Part D · Minkowski · spine

28

Electromagnetism was relativistic all along: the field tensor

E and B are not two fields but two blocks of one antisymmetric tensor, and a boost stirs them into each other — which is why a neutral wire pulls on a charge moving beside it.

needs 27, 25~2½ h slides + 5 h problemsproblems: ./mr problems 28

28 · overview

One wire, five sections

the experiment

A neutral wire carries $I = 1.00$ A. A charge $q = 1.00$ nC, $r = 2.00$ cm away, moves parallel to it at $v = 3.00\times10^{6}\ \mathrm{m\,s^{-1}}$.

In the lab the force is magnetic, $q\vec v\times\vec B$. In the charge's own frame the charge is at rest, so there is no magnetic force — yet it is still pulled in. What supplies the force?

where the force comes from, in four steps

1. Lab: the wire is neutral, so $\vec E = 0$; Ampère gives $B = 10.0\ \mu$T and a force $qvB = 3.000\times10^{-8}$ N towards the wire.

2. Charge's frame: lattice and electrons move at different speeds, so their charge per metre contracts by different factors. The wire carries $\lambda' = -\gamma Iv/c^2$.

3. Gauss turns $\lambda'$ into a field $E'$ at the charge; $qE'$ is the force, larger than step 1's by exactly $\gamma$.

4. That factor is how force transforms, $F_\perp = F'_\perp/\gamma$: one effect, two descriptions.

The plan. 1 one field, forced to be antisymmetric · 2 boosting, and the wire done twice · 3 Maxwell as two equations; two invariants · 4 $T^{\mu\nu}$, and Poynting · 5 radiation, and the runaway nobody fixed.

getting around

Words with a dotted underline are glossary terms: click one for its definition. G lists every term in the unit, N shows the notes, where the longer proofs live. A solid underline, like the wire's invariants, is a piece of the running example, shown on hover.

section 1

One field, not two

What kind of object can push a charge around without changing its mass?

28 · one field

First, what a force is in spacetime

definition · four-force

For a worldline with four-momentum $p$, the four-force is $f = \mathrm{d}p/\mathrm{d}\tau$, a vector in $V$ at each event.

In a frame, $\mathrm{d}\tau = \mathrm{d}t/\gamma$ and $p = (E/c,\ \vec p)$, so

$$f^\mu = \gamma\Big(\tfrac1c\vec F\cdot\vec v,\ \ \vec F\Big),\qquad \vec F = \frac{\mathrm{d}\vec p}{\mathrm{d}t}.$$

Newton's three-force is the spatial part, divided by $\gamma$. The time part is the power, also divided by $\gamma$ — one object, not two.

constraint

For a particle of fixed mass, $\eta(p,p) = -m^2c^2$ is constant, so

$$\eta(f, u) = 0 .$$

One line: differentiate $\eta(p,p)$ along the worldline and use $p = mu$.

A four-force is never free: it must be $\eta$-orthogonal to the four-velocity at every event, or the particle's mass changes.

28 · one field

The constraint, drawn: $f$ is $u$ reflected in the light line

ct x worldline light u f

On a Minkowski diagram $\eta$-orthogonal is not a right angle. At each event of a worldline, $f$ is $u$ reflected in the light line through that event.

In one space dimension, $u = \gamma(c, v)$, and

$$\eta(f,u) = \gamma\big(-cf^0 + vf^1\big) = 0$$ $$\iff\quad \frac{f^0}{f^1} = \frac vc .$$

$u$ leans from the time axis by slope $v/c$; $f$ leans from the space axis by the same slope. Mirror images in the $45^\circ$ line.

two readings

At rest ($u$ vertical), $f$ is horizontal: $f^0 = 0$, a pure push, no power — the rest energy $mc^2$ cannot change.

As $v\to c$, $u$ and $f$ fold onto the light line together; neither ever crosses it.

28 · one field

The one guess, and what it forces

Unit 23's Lorentz force $\vec F = q(\vec E + \vec v\times\vec B)$ is linear in the velocity. Make the mildest possible relativistic guess: the four-force is linear in the four-velocity, with coefficients built from the field at that event and the charge,

$$f^\mu \;=\; q\,F^\mu{}_\nu\,u^\nu ,$$

for some array $F^\mu{}_\nu(x)$ of 16 numbers per event. Now impose the constraint $\eta(f,u)=0$ for every worldline through the event. Writing $F_{\mu\nu} := \eta_{\mu\alpha}F^\alpha{}_\nu$, the constraint reads $q\,F_{\mu\nu}u^\mu u^\nu = 0$.

theorem · antisymmetry is not assumed

If $F_{\mu\nu}u^\mu u^\nu = 0$ for every future-pointing timelike $u$ with $\eta(u,u)=-c^2$, then $F_{\mu\nu} = -F_{\nu\mu}$.

proof

Let $S_{\mu\nu} := \tfrac12(F_{\mu\nu} + F_{\nu\mu})$, the symmetric part; only it survives contraction with $u^\mu u^\nu$. $Q(w) := S_{\mu\nu}w^\mu w^\nu$ is a quadratic form vanishing on the open cone $\mathcal T$ (scaling $u$ scales $Q$ by $\lambda^2$, and every $w\in\mathcal T$ is some $\lambda u$). A polynomial vanishing on a nonempty open set vanishes identically, so $Q\equiv0$; polarisation gives $S = 0$. $\square$

w⁰ w¹ η(u, u) = −c² u λu 𝒯 open Q = 0 here too

A 2-d slice of $V$. $Q = 0$ on the hyperbola, hence on every ray through it, hence on the open shaded cone $\mathcal T$ — and a quadratic that vanishes on an open set vanishes everywhere.

28 · one field

The field tensor, defined

definition · the electromagnetic field tensor

A smooth assignment, to each event $x$ of Minkowski space, of an antisymmetric bilinear form $$F_x : V\times V \to \mathbb R,\qquad F_x(w,z) = -F_x(z,w),$$ that is, an antisymmetric $(0,2)$-tensor field. Its value on a pair of vectors is a number every frame agrees on.

