Part D · Minkowski · spine

30

The equivalence principle, and why flat spacetime cannot hold gravity

One experimental coincidence — inertial mass equals gravitational mass — predicts falling light and slow clocks before any geometry exists, and then proves that no field on Minkowski space can be gravity.

needs 27, 05, 16~2½ h slides + 5 h problemsproblems: ./mr problems 30

30 · overview

One photon, five sections

the question

A photon climbs a 22.5 m tower. Does its frequency change, and by how much?

Nothing in units 26–29 answers this: on Minkowski space a photon's frequency is constant along its worldline between inertial observers at rest relative to one another. The answer comes from one experimental fact about falling bodies — all of them fall alike — and it is $\Delta\nu/\nu = -2.455\times10^{-15}$, measured in 1960 to ten per cent.

the route, in four steps

1. Swap the tower, standing in the Earth's field $g$, for a rocket of the same height $h$ accelerating at $g$ in empty space. The equivalence principle says no experiment inside can tell them apart.

2. Light from the floor needs $h/c$ to reach the ceiling; by then the ceiling has gained speed $gh/c$, away from the source.

3. A receiver receding at $v$ sees the frequency lowered by $v/c$ (unit 26's Doppler shift, to first order), so $\Delta\nu/\nu = -gh/c^2$.

4. $h = 22.5$ m: $-2.455\times10^{-15}$. Pound and Rebka measured $(2.57\pm0.26)\times10^{-15}$.

The plan. 1 $m_{\mathrm i} = m_{\mathrm g}$, how well it is known, three statements of it · 2 redshift, clock rates, bending, with no geometry · 3 Rindler: the same redshift exactly, on flat spacetime · 4 the rotating disc, whose space is not Euclidean · 5 tides: what no coordinate change removes.

section 1

Two masses, and three principles

A coincidence measured to one part in $10^{15}$, and the three different things it is taken to mean.

30 · masses

Two masses Newton did not have to make equal

In Newton's theory two constants attach to a body, and they appear in different laws.

the two masses

Inertial mass $m_{\mathrm i}$ is the constant in $\vec F = m_{\mathrm i}\ddot{\vec x}$: the resistance to being accelerated by any force.

Gravitational mass $m_{\mathrm g}$ is the charge in $\vec F = -m_{\mathrm g}\nabla\Phi$: the coupling to the gravitational field, exactly as $q$ couples to $\vec E$.

Nothing in the axioms relates them. If they differ, free fall reads $$\ddot{\vec x} = -\frac{m_{\mathrm g}}{m_{\mathrm i}}\,\nabla\Phi ,$$ and the trajectory depends on the body.

the Eötvös parameter

For two bodies $A$, $B$ in the same field, with free-fall accelerations $a_A$, $a_B$, the dimensionless $$\eta_{AB} := 2\,\frac{a_A - a_B}{a_A + a_B} = \frac{(m_{\mathrm g}/m_{\mathrm i})_A - (m_{\mathrm g}/m_{\mathrm i})_B}{\text{mean}} .$$ $\eta = 0$ for every pair is the claim under test.

The letter is the literature's. This $\eta$ is a number and has nothing to do with the Minkowski form $\eta_{\mu\nu}$, which returns in section 3.

what would falsify it

Any composition dependence. Bodies differ in nuclear binding energy per nucleon, in neutron-to-proton ratio, in electrostatic energy: if any of these carried its own gravitational charge at a different rate, $\eta\ne0$ for a beryllium–titanium pair even though both fall at $9.8\ \mathrm{m\,s^{-2}}$ to a part in $10^{4}$.

30 · masses

How well it is known

experimentdatemethod$|\eta|$ below
Newton, Principia III.61687paired pendulums$10^{-3}$
Bessel1832paired pendulums$2\times10^{-5}$
Eötvös, Pekár, Fekete1922torsion balance, Earth$5\times10^{-9}$
Roll, Krotkov, Dicke1964torsion balance, Sun$10^{-11}$
Braginsky, Panov1972torsion balance, Sun$10^{-12}$
Eöt-Wash (Adelberger)2008rotating torsion balance$2\times10^{-13}$
MICROSCOPE2022drag-free satellite$1.5\times10^{-15}$

Twelve orders of magnitude in three centuries, and the answer has never moved off zero.

