}\cdot S$. For the second claim: $G\cdot S\subseteq S$ gives, for $g\in G$, $S = g\cdot(g^{-1}\cdot S) \subseteq g\cdot S \subseteq S$. $\square$
So the question "which changes of frame preserve Maxwell's equations?" has a group for its answer. It is not a list of lucky coincidences, and it can be found by computing the symmetries of one operator.
Take $H$ = invertible linear maps of the $(t,x)$-plane acting on scalar fields, and $P = \partial_t^2 - c^2\partial_x^2$. Section 2 shows no Galilean boost with $v\ne0$ is in $\mathrm{Sym}(P)$. Section 4 computes $\mathrm{Sym}(P)\cap H$. Section 5 identifies it.
section 2
The chain rule, applied once. Terms appear that no choice of speed and no redefinition of the field can remove — and in Maxwell's equations they sit exactly where unit 24 put the displacement current.
25 · the boost fails
Let $(x', t') = (ax + bt,\ dx + et)$ with $ae - bd \ne 0$, and write a scalar field in the new variables: $u(x,t) = u'(x', t')$. The chain rule (unit 03) gives
$$\partial_x = a\,\partial_{x'} + d\,\partial_{t'},\qquad \partial_t = b\,\partial_{x'} + e\,\partial_{t'} .$$Squaring, with Clairaut to merge the mixed partials,
$$\begin{aligned}\partial_t^2 - c^2\partial_x^2 \;=\;& (e^2 - c^2d^2)\,\partial_{t'}^2 \\ &+ 2(be - c^2ad)\,\partial_{x'}\partial_{t'} \\ &+ (b^2 - c^2a^2)\,\partial_{x'}^2 .\end{aligned}$$This is unit 18's theorem $\tilde A = JAJ^{\mathsf T}$ for the symbol matrix $A = \mathrm{diag}(1, -c^2)$ in the order $(t, x)$, with $J = \begin{pmatrix} e & d\\ b & a\end{pmatrix}$ the Jacobian of $(t,x)\mapsto(t',x')$. No lower-order terms arise, because the map is linear.
$\partial_x$ is not $\frac{1}{a}\partial_{x'}$. A new coordinate depends on both old ones, so each old derivative is a combination of both new ones — the coefficients are the columns of the Jacobian. Getting this backwards is the commonest error in this unit.
25 · the boost fails · example
Step 1, the map. $x' = x - vt$, $t' = t$: so $a = 1$, $b = -v$, $d = 0$, $e = 1$.
Step 2, the derivatives. $\partial_x = \partial_{x'}$ and $\partial_t = \partial_{t'} - v\,\partial_{x'}$. The time derivative picks up a space derivative: at fixed $x$, $x'$ runs backwards at rate $v$.
Step 3, the coefficients. $e^2 - c^2d^2 = 1$; $\ be - c^2ad = -v$; $\ b^2 - c^2a^2 = v^2 - c^2$.
Step 4, the result.
$$P = \partial_{t'}^2 \;-\; 2v\,\partial_{x'}\partial_{t'} \;-\; (c^2 - v^2)\,\partial_{x'}^2 .$$Step 5, what it predicts. Put $u' = e^{\mathrm i(kx' - \omega t')}$: $\ -\omega^2 - 2vk\omega + (c^2 - v^2)k^2 = 0$, so $\omega = (\pm c - v)k$. Waves run at $c - v$ one way and $c + v$ the other.
Dimensions: $v\,\partial_{x'}\partial_{t'}$ and $v^2\partial_{x'}^2$ both have the dimensions of $\partial_{t'}^2$ ✓.
Limit $v \to 0$: $P$ comes back ✓.
Special case: the speeds $c \mp v$ are exactly Galileo's addition of velocities applied to a signal moving at $\pm c$ in the old frame ✓ — the operator knows the rule it was transformed by.
The next slide draws step 5: the two light lines, before and after the boost.
25 · the boost fails
The new operator is a perfectly good hyperbolic operator — Sylvester (unit 18) guarantees the type survives, so there are still two families of characteristics. What does not survive is the form: the characteristics are no longer symmetric about the time axis, and in the moving frame light is not isotropic.
For the Earth's orbital speed, $v/c = 1.0\times10^{-4}$: the lean is $10^{-4}$ rad, invisible in a drawing and, it will turn out, invisible to every experiment.
Spacetime diagrams, time up, with $v = 0.4c$ (exaggerated). Left: a flash at the origin spreads at $c$ both ways (dots, one time unit later). Right: the same two light lines in Galileo's coordinates lean to the left — $c - v$ forwards, $c + v$ backwards — away from the dashed lines where isotropic light would run.
25 · the boost fails
For $v \ne 0$, the Galilean boost is not a symmetry of $P = \partial_t^2 - c^2\partial_x^2$ — not even if the field is also multiplied by any smooth nowhere-zero function $m(x,t)$, and not even up to any smooth nowhere-zero factor $\lambda(x,t)$.