This is unit 16's definition of a tensor, with $\mathbb R^3$ replaced by $V$ and the Euclidean inner product replaced by $\eta$. A tensor field on Minkowski space is just a tensor attached to every event, varying smoothly.

The physical content is one equation:

$$\boxed{\ \frac{\mathrm{d}p^\mu}{\mathrm{d}\tau} \;=\; q\,F^\mu{}_\nu\,u^\nu\ }$$
what it is not

It is not "six numbers that transform in a certain way". The transformation law is a theorem about the components in different bases, proved at the start of the next section. The object is the bilinear map. Unit 16 made this point for the inertia tensor; here, for the first time, it stops being a matter of taste, because $F_{\mu\nu}$ and $F^{\mu\nu}$ have different signs in half their entries.

28 · one field

Its six components

Fix an inertial basis. $F$ has $16$ components $F_{\mu\nu} = F(e_\mu, e_\nu)$, antisymmetry leaves six, and the six are named:

$$F_{\mu\nu} = \begin{pmatrix} 0 & -E_x/c & -E_y/c & -E_z/c\\ E_x/c & 0 & B_z & -B_y\\ E_y/c & -B_z & 0 & B_x\\ E_z/c & B_y & -B_x & 0\end{pmatrix}$$

Compactly: $F_{0i} = -E_i/c$ and $F_{ij} = \varepsilon_{ijk}B_k$, with unit 14's Levi-Civita symbol.

this is a naming, not a derivation

The assignment is fixed by demanding that $q F^\mu{}_\nu u^\nu$ reproduce $q(\vec E + \vec v\times\vec B)$ — which is Worked example 1, after the slides on raising indices. Until then, read it as six labels.

count

$\binom42 = 6$ independent entries. Three with a time index, three without. That is exactly $\vec E$ and $\vec B$, and it is why there are two fields in three dimensions and one in four.

28 · one field

Raising and lowering, and why it now matters

$\eta$ is a nondegenerate bilinear form, so $w \mapsto \eta(w,\cdot)$ is an isomorphism $V\to V^*$ (unit 16's dual space). In components that is index lowering:

$$w_\mu = \eta_{\mu\nu}w^\nu,\qquad w^\mu = \eta^{\mu\nu}w_\nu,$$

with $\eta^{\mu\nu}$ the inverse matrix, numerically $\mathrm{diag}(-1,1,1,1)$ again. For a $(0,2)$-tensor, raise one index or both:

$$F^\mu{}_\nu = \eta^{\mu\alpha}F_{\alpha\nu},\qquad F^{\mu\nu} = \eta^{\mu\alpha}\eta^{\nu\beta}F_{\alpha\beta}.$$
in Euclidean space you could be sloppy. Not here

$\eta^{00} = -1$, so raising a $0$ index flips the sign:

$$F^{0i} = +E_i/c,\qquad F_{0i} = -E_i/c,$$

while $F^{ij} = F_{ij}$. In unit 16 the metric was $\delta_{ij}$ and up and down were the same numbers; that is why the distinction could be planted quietly in unit 04 and left. It cannot be left now.

28 · one field

Which entries flip: the sign pattern of $F^{\mu\nu}$

Fμν 0 −Eₓ/c −Ey/c −Ez/c Eₓ/c 0 Bz −By Ey/c −Bz 0 Bₓ Ez/c By −Bₓ 0 0 0 1 1 2 2 3 3 Fμν 0 Eₓ/c Ey/c Ez/c −Eₓ/c 0 Bz −By −Ey/c −Bz 0 Bₓ −Ez/c By −Bₓ 0 0 0 1 1 2 2 3 3 η·η row 0 × η⁰⁰ = −1, column 0 × −1 row μ, column ν

Raising both indices multiplies row $0$ by $\eta^{00} = -1$ and column $0$ by $-1$. The $(0,0)$ entry would be flipped twice, but it is zero; so exactly the six $\vec E$ entries change sign and the $\vec B$ block does not.

In matrices, $F^{\mu\nu} = \eta^{\mu\alpha}F_{\alpha\beta}\eta^{\beta\nu}$ is $\eta\,F_{\text{low}}\,\eta$: a diagonal matrix on the left scales rows, on the right scales columns.

Raise only the first index and only row $0$ flips: $F^\mu{}_\nu = \eta F_{\text{low}}$. Index position also fixes order: $F^\mu{}_\nu \ne F_\nu{}^\mu$, they differ by a sign.

28 · one field

Worked example 1 — the Lorentz force falls out

example · unpack $q F^\mu{}_\nu u^\nu$

Ingredients. $u^\nu = \gamma(c, \vec v)$ from unit 27, and the mixed components $F^\mu{}_\nu = \eta^{\mu\alpha}F_{\alpha\nu}$: $$F^i{}_0 = F_{i0} = \frac{E_i}{c},\quad F^i{}_j = F_{ij} = \varepsilon_{ijk}B_k,\quad F^0{}_j = -F_{0j} = \frac{E_j}{c},\quad F^0{}_0 = 0 .$$

Spatial part. $qF^i{}_\nu u^\nu = q\big(F^i{}_0u^0 + F^i{}_ju^j\big) = q\big(\tfrac{E_i}{c}\,\gamma c + \varepsilon_{ijk}B_k\,\gamma v^j\big) = \gamma q\big(E_i + \varepsilon_{ijk}v^jB_k\big) = \gamma q(\vec E + \vec v\times\vec B)_i .$

And $f^i = \gamma F^i_{\text{3-force}}$, so the $\gamma$s cancel: $\ \dfrac{\mathrm{d}\vec p}{\mathrm{d}t} = q(\vec E + \vec v\times\vec B)$ — unit 23's law, recovered.