10⁻³ 10⁻⁶ 10⁻⁹ 10⁻¹² 10⁻¹⁵ 1700 1800 1900 2000 Newton Bessel Eötvös Roll–Krotkov–Dicke Braginsky–Panov Eöt-Wash MICROSCOPE excluded still allowed, η = 0 among it pendulums torsion balances satellite |η| bound

Each point is a bound: $|\eta|$ above it is ruled out. The shaded region is everything excluded by the best result to date — it has only ever grown downward, and $\eta = 0$ has stayed inside what is left.

30 · masses

Why a torsion balance works

why a torsion balance

Hang two different materials on a horizontal beam. A difference $\eta$ in $m_{\mathrm g}/m_{\mathrm i}$ gives a differential acceleration $\eta a_\perp$ along the horizontal component of the source's field — the centrifugal residue of the Earth's rotation, $a_\perp\approx1.69\ \mathrm{cm\,s^{-2}}$ at mid-latitude, or the Sun's field swinging through $360^\circ$ each day.

Each mass is pushed $\tfrac12\eta a_\perp$ off the mean, in opposite senses, so the torque is $\tau = 2\cdot m\,\tfrac12\eta a_\perp\,d = m\,\eta a_\perp\,d$, and it twists a fibre of stiffness $\kappa$ through $\theta = \tau/\kappa$. The signal is periodic at a known frequency, which is what buys the extra orders of magnitude.

P12 designs one: for $\eta = 10^{-13}$, two 10 g masses 2 cm from the axis on a fibre with an 800 s period twist by $0.69$ nrad.

fibre Be Ti d m a⊥ m a⊥ +½ mηa⊥ −½ mηa⊥ twist θ a⊥ horizontal part of the field

Seen from above. The shared part of the pull, $m a_\perp$ on each end, has no torque about the fibre; only the $\pm\tfrac12 m\eta a_\perp$ differences turn the beam. The vertical part of the field is taken up by the fibre.

30 · masses

Einstein's elevator, and what it actually claims

Einstein, 1907, on the patent-office argument he later called "the happiest thought of my life": a man falling freely from a roof does not feel his own weight.

the thought experiment

A windowless box. Inside, release two balls of different composition.

  • Box at rest on the Earth: both fall at $g$.
  • Box in deep space with proper acceleration $g$: both appear to fall at $g$ — they are inertial and the floor rises.

Because $\eta = 0$, no mechanical experiment inside distinguishes the two. Einstein's step was to strike the word "mechanical".

the Earth both fall at g at rest on the Earth appear to fall at g accelerating in empty space a = g

Two balls of different composition in each box. On the left they fall at $g$; on the right they float, inertial, and the floor comes up to meet them at $g$. Seen from inside, the two pictures are the same.

30 · masses

Three principles, three different claims

WEP

Weak. The worldline of a freely falling test body, given its initial position and velocity, is independent of its mass and composition.

"Test body": small enough to ignore its own field, structureless, uncharged.

EEP

Einstein. WEP, plus: in any local freely falling frame the outcome of any non-gravitational experiment is independent of the frame's velocity (local Lorentz invariance) and of where and when it is performed (local position invariance).

SEP

Strong. EEP with "non-gravitational" deleted, and "test body" weakened to include bodies with appreciable gravitational self-energy — stars, planets, the Earth.

30 · masses

Nested, and strictly

WEP holds tested by Eöt-Wash, MICROSCOPE EEP holds tested by clock comparisons SEP holds tested by lunar laser ranging a scalar field coupled to light only Brans–Dicke general relativity a composition-dependent fifth force: none found

Each ring holds the theories that satisfy a principle; each named theory sits where it is known to belong. The experiment written on a boundary is the one that tests whether nature is inside it.

these are not rephrasings of one another

WEP $\Leftarrow$ EEP $\Leftarrow$ SEP, and both arrows are strict: theories are known that satisfy WEP and violate EEP (add a scalar field coupling to electromagnetism), and theories that satisfy EEP and violate SEP — every metric theory with an extra field does, including Brans–Dicke. General relativity is the standard example of a theory satisfying all three.

30 · masses

An experiment for each

WEP · Eöt-Wash, MICROSCOPE

Do two compositions fall alike? $|\eta| \lt 1.5\times10^{-15}$.

Falsified by any composition-dependent differential acceleration.

EEP · clock comparison

Does a clock's rate depend only on its potential, not on what it is made of or when it is read? Gravity Probe A (1976) flew a hydrogen maser to 10 000 km: prediction confirmed to $7\times10^{-5}$.

Two Galileo satellites launched into the wrong, eccentric orbit in 2014 turned into a redshift experiment: local position invariance holds to $2.5\times10^{-5}$.