Multiplying $u'$ by $m$ adds only first- and zeroth-order terms (product rule), so it cannot change the second-order part — the principal symbol (unit 18). The boosted symbol is $\tau^2 - 2v\tau\xi - (c^2 - v^2)\xi^2$ in the dual variables $(\tau,\xi)$ of $(t',x')$, and $\lambda(\tau^2 - c^2\xi^2)$ has no $\tau\xi$ term. They are equal only if $v = 0$. $\square$
"The solution set is carried onto itself" is weaker than "the operator is preserved", so the theorem needs one more step: the notes show that for this $P$ the two are equivalent. The slide's claim is therefore about solution sets — about physics.
Galilean covariance with a multiplier is not a vacuous escape. The heat equation $u_t = ku_{xx}$ is Galilean-covariant once the field is multiplied by $e^{-vx/2k + v^2t/4k}$ (problem P3). The wave operator is not, and the obstruction is in its symbol, where no multiplier reaches.
25 · the boost fails
A covariant theory needs $\rho$: how the field components mix. For electromagnetism Galileo's own mechanics supplies it. A charge $q$ with velocity $\vec u$ feels the Lorentz force of unit 23; in the boosted frame it has velocity $\vec u - \vec v$, and Galilean forces are the same in both frames. So for every $\vec u$,
$$q\big(\vec E' + (\vec u - \vec v)\times\vec B'\big) \;=\; q\big(\vec E + \vec u\times\vec B\big).$$$$\vec B' = \vec B,\qquad \vec E' = \vec E + \vec v\times\vec B,$$ both evaluated at the same event.
Proof. $\vec u = \vec v$ gives $\vec E' = \vec E + \vec v\times\vec B$. Substituting back leaves $\vec u\times(\vec B' - \vec B) = \vec 0$ for all $\vec u$, so $\vec B' = \vec B$. $\square$
Dimensions: $[vB] = \mathrm{m\,s^{-1}\cdot T} = \mathrm{V\,m^{-1}}$ ✓.
Limit $\vec v \to \vec 0$: the identity ✓.
Special case: in a pure magnetic field, a charge at rest in the moving frame feels $q\,\vec v\times\vec B$ in the old one and $q\vec E'$ in the new; the formula makes them the same force ✓.
Unit 23's handover slide promised that $\vec v\times\vec B$ depends on the frame. This is that dependence made into a rule. It is linear in the fields — a $6\times6$ matrix $\rho(\vec v)$ — which is what the next example needs.
25 · the boost fails · example
Step 1, a solution. In vacuum (unit 24), $\vec E = E_0\cos(kx - \omega t)\,\hat y$, $\vec B = \frac{E_0}{c}\cos(kx - \omega t)\,\hat z$ with $\omega = ck$.
Step 2, move the argument. At the event $(x', t')$, $x = x' + vt'$ and $t = t'$, so the phase is $kx' - (\omega - kv)t' = kx' - \omega't'$ with $\omega' = k(c - v)$.
Step 3, mix the components. Any invertible $\rho$ — Galileo's, or any other constant one — gives primed components that are constants times $\cos(kx' - \omega't')$, not all zero. With Galileo's: $\vec E' = E_0(1 - \tfrac vc)\cos(\cdot)\,\hat y$.
Step 4, test it. Every component of a vacuum Maxwell field obeys $P' = \partial_{t'}^2 - c^2\partial_{x'}^2$. On $\cos(kx' - \omega't')$:
$$\begin{aligned}P'\cos(\cdot) &= \big(c^2k^2 - \omega'^2\big)\cos(\cdot)\\ &= k^2v(2c - v)\cos(\cdot) \ne 0 .\end{aligned}$$For $0 \lt |v| \lt 2c$ and any constant invertible $\rho$, the boosted light wave is not a vacuum solution. Maxwell's equations are not covariant under Galilean boosts.
Dimensions: $k^2v(2c - v)$ is $\mathrm{s^{-2}}$, as $\partial_{t'}^2$ ✓. Limit $v \to 0$: $0$ ✓. Size: relative to $c^2k^2$ it is $2\beta - \beta^2$, with $\beta = v/c$: $2.0\times10^{-4}$ for the Earth's speed.
The wave in the new frame moves at $c - v$. Maxwell's equations, with their $\varepsilon_0$ and $\mu_0$, allow only $c$.
25 · the boost fails
With $\vec E' = \vec E + \vec v\times\vec B$, $\vec B' = \vec B$ and $\vec x' = \vec x - \vec vt$, $t' = t$: $$\nabla'\!\cdot\vec B' = 0,\qquad \nabla'\times\vec E' + \partial_{t'}\vec B' = \vec 0$$ hold whenever the unprimed equations do.
Proof. $\nabla' = \nabla$ and $\partial_{t'} = \partial_t + \vec v\cdot\nabla$ on fields at a fixed event. Then $\nabla\times(\vec v\times\vec B) = \vec v(\nabla\!\cdot\vec B) - (\vec v\cdot\nabla)\vec B$ (unit 23's product rule for curls, with $\vec v$ constant), and the $(\vec v\cdot\nabla)\vec B$ terms cancel. $\square$
In vacuum, on worked example 2's wave, $$\nabla'\times\vec B' - \frac{1}{c^2}\partial_{t'}\vec E' = \frac{E_0k}{c}\,\big(2\beta - \beta^2\big)\sin(kx' - \omega't')\,\hat y \ne \vec 0 .$$ Faraday's law and $\nabla\cdot\vec B = 0$ are Galilean; the term Maxwell added in 1862 — the one that makes light — is the one that is not.