Time part. $qF^0{}_\nu u^\nu = qF^0{}_ju^j = q\tfrac{E_j}{c}\gamma v^j = \tfrac\gamma c\,q\vec E\cdot\vec v$, and $f^0 = \gamma\dot E_{\text{en}}/c$, so $\ \dot E_{\text{en}} = q\vec E\cdot\vec v$: the magnetic field does no work, because $F_{ij}$ is antisymmetric and $v^iv^j$ is not.

28 · one field

Where $F$ comes from: the four-potential

Unit 23 and unit 24 wrote $\vec B = \nabla\times\vec A$ and $\vec E = -\nabla\phi - \partial_t\vec A$. Assemble:

definition · the four-potential

$A^\mu = (\phi/c,\ \vec A)$, a vector field on Minkowski space; equivalently $A_\mu = (-\phi/c,\ \vec A)$. Then

$$F_{\mu\nu} \;=\; \partial_\mu A_\nu - \partial_\nu A_\mu ,\qquad \partial_\mu := \frac{\partial}{\partial x^\mu}.$$

Check one entry: $F_{0i} = \tfrac1c\partial_tA_i + \partial_i(\phi/c) = -E_i/c$ ✓, and $F_{ij} = \partial_iA_j - \partial_jA_i = \varepsilon_{ijk}B_k$ ✓.

gauge freedom, four-dimensionally

$A_\mu \to A_\mu + \partial_\mu\chi$ leaves $F$ unchanged, by Clairaut. Unit 23's two separate gauge transformations, $\vec A\to\vec A+\nabla\chi$ and $\phi\to\phi-\partial_t\chi$, are one.

$\partial_\mu$ carries a lower index: $\partial_\mu f$ are the components of the covector $\mathrm{d}f$, which is unit 04's point arriving with teeth.

section 2

Boosting a field

The wire, twice: magnetism in one frame, electrostatics in the other, the same force.

28 · boosting

The transformation law is a theorem

theorem · change of basis

Let $e'_\mu = e_\nu\,(\Lambda^{-1})^\nu{}_\mu$ be a second inertial basis, so that vector components obey $w'^\mu = \Lambda^\mu{}_\nu w^\nu$. Then the components of the $(0,2)$-tensor $F$ in the two bases are related by

$$F'_{\mu\nu} = (\Lambda^{-1})^\alpha{}_\mu (\Lambda^{-1})^\beta{}_\nu\,F_{\alpha\beta},\qquad\text{equivalently}\qquad F'^{\mu\nu} = \Lambda^\mu{}_\alpha\Lambda^\nu{}_\beta\,F^{\alpha\beta}.$$
proof

$F'_{\mu\nu} = F(e'_\mu, e'_\nu) = F\big(e_\alpha(\Lambda^{-1})^\alpha{}_\mu,\ e_\beta(\Lambda^{-1})^\beta{}_\nu\big)$, and bilinearity pulls both scalars out. $\square$ The raised version follows by raising with $\eta$ and using $\Lambda^\top\eta\Lambda = \eta$.

Nothing here is about electromagnetism: it is unit 16's transformation law, in four dimensions, for a tensor that happens to be antisymmetric. What is about electromagnetism is which physical quantities sit in which slots.

28 · boosting

The mixing rules

Take $\Lambda$ the boost of unit 26 with speed $v$ along $\hat x$, and multiply out. Split into components along and across the boost:

theorem · field transformation rules $$\begin{aligned} E'_\parallel &= E_\parallel, & B'_\parallel &= B_\parallel,\\ \vec E{}'_\perp &= \gamma\big(\vec E + \vec v\times\vec B\big)_\perp, & \vec B{}'_\perp &= \gamma\Big(\vec B - \tfrac{1}{c^2}\vec v\times\vec E\Big)_\perp . \end{aligned}$$

Along $\hat x$: $E'_y = \gamma(E_y - vB_z)$, $E'_z = \gamma(E_z + vB_y)$, $B'_y = \gamma(B_y + vE_z/c^2)$, $B'_z = \gamma(B_z - vE_y/c^2)$.

checks

Dimensions. $[vB] = \mathrm{m\,s^{-1}T} = \mathrm{V\,m^{-1}}$ ✓; $[vE/c^2] = \mathrm{T}$ ✓.

Limit $v\to0$. Both reduce to $\vec E{}'=\vec E$, $\vec B{}'=\vec B$ ✓.

First order in $v/c$. $\vec E{}' = \vec E + \vec v\times\vec B$, $\vec B{}' = \vec B$ — exactly unit 25's Galilean field transformation, the rule its magnetic limit is built on, now seen as a truncation rather than a theory.

28 · boosting

The mixing rules, plotted: a pure $\vec B$ seen on the move

B′z / B = γ −E′y / cB = γβ √𝓘₁ / B = 1, every β the wire's charge: β = 0.0100 0 1 2 3 0.25 0.5 0.75 1 β = v/c of the observer

A field that is purely magnetic in the lab ($\vec E = 0$, $\vec B = B\hat z$), seen by an observer moving at $\beta\hat x$. An electric field appears and both grow without bound, but the difference of their squares never moves.

Put $\vec E = 0$ into the rules of the previous slide:

$$B'_z = \gamma B,\qquad E'_y = -\gamma vB .$$

So $B'^2 - E'^2/c^2 = \gamma^2B^2(1 - \beta^2) = B^2$ at every speed: the flat dashed line.

the wire's charge

$\beta = 0.0100$ gives $E'_y = -\gamma vB = -30.0015\ \mathrm{V\,m^{-1}}$ — the dot at the far left, where both curves have barely moved. Worked example 3 gets the same number from charge densities.

As $\beta\to1$, $|E'|/cB' = \beta\to1$: a fast observer sees $\vec E\perp\vec B$ with $E\approx cB$, almost a light wave.