SEP · lunar laser ranging

Do the Earth and Moon, with different self-energies, fall alike toward the Sun? A violation polarises the lunar orbit toward the Sun — the Nordtvedt effect. Corner cubes left in 1969 give $\eta_{\mathrm N} = (4.4\pm4.5)\times10^{-4}$.

this is the checkpoint's second clause

A torsion balance cannot falsify EEP: it contains no clock. A maser cannot falsify SEP: a hydrogen atom has no gravitational self-energy worth the name. Only a body the size of the Earth tests SEP, and only because the Moon's distance is known to millimetres. And the running example is an EEP experiment: a tower full of gamma rays tests local position invariance, and bounds $\eta$ not at all.

30 · masses

What the WEP says mathematically

free fall is a structure, not a force

WEP says: through each event $p$ and each admissible four-velocity $u$ at $p$ there passes exactly one free-fall worldline, and it does not depend on which body travels it.

So gravity determines a map $$(p, u) \;\longmapsto\; \text{a curve through } p \text{ with tangent } u ,$$ a family of preferred curves on spacetime — a path structure, the same kind of datum as the family of straight lines on an affine space.

In Newtonian language: the equation $\ddot{\vec x} = -\nabla\Phi$ has no $m$ in it. In unit 12's language, the Lagrangian $L = \tfrac12 m|\dot{\vec x}|^2 - m\Phi$ has an overall $m$ that the Euler–Lagrange equations divide out.

height t Be and Ti, together p g

Free fall in a uniform field, drawn in spacetime (exaggerated). One curve leaves $p$ for each initial velocity; a beryllium ball and a titanium ball launched alike share one of them, whatever they are made of.

30 · masses

A property of the arena

position t +1 +½ 0 −½ −1 qE/m, in plot units: p E

The same launch, $p$ and $u$ fixed, in a uniform electric field instead (exaggerated). Now $q/m$ picks the curve: bodies that start together part company.

why this is the whole programme

A field that acts on every body identically is indistinguishable from a property of the arena. Electromagnetism is not like this: unit 28's Lorentz force carries $q/m$, so charged and neutral bodies take different paths and the field is visibly a thing on spacetime.

A rule assigning a preferred family of curves to a manifold is an affine connection; its preferred curves are geodesics. Unit 32 defines both. Everything after this unit is the construction of that object.

The one available candidate is already in hand: unit 27's free particle extremises proper time. If the metric is allowed to vary from place to place, extremal proper time becomes a nontrivial equation — unit 32.

section 2

Three consequences, before any geometry

Light loses frequency climbing, clocks low down run slow, and light bends — all from a box and a Doppler shift.

30 · consequences

The rocket argument

A rocket of height $h$, proper acceleration $g$, far from everything. The floor emits a photon upward; work in the inertial frame momentarily comoving at that instant.

three lines

1. To first order the photon reaches the ceiling after time $t = h/c$.
2. By then the ceiling has speed $\Delta v = gt = gh/c$, away from the source.
3. Unit 26's Doppler factor for a receding receiver is $1 - \Delta v/c$ to first order.

gravitational redshift, from the equivalence principle $$\boxed{\ \frac{\Delta\nu}{\nu} \;=\; -\frac{gh}{c^2} \;=\; \frac{\Delta\Phi}{c^2}\ }$$
ct height ceiling's place at emission floor photon emitted received ceiling tilted: receding at Δv ≈ gh/c h

The rocket in the inertial frame of the floor at emission (exaggerated: $gh/c^2 = 0.3$ here). When the photon arrives, the ceiling's worldline has tilted: it is moving away. No gravity anywhere in the picture.

$\Delta\Phi = \Phi_{\text{emit}} - \Phi_{\text{receive}}$ in a general static field. Checks. $gh/c^2$ dimensionless ✓; $g\to0$, no shift ✓; receiver recedes, so redder ✓.

30 · consequences · example

Worked example 1 — Pound and Rebka's tower

the running example, evaluated

1. $h = 22.5$ m (Jefferson Laboratory, Harvard), $g = 9.80665\ \mathrm{m\,s^{-2}}$, $c^2 = 8.987552\times10^{16}\ \mathrm{m^2\,s^{-2}}$.

2. $\dfrac{gh}{c^2} = \dfrac{9.80665\times22.5}{8.987552\times10^{16}} = \mathbf{2.455\times10^{-15}}$.