Drop the displacement current and the rest is a consistent Galilean theory, the magnetic limit of electromagnetism (cited: Le Bellac and Lévy-Leblond, 1973). But it has no light in it.
section 3
If Maxwell and Galileo disagree, either Maxwell holds in only one frame, or light is not what Maxwell says, or Maxwell is wrong. Each was tried, each made a prediction, and each prediction failed.
25 · three ways out
| response | claim | what it predicts | killed by |
|---|---|---|---|
| an ether | Maxwell holds in one frame only, the rest frame of a medium; elsewhere the boosted operator of worked example 1 is correct | light at $c \mp v$ in the lab, so an ether wind of order $\beta = 10^{-4}$ or $\beta^2 = 10^{-8}$ | Michelson–Morley, 1887 |
| emission | light leaves its source at $c$ relative to the source, as a thrown ball would | light from an approaching star arrives early; double stars look scrambled | de Sitter, 1913 |
| new Maxwell | replace Maxwell's equations by Galilean-covariant ones | moving matter drags light with it completely | Fizeau, 1851 — already on the books |
The medium whose rest frame, the ether frame, is the one frame where $Pu = 0$ holds. Light's transverse polarisation (unit 24) made it an elastic solid, stiff enough to carry waves at $3\times10^8\ \mathrm{m\,s^{-1}}$, yet offering no measurable drag to the planets.
Keep Maxwell exactly and give up Galileo. Nobody took it seriously until the other three had failed, because it means changing $t' = t$ — the hypothesis Newton never stated.
25 · three ways out
Stars appear displaced towards the direction of the Earth's motion by up to $\arctan(v/c)$, cycling yearly. With $v = 29.78\ \mathrm{km\,s^{-1}}$ that is $9.93\times10^{-5}$ rad $= 20.49''$ — what Bradley measured.
It is rain on a moving car: the telescope must be tilted because it moves while the light crosses it. It needs light to arrive through a medium not dragged along by the Earth — a stationary ether.
So by 1728 the ether, if there is one, does not move with the Earth. The next slide finds that moving water does drag light — but only partly.
In a frame where the starlight falls straight down: while it falls the tube's length, $cT$, the tube moves $vT$. To keep the light on its axis the tube must lean forward by $\alpha$, $\tan\alpha = v/c$. Schematic, with $v/c$ exaggerated to $0.3$; the real $\alpha$ is $20.49''$.
25 · three ways out
Light in water of refractive index $n$, moving at $w$, travels in the lab at $$\frac cn + f\,w,\qquad f = 1 - \frac{1}{n^2}\ \ \text{(Fresnel, 1818)}.$$ For water, $n = 1.333$: $f = 0.437$. Measured by Michelson and Morley in 1886: $0.434 \pm 0.02$.
Not $f = 0$ (stationary ether) and not $f = 1$ (dragged ether): moving water drags light by 44%, a number with no mechanism behind it. Section 5 derives it.
Schematic. The two beams share one loop, so every length and mirror is common to both; only the water's motion distinguishes them. The difference of their travel times, $\propto f\,w$, moves the fringes when the flow is reversed.
25 · three ways out · example
Setup. A Michelson interferometer: two arms of length $L$ at right angles, one along the wind $v$. Work in the ether frame, where light moves at $c$.
Along. Out at $c - v$ relative to the mirror, back at $c + v$: $t_\parallel = \frac{L}{c - v} + \frac{L}{c + v} = \frac{2L}{c}\gamma^2$, $\ \gamma^2 = \frac{1}{1 - \beta^2}$.
Across. The light must aim upwind, crossing at $\sqrt{c^2 - v^2}$: $t_\perp = \frac{2L}{c}\gamma$.
Difference. $c(t_\parallel - t_\perp) = 2L(\gamma^2 - \gamma) = L\beta^2 + O(\beta^4)$.
Rotate by 90°. The arms swap roles, so the fringes move by $$\Delta N = \frac{2L\beta^2}{\lambda} = \frac{2(11\ \mathrm m)(1.0\times10^{-8})}{5.5\times10^{-7}\ \mathrm m} = 0.40 .$$
Dimensions: $L\beta^2/\lambda$ is a pure number ✓. Limit $v\to0$: $\Delta N \to 0$ ✓. Second order: the first-order terms cancel on the round trip — which is why nothing before 1881 could see the wind.
Here $\beta = v/c$, $\gamma = 1/\sqrt{1 - \beta^2}$ is shorthand for the factor that falls out of the algebra, and $\lambda$ is the wavelength of the light. The next slide draws both round trips, and gives the verdict.
25 · three ways out
Left: along the motion the light chases a receding mirror at $c - v$, then meets the splitter at $c + v$. Right: across it, in the ether frame, the light must aim ahead to hit a mirror that has moved $vT$; it runs the hypotenuse $cT$, so $c^2T^2 = L^2 + v^2T^2$. Schematic, $v/c$ exaggerated to $0.5$.