28 · boosting

Worked example 2 — the wire in the lab

example · the magnetic story

Setup. Wire along $\hat x$, $I = 1.00$ A in $+\hat x$; charge $q = 1.00$ nC at $(0, r, 0)$, $r = 2.00$ cm, velocity $v\hat x$ with $v = 3.00\times10^{6}\ \mathrm{m\,s^{-1}}$.

The field. The wire is neutral: the lattice's positive line density and the conduction electrons' negative one cancel exactly, so $\vec E = 0$. Ampère (unit 23) gives

$$B_z = \frac{\mu_0 I}{2\pi r} = \frac{(4\pi\times10^{-7})(1.00)}{2\pi(0.0200)} = 10.0\ \mu\mathrm T .$$

The force. $\vec F = q\vec v\times\vec B = qvB_z\,(\hat x\times\hat z) = -qvB_z\,\hat y$, so

$$\begin{aligned}F_y &= -(1.00\times10^{-9})(3.00\times10^{6})\\ &\qquad\times(1.00\times10^{-5})\\ &= -3.000\times10^{-8}\ \mathrm N,\end{aligned}$$

towards the wire. A positive charge moving with the current is attracted — parallel currents attract.

+ − + − + − + − + − + − + − + − + electrons drift at u I v F = qvB, towards the wire q r B, out of the page B at q: 10.0 μT x y z

The lab. Ions and electrons equally spaced, so no $\vec E$. Above the wire $\vec B$ points out of the page; $\hat x\times\hat z = -\hat y$ turns $q\vec v\times\vec B$ towards the wire.

28 · boosting

Worked example 3 — the same wire, from the charge

example · Purcell's argument, in full

Step 1 — proper densities. The lattice is at rest in the lab with density $+\lambda$, so its proper line density is $\lambda$. The electrons move at $-u\hat x$ with lab density $-\lambda$, so their proper density is $-\lambda/\gamma_u$ (their lab density is already contracted).

Step 2 — boost to the charge. In the charge's frame the lattice moves at $-v$, so $\lambda'_+ = \gamma_v\lambda$. The electrons' speed there follows from unit 26's velocity addition, $\gamma_{u'} = \gamma_u\gamma_v(1 + uv/c^2)$, so $\lambda'_- = -\gamma_v\lambda\,(1 + uv/c^2)$.

lab: the wire is neutral + + + + + + + + − − − − − − − at rest drift u charge's frame (exaggerated) + + + + + + + + + − − − − − − − − − − − move at v faster 6 + and 6 − : net 0 8 + and 9 − : net negative

The same stretch of wire in both frames, exaggerated ($\gamma_v = 1.25$, $1 + uv/c^2 = 1.2$; really $1 + 5\times10^{-5}$ and $1 + 2.5\times10^{-15}$). In the lab the window holds as many electrons as ions. Seen from the charge both rows bunch up, the faster electrons more: the wire is negative.

28 · boosting

Worked example 3, continued — the net charge and its field

example · Purcell's argument, concluded

Step 3 — the net. $\ \lambda' = \lambda'_+ + \lambda'_- = -\gamma_v\lambda\,\dfrac{uv}{c^2} = -\gamma_v\dfrac{Iv}{c^2} = -3.3381\times10^{-11}\ \mathrm{C\,m^{-1}} .$

Step 4 — the force. Gauss (unit 05) on a cylinder, with $r' = r$ because transverse lengths do not contract:

$$E'_y = \frac{\lambda'}{2\pi\varepsilon_0 r} = -30.0015\ \mathrm{V\,m^{-1}},$$ $$F'_y = qE'_y = -3.00015\times10^{-8}\ \mathrm N .$$

The wire is charged, the charge sits still, and the force is pure electrostatics.

− the wire, end on: λ′ < 0 F′ = qE′ q, at rest r′ = r Gauss cylinder E′

The charge's frame, end on. The wire is negative, the charge is at rest, and the only force available is electric — pointing at the wire, as in the lab.

28 · boosting

The two answers, to the last $\gamma$

Lab: $F_y = -3.000\times10^{-8}$ N. Charge's frame: $F'_y = -3.00015\times10^{-8}$ N. They differ by $\gamma_v = 1.0000500730$. That is not a discrepancy — it is the law.

theorem · transverse force

If a particle is instantaneously at rest in $S'$ and moves at $v\hat x$ in $S$, then

$$F_\perp = \frac{F'_\perp}{\gamma}.$$
proof

$p^y$ is unchanged by an $x$-boost, so $\mathrm{d}p_y = \mathrm{d}p'_y$; and $\mathrm{d}t = \gamma\,\mathrm{d}\tau = \gamma\,\mathrm{d}t'$. Divide. $\square$

the loop closes

$\dfrac{F'_y}{\gamma_v} = \dfrac{-3.00015\times10^{-8}}{1.0000500730} = -3.000\times10^{-8}\ \mathrm N$ ✓

And the same answer comes out of the mixing rules with no charge densities at all: with $\vec E = 0$ in the lab, $E'_y = \gamma(E_y - vB_z) = -\gamma vB_z$, which is $-30.0015\ \mathrm{V\,m^{-1}}$ ✓. Three routes, one number.

28 · boosting

Purcell's moral: magnetism is a $10^{-13}$ effect

The relativistic correction to the wire's charge balance is a fraction

$$\frac{uv}{c^2} = \frac{(7.352\times10^{-5})(3.00\times10^{6})}{8.98755\times10^{16}} = 2.454\times10^{-15},$$

with $u/c = 2.452\times10^{-13}$ carrying most of the smallness. But it multiplies $\lambda = 1.3602\times10^{4}\ \mathrm{C\,m^{-1}}$, and $10^{-15}\times10^{4}$ is $10^{-11}$ C per metre — enough to pull on a nanocoulomb with $3\times10^{-8}$ N.

Magnetism is what is left of Coulomb's law after a cancellation of fifteen figures fails to be exact.

10⁻¹² 10⁻⁹ 10⁻⁶ 10⁻³ 10⁰ 10³ line charge density (C m⁻¹), log scale λ = 1.36×10⁴ each sign |λ′| = 3.3×10⁻¹¹ the net × uv/c² = 2.45×10⁻¹⁵

One factor of $uv/c^2$ takes the charge per metre down almost fifteen decades.

do not over-claim

This argument explains the field of a steady current in a neutral conductor seen from a boosted frame. It does not derive magnetism from electrostatics in general: a permanent magnet's field comes from electron spin, which is quantum, and no boost turns an intrinsic magnetic moment into a charge density.

What is true in general is the tensor statement: $\vec E$ and $\vec B$ are blocks of one object, so no frame-independent line separates them.

section 3

Maxwell, in two lines

Four vector equations, eight scalar ones, and they are two tensor equations.

28 · maxwell

The four-current

definition · the four-current

$J^\mu = (c\rho,\ \vec J)$, a vector field on Minkowski space. For a single species of charge with proper density $\rho_0$ moving with four-velocity $u$: $J^\mu = \rho_0 u^\mu$.

The second form is the honest one: it manifestly builds a vector, and $\rho = \gamma\rho_0$, $\vec J = \rho\vec v$ drop out of it. Charge per unit volume is frame-dependent for the same reason charge per unit length was.

theorem · covariant continuity $$\partial_\mu J^\mu = 0 \iff \partial_t\rho + \nabla\cdot\vec J = 0 .$$
proof

$\partial_\mu J^\mu = \tfrac1c\partial_t(c\rho) + \partial_iJ^i$. $\square$

Unit 23's continuity equation, unit 22's mass version, and this are one statement: the divergence of a flux four-vector vanishes.

28 · maxwell

The wire's four-current is spacelike

ct x light ct′ x′ J J′⁰ < 0, so ρ′ < 0 lab: J⁰ = cρ = 0

In the lab the wire's $J$ has no time component. Resolved along a moving frame's axes ($\beta = 0.5$ here, for visibility) it acquires one, and it is negative: a charged wire.

In the lab, $\rho = 0$ and $\vec J = (I/A)\hat x = 1.00\times10^{6}\ \mathrm{A\,m^{-2}}\,\hat x$, so

$$J^\mu = (0,\ J_x,\ 0,\ 0),\qquad \eta(J,J) = J_x^2 > 0 .$$

Boost to the charge: $J'^0 = \gamma(J^0 - \beta J^1) = -\gamma\beta J_x$, so

$$\rho' = -\frac{\gamma vJ_x}{c^2} = -3.3381\times10^{-5}\ \mathrm{C\,m^{-3}} .$$
the wire again

Times the cross-section $A = 1.00\ \mathrm{mm^2}$: $\rho'A = -\gamma vI/c^2 = \lambda'$ ✓ — Worked example 3's net charge, with no counting of ions and electrons at all.

28 · maxwell

The sourced pair, in one equation

theorem · the inhomogeneous Maxwell equations $$\boxed{\ \partial_\mu F^{\nu\mu} \;=\; \mu_0 J^\nu\ }$$

is, component by component, Gauss's law ($\nu = 0$) and the Ampère–Maxwell law ($\nu = i$).

$\nu = 0$: $\ \partial_iF^{0i} = \partial_i(E_i/c) = \nabla\cdot\vec E/c$, and $\mu_0J^0 = \mu_0c\rho$. So $\nabla\cdot\vec E = \mu_0c^2\rho = \rho/\varepsilon_0$ ✓

$\nu = i$: $\ \partial_0F^{i0} + \partial_jF^{ij} = -\tfrac1{c^2}\partial_tE_i + (\nabla\times\vec B)_i = \mu_0J_i$ ✓

bonus: continuity, free

$\partial_\nu\partial_\mu F^{\nu\mu} = 0$, because $\partial_\nu\partial_\mu$ is symmetric (Clairaut) and $F^{\nu\mu}$ antisymmetric. Hence $\partial_\nu J^\nu = 0$ automatically: charge conservation is a corollary of Maxwell, not an extra law. Unit 24 found the displacement current by insisting on this; here it is one line.

28 · maxwell

The symbol, and the tensor

definition · the Levi-Civita symbol

$[\mu\nu\rho\sigma]$ is $+1$ for an even permutation of $(0,1,2,3)$, $-1$ for an odd one, $0$ otherwise. It is an array of numbers, declared to be the same in every basis — not a tensor.

definition · the Levi-Civita tensor

$\epsilon_{\mu\nu\rho\sigma} := \sqrt{|\det\eta|}\,[\mu\nu\rho\sigma] = [\mu\nu\rho\sigma]$ here, a $(0,4)$-tensor: the unique totally antisymmetric one with $\epsilon_{0123} = 1$.

theorem · when they coincide

Under a change of basis by $\Lambda$, the components of the tensor pick up $\det\Lambda$. For $\Lambda\in SO(1,3)$, $\det\Lambda = +1$, so the components are unchanged and the tensor's components equal the symbol in every proper Lorentz frame.

Under a reflection they differ by a sign: $\epsilon$ is a pseudotensor with respect to the full Lorentz group. Raised: $\epsilon^{0123} = \eta^{00}\eta^{11}\eta^{22}\eta^{33}\epsilon_{0123} = -1$.

28 · maxwell

The dual, and the other pair

definition · the dual field tensor $$\tilde F^{\mu\nu} := \tfrac12\,\epsilon^{\mu\nu\rho\sigma}F_{\rho\sigma}.$$

Computing the components: $\tilde F^{0i} = -B_i$ and $\tilde F^{ij} = \varepsilon_{ijk}E_k/c$. So dualising is the substitution

$$\vec E/c \longmapsto -\vec B,\qquad \vec B\longmapsto \vec E/c,$$

a duality rotation by a quarter turn; $\tilde{\tilde F} = -F$.

theorem · the source-free pair $$\partial_\mu\tilde F^{\nu\mu} = 0 \iff \nabla\cdot\vec B = 0\ \text{ and }\ \partial_t\vec B + \nabla\times\vec E = 0 .$$

Equivalently, without the dual,

$$\partial_\lambda F_{\mu\nu} + \partial_\mu F_{\nu\lambda} + \partial_\nu F_{\lambda\mu} = 0,$$

the Bianchi identity. It is automatic once $F = \partial A - \partial A$: substitute and the six terms cancel in pairs by Clairaut.

count

Two tensor equations, eight scalar equations, exactly Maxwell's four vector laws. And half of them say only "$F$ comes from a potential".