Along: $t_\parallel = \frac{2L}{c}\gamma^2$. Across: $t_\perp = \frac{2L}{c}\gamma$. The across trip is quicker by one factor of $\gamma$; rotating the slab $90°$ swaps the arms and should move the fringes by $0.40$.
Michelson and Morley, Cleveland, July 1887: the shift was "probably less than the fortieth part" of $0.40$ — below $0.01$ fringe, at noon and in the evening. Later repetitions at other seasons agreed.
Worked example 1's operator predicts $c - v$ and $c + v$. This is that operator, tested at second order, and it fails.
25 · three ways out
| ether model | aberration | Fizeau, $f = 0.437$ | Michelson–Morley |
|---|---|---|---|
| stationary, Fresnel's partial drag | ✓ | ✓ (by fiat) | ✗ predicts $0.40$ |
| completely dragged near the Earth (Stokes, 1845) | ✗ | ✗ predicts $f = 1$ | ✓ |
| stationary + contraction hypothesis | ✓ | ✓ (by fiat) | ✓ |
A body moving through the ether at $v$ shortens along its motion by the factor $\sqrt{1 - \beta^2}$. Then $t_\parallel$ becomes $\frac{2L}{c}\gamma^2\cdot\frac1\gamma = \frac{2L}{c}\gamma = t_\perp$: the null result, exactly, at every speed.
The third row fits by adjusting one new function per experiment. For the Earth at $30\ \mathrm{km\,s^{-1}}$ the contraction of its diameter is $6.4$ cm. Section 5 finds that both patches — Fresnel's $f$ and this — fall out of the substitution section 4 derives.
25 · three ways out
Light leaves its source at $c$ relative to the source, and keeps the source's velocity: Galilean addition applied to light. Michelson–Morley's null result is then automatic, since source and mirrors share one frame.
It keeps Galileo and gives up Maxwell's field theory: the wave equation's solutions travel at the $c$ in the operator, whatever the source did (notes).
A star in a binary orbit, speed $u$, distance $D$. Light emitted while approaching arrives earlier than light emitted while receding by $$\Delta t = \frac{D}{c - u} - \frac{D}{c + u} \approx \frac{2Du}{c^2}.$$
Dimensions: $Du/c^2$ is $\mathrm{m\cdot m\,s^{-1}/m^2\,s^{-2}} = \mathrm s$ ✓. Limit $u\to0$: no effect ✓.
25 · three ways out
$u = 100\ \mathrm{km\,s^{-1}}$, $D = 1000$ light-years $= 9.46\times10^{18}$ m: $\ \Delta t = 2.11\times10^7$ s $= 244$ days.
A binary with a period of days would show several images of each star at once, and a Doppler curve scrambled beyond recognition. Spectroscopic binaries show clean Keplerian orbits.
The figure takes a period of 100 days, so that the curve can still be drawn. Shorter periods fold it more often, and give more images.
Under an emission theory, light leaves at $c + u_r$, with $u_r = u\sin(2\pi t/100\ \mathrm{d})$ the star's velocity towards us. Arrival time against emission time swings $\pm 122$ days about the dashed line, so it doubles back: on one night (the dashed horizontal line) light from five moments of the orbit arrives together.
25 · three ways out
Replace each $\partial_t$ in Maxwell's equations by the derivative following the moving matter, $\partial_t + \vec w\cdot\nabla$, as unit 22's material derivative would. The equations become Galilean-covariant by construction, in the way the boosted operator of worked example 1 would become $P$ again if $v$ were the local velocity of the medium.
Light in a medium is carried completely by it: $f = 1$ in Fizeau's formula. The measured $f$ is $0.434 \pm 0.02$.
Every other test pointed the same way. Maxwell's $c = 1/\sqrt{\varepsilon_0\mu_0}$ from two bench-top constants matched the speed of light (unit 24). Hertz himself produced radio waves in 1887–88 and showed they reflect, refract and polarise as light does, at a finite speed comparable with light's.
Maxwell's equations are right. They hold in the lab to $10^{-8}$ though the lab moves. Galilean relativity forbids both at once. Of the four premises — Maxwell, relativity, Galileo, and the unstated $t' = t$ — something in the last two must go.
section 4
Keep Maxwell, keep the principle of relativity, and ask the chain rule which linear change of frame leaves the wave operator alone. Two conditions; one family; $c$ already inside it.
25 · the right substitution
Look for an invertible linear map $(x', t') = (ax + bt,\ dx + et)$ describing a frame whose origin moves at velocity $v$. Then:
The second demand is not "Maxwell holds in the new frame by assumption about light". It is the principle of relativity, applied to Maxwell's equations as they stand.
From the coefficient formula of section 2, form-invariance is (i) no cross term and (ii) the right ratio:
$$\begin{aligned}\text{(i)}\quad & be - c^2ad = 0,\\ \text{(ii)}\quad & b^2 - c^2a^2 = -c^2\,(e^2 - c^2d^2).\end{aligned}$$Equivalently: the two families of characteristics, $x \pm ct = $ const, are each carried to themselves.
Four unknowns $a, b, d, e$; $v$ fixes $b$ in terms of $a$; two conditions leave one free number.