28 · maxwell

The two invariants

theorem · every frame agrees on exactly two numbers $$\tfrac12F_{\mu\nu}F^{\mu\nu} = B^2 - \frac{E^2}{c^2} \;=:\;\mathcal I_1,\qquad \tfrac c4 F_{\mu\nu}\tilde F^{\mu\nu} = \vec E\cdot\vec B \;=:\;\mathcal I_2 .$$
proof of the first

$F_{\mu\nu}F^{\mu\nu} = 2F_{0i}F^{0i} + F_{ij}F^{ij} = 2\big(-\tfrac{E_i}{c}\big)\big(\tfrac{E_i}{c}\big) + \varepsilon_{ijk}\varepsilon_{ijl}B_kB_l = -\tfrac{2E^2}{c^2} + 2B^2 .$ $\square$

Both are scalars because every index is contracted; that is the whole argument, and it is unit 16's contraction lemma.

on the wire

Lab: $\mathcal I_1 = (10.0\,\mu\mathrm T)^2 = 1.0000\times10^{-10}\ \mathrm{T^2}$, $\mathcal I_2 = 0$.

Charge's frame: $B'^2 - E'^2/c^2 = \gamma^2B^2 - \gamma^2v^2B^2/c^2 = B^2$ — the $\gamma^2$ cancels against $1-v^2/c^2$ exactly, giving $1.0000\times10^{-10}\ \mathrm{T^2}$ ✓, and $\vec E{}'\perp\vec B{}'$ so $\mathcal I_2 = 0$ ✓.

28 · maxwell

Worked example 4 — which field can you transform away?

example · reading the invariants

The rule. If $\mathcal I_2 = \vec E\cdot\vec B = 0$ and $\mathcal I_1 > 0$, a frame exists where the field is purely magnetic; if $\mathcal I_2 = 0$ and $\mathcal I_1 \lt 0$, purely electric; if $\mathcal I_1 = \mathcal I_2 = 0$ with $F\ne0$, neither, ever. If $\mathcal I_2\ne0$, both fields are nonzero in every frame.

Case A. $\vec E = 6.00\times10^{5}\,\hat y\ \mathrm{V\,m^{-1}}$, $\vec B = 1.00\times10^{-3}\,\hat z$ T. Then $\mathcal I_2 = 0$ and $\mathcal I_1 = 1.00\times10^{-6} - 4.0055\times10^{-6} = -3.0055\times10^{-6}\ \mathrm{T^2} \lt 0$: purely electric somewhere.

The boost. Kill $B'_z = \gamma(B_z - vE_y/c^2)$: take $v = c^2B_z/E_y = 1.4979\times10^{8}\ \mathrm{m\,s^{-1}}$, i.e. $\beta = cB/E = 0.499654$, $\gamma = 1.15443$. Then $E'_y = \gamma(E_y - vB_z) = \gamma E_y(1-\beta^2) = E_y/\gamma = 5.1974\times10^{5}\ \mathrm{V\,m^{-1}}$.

Check. $-E'^2/c^2 = -3.0055\times10^{-6}\ \mathrm{T^2}$ ✓ — the invariant is unchanged to five figures.

28 · maxwell

The invariants, drawn: boosts slide along hyperbolae

E/c (mT) B (mT) 1 1 2 2 E = cB: null A A′: B′ = 0 𝓘₁ < 0 W 𝓘₁ > 0

$\vec E = E\hat y$, $\vec B = B\hat z$, boosts along $\hat x$. A boost moves the point $(E/c, B)$ along its hyperbola $B^2 - E^2/c^2 = \mathcal I_1$, never off it. Case A rides its branch down to the axis. A point on a dashed null line stays on it.

For $\vec E = E\hat y$, $\vec B = B\hat z$ and a boost along $\hat x$, the mixing rules read

$$\tfrac{E'}{c} = \gamma\big(\tfrac Ec - \beta B\big),$$ $$B' = \gamma\big(B - \beta\tfrac Ec\big):$$

a Lorentz boost of the pair itself. Its orbits are the hyperbolae of constant $\mathcal I_1$.

example · the rule, read off the picture

Case B — the wire. $\mathcal I_1 = +1.00\times10^{-10}\ \mathrm{T^2} \gt 0$, $\mathcal I_2 = 0$: purely magnetic somewhere, and the lab is that frame. No boost removes the magnetic field, which is why the charge's frame has both.

A branch that crosses an axis has a frame with one field zero there. The null lines cross neither axis away from the origin, so a light wave keeps both fields in every frame.

section 4

Where the energy is

One symmetric tensor, one vanishing divergence, and unit 24's two theorems fall out together.

28 · energy

The stress-energy tensor of the field

definition · the electromagnetic stress-energy tensor $$T^{\mu\nu} \;=\; \frac{1}{\mu_0}\Big(F^{\mu\alpha}F^{\nu}{}_{\alpha} \;-\; \tfrac14\,\eta^{\mu\nu}F_{\alpha\beta}F^{\alpha\beta}\Big).$$

Mathematically: up to scale, the only symmetric $(2,0)$-tensor quadratic in $F$, built with $\eta$ alone, that is traceless — proof in the notes. The first term is the obvious quadratic contraction; the second subtracts its trace.