25 · the right substitution · example
Step 1, use $b = -va$ in (i). $-vae - c^2ad = 0$, and $a \ne 0$ (else $x'$ would not depend on $x$ and the map would send the line $t = 0$ to a point of $x'$), so $$d = -\frac{v}{c^2}\,e .$$
Step 2, use both in (ii). Left: $v^2a^2 - c^2a^2 = -c^2a^2(1 - \beta^2)$. Right: $-c^2(e^2 - v^2e^2/c^2) = -c^2e^2(1 - \beta^2)$. So, for $|v| \ne c$, $$a^2 = e^2 .$$
Step 3, pick the branch. At $v = 0$ the map must be the identity, and $a, e$ depend continuously on $v$ and never vanish, so $a = e \gt 0$. Call it $A(v)$.
Step 4, the family. $$x' = A(v)\,(x - vt),\qquad t' = A(v)\Big(t - \frac{v x}{c^2}\Big),$$ and then $P = A^2(1 - \beta^2)\,\big(\partial_{t'}^2 - c^2\partial_{x'}^2\big)$.
Dimensions: $vx/c^2$ is $\mathrm{m\,s^{-1}\cdot m/m^2\,s^{-2}} = \mathrm s$ ✓.
Limit $c\to\infty$: $t' = At$, $x' = A(x - vt)$; with $A = 1$ this is Galileo ✓.
Light: $x = ct$ gives $x' = A(c - v)t$ and $t' = A(1 - \beta)t$, so $x' = ct'$ ✓. The invariant speed is $c$, in both directions.
One function, $A(v)$, is still free — and $P$ cannot fix it, since a dilation $(x,t)\mapsto(sx, st)$ multiplies $P$ by $s^{-2}$ and is a symmetry.
25 · the right substitution
The new coordinates drawn in the old frame, $v = c/2$, with $A = \gamma = 1.155$. Solid: lines of constant $x'$; dashed: lines of constant $ct'$, one unit apart. The light lines $x = \pm ct$ pass exactly through the grid's corners where $x' = \pm ct'$ (dots).
Galileo's map tilts only the lines of constant $x'$; its lines of constant $t'$ stay horizontal. This one tilts both, by the same angle, towards the light line: the $x'$-axis ($t' = 0$, the line $t = vx/c^2$) is the mirror image of the $t'$-axis ($x = vt$) in $x = ct$.
Condition (i) is that mirror symmetry. Condition (ii), $a = e$, spaces the two families alike, so each light line runs along the diagonals of the cells: each family of characteristics goes to itself.
The cross term died because $t'$ now depends on $x$. The new clocks are set differently at different places: "at the same time" is frame-dependent. That is the price, and it is the whole of it.
25 · the right substitution
In space, $P = \partial_t^2 - c^2(\partial_x^2 + \partial_y^2 + \partial_z^2)$. Keep the boost along $x$, and let $y' = sy$, $z' = sz$ with a transverse scale factor $s \gt 0$ (isotropy about the $x$-axis makes the two equal). The $(x,t)$ part is as before, and the transverse part becomes $-c^2s^2(\partial_{y'}^2 + \partial_{z'}^2)$. Form-invariance now needs
$$A^2(1 - \beta^2) = \lambda = s^2 .$$The boost-shaped linear maps preserving $P$ up to a factor are exactly $$x' = s\gamma(x - vt),\ \ t' = s\gamma\Big(t - \frac{vx}{c^2}\Big),\ \ y' = sy,\ \ z' = sz,$$ with $\gamma = (1 - \beta^2)^{-1/2}$, $|v| \lt c$, and $s = s(v) \gt 0$ free.
$\lambda = s^2 \gt 0$ forces $1 - \beta^2 \gt 0$, i.e. $|v| \lt c$; then $A = s/\sqrt{1 - \beta^2} = s\gamma$ (positive root, as before). Conversely, each such map multiplies $P$ by $s^2$. $\square$
Dimensions: $\gamma$ and $s$ are pure numbers ✓. Limit $v\to0$: $\gamma\to1$, a pure dilation by $s(0)$, which must be $1$ ✓. Special case: $s = 1/\gamma$ gives $A = 1$, worked example 4's Voigt case ✓.
The speed limit $|v| \lt c$ has appeared, and nothing about particles or energy was used: it is a statement about which linear maps a hyperbolic operator with three space directions allows.
25 · the right substitution
Write $L_s(v)$ for the map of the family at velocity $v$, with its scale $s = s(v)$. The principle of relativity, once more: the old frame's origin moves at $-v$ in the new frame (check: $x = 0$ gives $x' = -vt'$), so the inverse map must be the same rule with $-v$: $$L_s(v)^{-1} = L_s(-v).$$
A half-turn about the $z$-axis, $(x,y)\mapsto(-x,-y)$, turns the boost at $v$ into the boost at $-v$ without changing its transverse lengths: $s(-v) = s(v)$.
Write $L_s(v) = s(v)\,\Lambda(v)$, $\Lambda$ the $s = 1$ map. Direct multiplication gives $\Lambda(v)\Lambda(-v) = I$. Reciprocity then says $s(v)^{-1}\Lambda(-v) = s(-v)\Lambda(-v)$, so $s(v)s(-v) = 1$; isotropy makes it $s(v)^2 = 1$; and $s \gt 0$. $\square$
Voigt's transformation, $s = 1/\gamma$, preserves $P$ up to the factor $1/\gamma^2$ — but its inverse is $\gamma\Lambda(-v)$, not $\gamma^{-1}\Lambda(-v)$. The two frames would disagree about which of them had the shrunken rulers.
25 · the right substitution
with the Lorentz factor $\gamma = 1/\sqrt{1 - v^2/c^2}$, $|v| \lt c$. It carries $P$ to $P'$ exactly: $\lambda = s^2 = 1$.
Dimensions: $\gamma$ is a number, $vx/c^2$ a time ✓.
Limit $c \to \infty$: $\gamma \to 1$, $vx/c^2 \to 0$: Galileo ✓.
Size at $30\ \mathrm{km\,s^{-1}}$: $\gamma - 1 = 5.0\times10^{-9}$; $\ vx/c^2$ over $x = 1$ km is $3.3\times10^{-10}$ s.
Light: $x = \pm ct \iff x' = \pm ct'$ ✓.
$\partial_x = \gamma\big(\partial_{x'} - \tfrac{v}{c^2}\partial_{t'}\big)$, $\ \partial_t = \gamma\big(\partial_{t'} - v\,\partial_{x'}\big)$, and
$$\begin{aligned}\partial_t^2 - c^2\partial_x^2 &= \gamma^2\big[(1 - \beta^2)\partial_{t'}^2 + 0\cdot\partial_{x'}\partial_{t'}\\ &\qquad - c^2(1 - \beta^2)\partial_{x'}^2\big]\\ &= \partial_{t'}^2 - c^2\partial_{x'}^2 .\end{aligned}$$Worked example 1's $-2v\,\partial_{x'}\partial_{t'}$ is cancelled by $+2v\,\partial_{x'}\partial_{t'}$ from the $-\tfrac{v}{c^2}\partial_{t'}$ in $\partial_x$ — the term Galileo did not have.
25 · the right substitution
The Lorentz boost; the speed limit $|v| \lt c$; that $c$ is the same in every frame; and its value, $1/\sqrt{\varepsilon_0\mu_0}$, read off the operator.
Einstein's 1905 postulates were the principle of relativity and the constancy of the speed of light. Here the second is a theorem: the principle of relativity, applied to Maxwell's equations as they were already written, has no room for any other invariant speed.
"Maxwell holds in every frame with the same $\varepsilon_0, \mu_0$" contains the constancy of $c$, so no magic has happened: the postulate has been located inside a principle everyone already believed and an equation everyone already trusted. Unit 26 derives the same group with the invariant speed as an unknown, and cites this slide for its value.
section 5
Lorentz's local time and FitzGerald's contraction were two patches; Poincaré saw they were one group. Its composition law explains Fizeau, its larger cousin is the conformal group, and its free function is fixed by one experiment.
25 · a group
In a frame moving through the ether at $v$, use the Galilean position $x' = x - vt$ but the clock reading $$t_{\mathrm{loc}} = t - \frac{vx}{c^2}.$$ Lorentz called it a mathematical aid, not the time.
It is worked example 4 with $A = 1$: to all orders in 1+1 dimensions it kills the cross term, and $P = (1 - \beta^2)(\partial_{t_{\mathrm{loc}}}^2 - c^2\partial_{x'}^2)$. The leftover factor is harmless in 1+1; in 3+1 it clashes with the transverse terms at order $\beta^2$.
| patch | in the family | order in $\beta$ |
|---|---|---|
| local time, 1895 | $t' \ni -vx/c^2$ | first |
| contraction, 1889–92 | $x' = \gamma(x - vt)$ | second |
| time dilation, Larmor 1897–1900 | $t' = \gamma(\cdots)$ | second |
| $\ell = 1$, Poincaré 1905 | $s = 1$ | — |
All four rows are one map. The next slide shows the contraction falling out of it.
25 · a group
A rod at rest in the new frame, drawn in the old one with $v = 0.6c$, $\gamma = 1.25$. Its ends sweep out the strip between $x' = 0$ and $x' = L$. Cut across at one old time and the strip is $L/\gamma = 0.8L$ wide; cut along a line of constant $t'$ and it is the rod's own length $L$.
A rod at rest in the new frame, $x' \in [0, L]$, occupies $x \in [vt, vt + L/\gamma]$ at old time $t$: contraction by $1/\gamma$, derived rather than hypothesised.
FitzGerald and Lorentz needed the contraction as a separate hypothesis about matter. Here it is a statement about which events count as "the ends, at the same time" — and the two frames answer differently.
25 · a group
$\Lambda(u)\,\Lambda(v) = \Lambda(w)$ with $$w = \frac{u + v}{1 + uv/c^2}.$$ With $\Lambda(v)^{-1} = \Lambda(-v)$ and $\Lambda(0) = I$, the boosts along $x$ form a group.