Physically, the components are unit 24's:

$$T^{00} = u,\qquad T^{0i} = \frac{S_i}{c},\qquad T^{ij} = -\sigma_{ij},$$

with $u = \tfrac{\varepsilon_0}2E^2 + \tfrac1{2\mu_0}B^2$, $\vec S = \vec E\times\vec B/\mu_0$, and $\sigma$ the Maxwell stress tensor.

two properties, immediately

Symmetric: $F^{\mu\alpha}F^\nu{}_\alpha = \eta_{\alpha\beta}F^{\mu\alpha}F^{\nu\beta}$ is visibly symmetric in $\mu\nu$.

Traceless: $T^\mu{}_\mu = \frac1{\mu_0}(F^{\mu\alpha}F_{\mu\alpha} - \frac44F_{\alpha\beta}F^{\alpha\beta}) = 0$, because $\eta^\mu{}_\mu = 4$.

a sign to keep straight

$T^{ij} = -\sigma_{ij}$: unit 24's $\sigma$ is the force per area transmitted across a surface, while $T^{ij}$ is the flux of $i$-momentum in direction $j$. Momentum flowing out is momentum lost.

28 · energy

One divergence, two conservation laws

theorem · the divergence identity $$\boxed{\ \partial_\nu T^{\mu\nu} \;=\; -\,F^{\mu}{}_{\nu}J^{\nu}\ }$$

The right-hand side is minus the Lorentz force density: $-F^\mu{}_\nu J^\nu$ has components $-(\vec J\cdot\vec E/c,\ \rho\vec E + \vec J\times\vec B)$.

Proof, in three moves. Expand the derivative; use $\partial_\nu F^{\nu\alpha} = -\mu_0J^\alpha$ on the first piece; and show the remaining two pieces cancel by the Bianchi identity. The full working is in the notes.

In vacuum, $J = 0$ and $\partial_\nu T^{\mu\nu} = 0$: energy and momentum are locally conserved, in exactly unit 22's sense — there a flux tensor for mass and momentum; here one with a row and a column more, and the extra row is energy.

u S₁/c S₂/c S₃/c S₁/c −σ₁₁ −σ₁₂ −σ₁₃ S₂/c −σ₂₁ −σ₂₂ −σ₂₃ S₃/c −σ₃₁ −σ₃₂ −σ₃₃ μ = 0 μ = i ν = 0 ν = j ∂ν runs along each row energy: ∂ₜu + ∇·S = −J·E momentum, 3 rows: ∂ₜg − div σ = −(ρE + J×B) symmetric: column 0 = row 0, so g = S/c²

$\partial_\nu$ contracts the column index, so each row of $T$ is one conservation law: row $0$ energy, rows $1$–$3$ the three components of momentum. Four laws, one equation; Worked example 5 reads each off.

28 · energy

Worked example 5 — reading off Poynting and the stress balance

example · the four components of one identity

$\mu = 0$. Left: $\partial_\nu T^{0\nu} = \partial_0T^{00} + \partial_iT^{0i} = \tfrac1c\big(\partial_tu + \nabla\cdot\vec S\big)$. Right: $-F^0{}_\nu J^\nu = -F^0{}_jJ^j = -\tfrac{E_j}{c}J_j$. Multiply by $c$:

$$\partial_tu + \nabla\cdot\vec S = -\vec J\cdot\vec E ,$$

which is Poynting's theorem (unit 24), letter for letter.

$\mu = i$. Left: $\partial_0T^{i0} + \partial_jT^{ij} = \partial_t\big(S_i/c^2\big) - \partial_j\sigma_{ij}$. Right: $-\big(F^i{}_0J^0 + F^i{}_jJ^j\big) = -\big(\rho E_i + (\vec J\times\vec B)_i\big)$. So

$$\partial_t\vec g - \operatorname{div}\sigma = -\big(\rho\vec E + \vec J\times\vec B\big),\qquad \vec g = \vec S/c^2,$$

which is unit 24's momentum balance, letter for letter.

What was gained. Unit 24 proved these separately, each by a page of vector identities. Here they are the four components of one tensor equation, and the symmetry $T^{0i} = T^{i0}$ — which unit 24 could only check — is why $\vec g = \vec S/c^2$.

section 5

Radiation, honestly

One invariant gives the radiated power. The recoil from it breaks the theory.

28 · radiation

Larmor, made covariant

theorem · the Liénard formula $$P = \frac{\mu_0q^2}{6\pi c}\,a^\mu a_\mu = \frac{\mu_0q^2}{6\pi c}\,\gamma^6\Big(|\vec a|^2 - \frac{|\vec v\times\vec a|^2}{c^2}\Big).$$

Why. (i) $P$ is a Lorentz scalar: in the instantaneous rest frame the dipole pattern is $\sin^2\theta$ (unit 24), so the radiated four-momentum has no spatial part there, and $\mathrm{d}E = \gamma\,\mathrm{d}E_0$, $\mathrm{d}t = \gamma\,\mathrm{d}\tau$ divide out. (ii) Assuming $P$ depends only on $u$ and $a$ and is quadratic in $a$, the only available scalar is $a^\mu a_\mu$. (iii) The constant is fixed by the rest frame, where Larmor gives $\mu_0q^2|\vec a|^2/6\pi c$.

check

Limit. $v\to0$: $\gamma\to1$, $\vec v\times\vec a\to0$, and $P\to\mu_0q^2a^2/6\pi c$, Larmor ✓ (unit 24's form with $1/\varepsilon_0c^3 = \mu_0/c$). Dimensions in the notes.

a n −n θ = 0 ∝ sin²θ: equal and opposite in n and −n

Step (i), drawn. In the instantaneous rest frame the radiation goes out as $\sin^2\theta$ about $\vec a$: as much along $-\hat n$ as along $\hat n$, so the radiated momentum sums to zero and only energy leaves.