In the order $(x, t)$, $\Lambda(v) = \gamma_v\begin{pmatrix}1 & -v\\ -v/c^2 & 1\end{pmatrix}$. The product has diagonal entries $\gamma_u\gamma_v(1 + uv/c^2)$ and off-diagonal entries $-\gamma_u\gamma_v(u + v)$ and $-\gamma_u\gamma_v(u + v)/c^2$ — the shape of $\Lambda(w)$, with prefactor $\gamma_u\gamma_v(1 + uv/c^2) = \gamma_w$ (notes). $\square$
Together with rotations, these generate the Lorentz group (Poincaré's name, 1905), and by the lemma of section 1 it is a subgroup of the symmetry group, among linear maps, of Maxwell's vacuum equations — the whole of it, once unit 28 supplies the $\rho$ that makes the full system covariant (cited). Adding the four translations gives the ten changes of inertial frame. Unit 26 parametrises it properly.
25 · a group
Dimensions: $uv/c^2$ is a pure number, $w$ a speed ✓.
Limit $c\to\infty$: $w = u + v$, Galileo's addition ✓.
Light: $u = c$ gives $w = (c + v)/(1 + v/c) = c$ for every $v$ ✓.
Number: $u = v = c/2$ gives $w = 0.8c$ ✓.
Galileo's sum crosses $c$ as soon as $u + v \gt c$. The composition law bends every curve over so that it reaches $c$ exactly at $u = c$ — light composed with anything is still light — and never above.
$w = (u + v)/(1 + uv/c^2)$ against $u$, for $v = c/2$ and $v = 0.9c$. The dotted line is Galileo's $u + c/2$; the open circle is where it says $c/2$ plus $c/2$ is $c$, and the dot is the composition law's $0.8c$.
25 · a group · example
Step 1, the rest frame of the water. There light moves at $u = c/n$: the water is at rest, and its refractive index is a property of the water at rest.
Step 2, the lab. The water moves at $w$ in the lab, so compose: $$u_{\mathrm{lab}} = \frac{c/n + w}{1 + w/(nc)} .$$
Step 3, expand in $w/c$. $\frac{1}{1 + w/nc} = 1 - \frac{w}{nc} + O(w^2/c^2)$, so $$u_{\mathrm{lab}} = \frac cn + w - \frac{w}{n^2} + O\Big(\frac{w^2}{c}\Big) = \frac cn + \Big(1 - \frac1{n^2}\Big)w + \dots$$
Step 4, read off. $f = 1 - 1/n^2$: Fresnel's coefficient, $0.437$ for water, with no ether in sight.
Dimensions: $w/(nc)$ is a pure number ✓.
Limit $n\to1$: $f\to0$ — vacuum is not dragged, and $u_{\mathrm{lab}} = c$ exactly ✓.
Limit $n\to\infty$: $f\to1$ — light stuck in the medium goes where it goes ✓.
Size: at $w = 7.059\ \mathrm{m\,s^{-1}}$, the first-order drag is $3.086\ \mathrm{m\,s^{-1}}$ and the next term $-5.5\times10^{-8}\ \mathrm{m\,s^{-1}}$.
The next slide sets the derived coefficient against the two ether theories it replaces.
25 · a group
A coefficient that took an ether, a partial drag and sixty years of argument is two lines of the group law. It is Galileo's addition, $u + w$, that was wrong for light in water — Hertz's $f = 1$.
A stationary ether says light in moving water ignores the water: $f = 0$. A dragged ether, or Hertz's equations, say the water carries it fully: $f = 1$. The composition law says $f = 1 - 1/n^2$ — between the two, near $0$ for thin media and near $1$ for dense ones.
The drag coefficient against refractive index. Water sits on the curve: $1 - 1/1.333^2 = 0.437$, against Michelson and Morley's $0.434 \pm 0.02$ (bar). Both ether lines miss it by far more than the error.
25 · a group
In units with $c = 1$, the invertible linear maps under which $P = \partial_t^2 - \partial_x^2$ is invariant up to a factor are exactly $\mu M$ and $\mu MS$ with $\mu \gt 0$, $M$ in the group $O(1,1)$ of maps preserving $t^2 - x^2$, and $S$ the swap $(t,x)\mapsto(x,t)$.
$O(1,1)$ has four pieces: the boosts, and the boosts composed with $x\mapsto-x$, with $t\mapsto -t$, and with both. The dilations $\mu$ are what $P$ cannot see, and why $s$ needed reciprocity.
The swap $S$ exchanges space and time; it is a symmetry of the 1+1 operator only, and the transverse slide excluded it in 3+1. Allow nonlinear maps and the group grows enormously — the next slide.
25 · a group
Allow nonlinear maps. In null coordinates $\xi = x - ct$, $\eta = x + ct$, $P = -4c^2\partial_\xi\partial_\eta$, and for any $C^2$ bijections $F, G$ of $\mathbb R$ with $F', G' \ne 0$, $$\partial_\xi\partial_\eta = F'(\xi)\,G'(\eta)\,\partial_{\xi'}\partial_{\eta'},\quad \xi' = F(\xi),\ \eta' = G(\eta).$$ Solutions go to solutions: in 1+1 the symmetry group is infinite-dimensional.
In 3+1 it is fifteen-dimensional: translations (4), Lorentz (6), dilation (1), and four "special conformal" maps — cited: Bateman and Cunningham, 1909–10. Only the ten Poincaré maps are changes of inertial frame.