28 · radiation

Synchrotron loss: the $\gamma^4$ that ended LEP

1 meV 1 eV 1 keV 1 MeV 1 GeV 1 TeV 10 GeV 100 GeV 1 TeV 10 TeV beam energy, log scale energy lost per turn ΔE = E LEP: 3.41 GeV LHC: 5.93 keV electrons, R = 3096 m protons, R = 2804 m

Energy lost per turn, $q^2\gamma^4/3\varepsilon_0R$, in LEP's ring for electrons and the LHC's for protons. Both lines have slope 4; at equal energy they sit $(m_p/m_e)^4 \approx 10^{13}$ apart. Above about 330 GeV an electron in LEP's tunnel would radiate more than its whole energy each turn.

circular motion

Circular motion, $\vec v\perp\vec a$: $a\cdot a = \gamma^4a^2$, so $P\propto\gamma^4$. Energy lost per turn is $\Delta E = q^2\gamma^4/3\varepsilon_0R$, with $R$ the ring's bending radius (not $\rho$, which in this unit is charge density).

Numbers. LEP at 104.5 GeV, $R = 3096$ m: $\gamma = 2.045\times10^{5}$, $\Delta E = 3.41$ GeV per turn. LHC protons at 6.8 TeV, $R = 2804$ m: $\gamma = 7247$, $\Delta E = 5.93$ keV. A factor $5.7\times10^{5}$, and the reason LEP's tunnel now holds the LHC.

28 · radiation

The recoil, and where classical theory stops

A radiating charge loses energy, so something must push back. Matching the work done over a period to the radiated energy gives the Abraham–Lorentz force

$$\vec F_{\text{rad}} = \frac{\mu_0q^2}{6\pi c}\,\dot{\vec a} = m\tau_0\,\dot{\vec a},\qquad \tau_0 = \frac{\mu_0q^2}{6\pi mc},$$

with $\tau_0 = 6.266\times10^{-24}$ s for an electron — the light-crossing time of $\tfrac23$ of the classical electron radius $r_e = 2.818\times10^{-15}$ m.

and now the trouble

$m\dot{\vec v} = m\tau_0\ddot{\vec v} + \vec F_{\text{ext}}$ is third order. With $\vec F_{\text{ext}} = 0$ it admits $\vec a(t) = \vec a_0e^{t/\tau_0}$: a free electron that accelerates itself forever — a runaway solution.

Discarding runaways by a boundary condition at $t=+\infty$ buys pre-acceleration: the charge starts moving a time $\sim\tau_0$ before the force arrives.

Neither is acceptable, and no fully satisfactory classical repair exists. This is stated, not solved.

28 · radiation

Runaway and pre-acceleration, plotted

force switched on pre-acceleration a = F₀/m runaway, no force 0 1 −4 −3 −2 −1 0 1 2 3 t / τ₀ a / (F₀/m)

A force $F_0$ switched on at $t = 0$. Without radiation reaction the acceleration would jump straight from $0$ to $F_0/m$ (dotted). With it, either the charge runs away — shown with no force at all — or, if runaways are forbidden, it starts accelerating before the force arrives.

Write the equation as $\ \vec a - \tau_0\dot{\vec a} = \vec F_{\text{ext}}/m$. Its general solution is any particular one plus $\vec a_0e^{t/\tau_0}$, the runaway.

The only solution that stays bounded as $t\to+\infty$ is

$$\vec a(t) = \frac1{\tau_0}\int_t^\infty e^{(t-s)/\tau_0}\,\frac{\vec F_{\text{ext}}(s)}{m}\,\mathrm{d}s ,$$

an average of the force over the future, weighted over a time $\tau_0$.

for the step

$t > 0$: $a = F_0/m$. $\ t \lt 0$: $a = (F_0/m)\,e^{t/\tau_0}$ — nonzero before the force exists. For an electron the lead time is $\sim 6\times10^{-24}$ s.

28 · closing

What this bought

the wire, closed

Lab: $3.000\times10^{-8}$ N, magnetic.
Charge's frame: $3.00015\times10^{-8}$ N, electrostatic.
Ratio $\gamma_v$, exactly.
$\mathcal I_1 = 1.0000\times10^{-10}\ \mathrm{T^2}$ in both.

the objects

$F_{\mu\nu}$ antisymmetric, six components.
$J^\mu$, with continuity as a corollary.
$\tilde F$, $\mathcal I_1$, $\mathcal I_2$.
$T^{\mu\nu}$: symmetric, traceless, with $\partial_\nu T^{\mu\nu} = -F^\mu{}_\nu J^\nu$.

what uses it

29: $T^{\mu\nu}$ from Noether, honestly.
30: the equivalence principle.
32–33: the same index calculus with $\eta\to g$ and $\partial\to\nabla$.
38: a wave equation for a tensor, sourced by $T$.

The one habit to carry forward: write the tensor equation first, then choose a frame. Every calculation in this unit that was hard in three-vector notation — Poynting's theorem, the momentum balance, the field transformations — became a line of index bookkeeping, and every one that was easy stayed easy.

28 · checkpoint

Checkpoint

you can now

Given $F^{\mu\nu}$ and a boost, derive the $\vec E$ and $\vec B$ transformation rules and verify both invariants numerically; and show by explicit computation that $\partial_\nu T^{\mu\nu} = -F^\mu{}_\nu J^\nu$, reading Poynting's theorem off the time component and the momentum balance off the spatial ones.

it is false if

you cannot say which index of $F$ the divergence is taken in and why the sign depends on it; or you compute $\mathcal I_1$ in two frames and get two numbers; or the proof of the divergence identity stops at "the other terms cancel".

to check it

Close the deck. On paper: the six mixing rules from $F'^{\mu\nu} = \Lambda^\mu{}_\alpha\Lambda^\nu{}_\beta F^{\alpha\beta}$; then $\mathcal I_1$ for the wire in both frames, to five figures; then $\partial_\nu T^{\mu\nu}$ in full, Bianchi step included. Then ./mr problems 28.