Left: light lines $\xi = x - ct$ and $\eta = x + ct$ at even spacing, and a straight worldline. Right: the same lines after $\xi' = F(\xi)$, $\eta' = G(\eta)$ for two increasing functions — still light lines, so still the characteristics, but unevenly spaced; the worldline has bent.
25 · a group
Make the ether theory as general as possible — a test theory. In the frame where light is isotropic, an apparatus moving at $v$ has its lengths along and across the motion scaled by $\ell_\parallel(v), \ell_\perp(v)$, and its clocks run at rate $\tau(v)$. Round trips then give:
| experiment | measures | forces |
|---|---|---|
| Michelson–Morley, 1887 | equal arms, rotated | $\ell_\parallel/\ell_\perp = 1/\gamma$ |
| Kennedy–Thorndike experiment, 1932 | unequal arms, watched for months | $\tau\,\ell_\perp = 1/\gamma$ |
| Ives–Stilwell experiment, 1938 | moving atoms' frequency | $\tau = 1/\gamma$ |
A rod along $x'$ has $\ell_\parallel = 1/(s\gamma)$; across, $\ell_\perp = 1/s$; a clock at $x' = 0$ reads $t' = st/\gamma$, so $\tau = s/\gamma$. Then $\ell_\parallel/\ell_\perp = 1/\gamma$ ✓ and $\tau\ell_\perp = 1/\gamma$ ✓ for every $s$, and $\tau = 1/\gamma$ only for $s = 1$.
The next slide plots the Ives–Stilwell prediction for Lorentz, for Voigt, and for an ether with absolute time.
25 · a group
Both light-only experiments are blind to $s$, because the wave operator is: dilations are its symmetries. The one experiment with a material clock — time dilation of moving atoms — measures it. Voigt's $s = 1/\gamma$ predicts twice the Ives–Stilwell shift.
An atom moving at $\beta c$ emits at the rate $\tau\nu_0$, and seen forwards and backwards its line sits at $\lambda_0(1 \mp \beta)/\tau$. The mean of the two is shifted by $\lambda_0(1/\tau - 1)$: no first-order Doppler, only the clock.
The mean shift of the H$_\beta$ line, $\lambda_0 = 486.13$ nm, from atoms at speed $\beta c$, for three clock rates: Lorentz's $\tau = 1/\gamma$, Voigt's $\tau = 1/\gamma^2$, and absolute time, $\tau = 1$. At $\beta = 0.005$ (dots) the first two differ by a factor of two. Ives and Stilwell found the Lorentz value.
25 · a group
| Galileo | Lorentz | |
|---|---|---|
| map | $x - vt,\ \ t$ | $\gamma(x - vt),\ \ \gamma(t - vx/c^2)$ |
| $\partial_t$ | $\partial_{t'} - v\partial_{x'}$ | $\gamma(\partial_{t'} - v\partial_{x'})$ |
| $\partial_x$ | $\partial_{x'}$ | $\gamma(\partial_{x'} - \tfrac{v}{c^2}\partial_{t'})$ |
| cross term | $-2v\,\partial_{x'}\partial_{t'}$ | $0$ |
| light speeds | $c - v,\ \ c + v$ | $c,\ \ c$ |
| composition | $u + v$ | $(u+v)/(1 + uv/c^2)$ |
| $c \to \infty$ | — | Galileo |
The chain rule, applied to $P$ under $x' = x - vt$, produces a cross term; Maxwell's equations are therefore not Galilean-covariant, and the failure is exactly where the displacement current sits. Demanding that the cross term vanish, that the ratio be right, and that the frames be reciprocal leaves one answer, whose invariant speed is the $c$ written in $P$.
At $30\ \mathrm{km\,s^{-1}}$ the two columns differ by $\gamma - 1 = 5\times10^{-9}$ and by clocks offset $vx/c^2$. Every nineteenth-century experiment lived in that gap.
25 · what next
| 26 Minkowski | derives the boost from homogeneity, isotropy and the group axioms with the invariant speed unknown; this unit's wave operator fixes it at $c$. The symbol $\tau^2 - c^2|\vec\xi|^2$ becomes the bilinear form $\eta$. |
| 27 dynamics | Newton's law is Galilean-covariant and so must change; four-vectors are what the Lorentz group acts on. |
| 28 field tensor | the $\rho$ this unit could not find: $\vec E$ and $\vec B$ as one antisymmetric tensor, with sufficiency of the Lorentz boost proved. |
| 30 equivalence | a non-inertial frame is a nonlinear change of coordinates — the kind section 4 excluded — and the metric stops being constant. |
A law is the same in every frame when the equations are covariant under the group relating the frames, and the symmetries of an equation always form a group. Maxwell's operator acquires a cross term under a Galilean boost that no speed and no field redefinition removes. The linear maps that preserve it, made reciprocal, are the Lorentz boosts, and their invariant speed is the $c$ in the operator.
25 · checkpoint
On paper and without notes, you can:
A Galilean computation with no cross term (the chain rule went the wrong way); a Lorentz computation that leaves one; a derivation that writes "light moves at $c$ in both frames" as a premise; or a family with $s$ left free and called the answer.
26 Minkowski space, where this group becomes the geometry of a quadratic form · 28 after 27, where Maxwell's equations are shown covariant in full.