3. Pound and Rebka measured the difference between source-up and source-down, which is $2gh/c^2 = 4.910\times10^{-15}$.

4. Their result: $(5.13\pm0.51)\times10^{-15}$, i.e. $(2.57\pm0.26)\times10^{-15}$ per one-way trip.

5. Ratio measured/predicted $= 1.04\pm0.10$. Inside the error bar.

how anyone measures $10^{-15}$

The Mössbauer effect: a $^{57}$Fe nucleus in a crystal emits a $14.4$ keV gamma ray with the recoil taken by the whole crystal, so the line is absurdly narrow — $\Gamma/E = 3\times10^{-13}$. A shift of $10^{-15}$ is a detectable fraction of that width.

The shift was cancelled by moving the source on a loudspeaker cone: the speed needed is $v = c\,(2gh/c^2) = 1.47\ \mu\mathrm{m\,s^{-1}}$.

check

$g$ from $GM_\oplus/R_\oplus^2 = 9.7983\ \mathrm{m\,s^{-2}}$ instead of standard gravity gives $2.453\times10^{-15}$ — a $0.09\%$ change, a hundred times inside the experiment's error bar ✓.

30 · consequences · example

Worked example 2 — the clocks that run the satnav

the GPS budget

A clock moving with speed $v$ at potential $\Phi$ runs, relative to coordinate time in the Earth-centred inertial frame, at $$\frac{\mathrm d\tau}{\mathrm dt} = 1 + \frac{\Phi}{c^2} - \frac{v^2}{2c^2} + O(c^{-4}).$$ First term: section 2's redshift. Second: unit 26's time dilation, expanded.

Potential. $a = 26\,561$ km, $R_\oplus = 6378.137$ km, $GM_\oplus = 3.986004\times10^{14}\ \mathrm{m^3\,s^{-2}}$: $$\frac{GM_\oplus}{c^2}\Big(\frac1{R_\oplus} - \frac1a\Big) = 5.2837\times10^{-10} \;\Rightarrow\; +45.65\ \mu\mathrm{s/day}.$$

Speed. $v = \sqrt{GM_\oplus/a} = 3874\ \mathrm{m\,s^{-1}}$, so $v^2/2c^2 = 8.349\times10^{-11} \Rightarrow -7.21\ \mu\mathrm{s/day}$.

Net. $+38.44\ \mu$s/day; $+38.54$ with the ground clock's own $465\ \mathrm{m\,s^{-1}}$ of rotation restored.

what it costs to ignore

Position is inferred from time-of-flight, so a clock error $\delta t$ is a range error $c\,\delta t$: $$c \times 38.5\ \mu\mathrm s = \mathbf{11.5\ km\ per\ day}.$$

The satellite oscillators are therefore set low before launch, by a fractional $4.4647\times10^{-10}$, so that they tick at $10.23$ MHz once in orbit.

30 · consequences · example

One term alone

both terms, always

The two effects have opposite signs and differ by a factor of six. Keep only the potential term and the prediction is $+45.65$ — $7.2\ \mu$s/day fast. Keep only the speed term and it is $-7.21$, off by $45.7\ \mu$s/day: worse than dropping both, which is off by $38.4$.

It is the cleanest working demonstration that special and general relativity are one subject.

right answer predicted neither 0 off by 38.4 speed only −7.21 off by 45.7 potential only +45.65 off by 7.2 both +38.44 −10 0 10 20 30 40 50 μs per day gained in orbit

Four predictions for the daily gain of an orbiting clock over a ground clock, against the right answer (dashed). Section 2's redshift alone overshoots by $7.2\ \mu$s; unit 26's time dilation alone has the wrong sign.

30 · consequences

Clocks, and the first non-constant metric

Read the redshift as a statement about clocks. A signal emitted at rate $\nu_1$ from potential $\Phi_1$ is received at rate $\nu_2$ at $\Phi_2$ with $\nu_2/\nu_1 = 1 + (\Phi_1-\Phi_2)/c^2$. Nothing accumulates in between — the field is static — so this is a permanent ratio of clock rates, not a transient.

the uniform-field metric

Let $t$ label the ticks of a reference clock at $\Phi = 0$. Then a static clock at $\Phi$ has $\mathrm d\tau = (1 + \Phi/c^2)\,\mathrm dt$, so $$-c^2\mathrm d\tau^2 = -\Big(1 + \frac{2\Phi}{c^2}\Big)c^2\,\mathrm dt^2 + \dots$$ to first order in $\Phi/c^2$: the $00$ component of a metric that varies from place to place.

Notation: from here on $g_{\alpha\beta}$, always with two indices, is a metric component; a bare $g$ is still the acceleration, $9.80665\ \mathrm{m\,s^{-2}}$ for the Earth.

what is and is not established

Established: $g_{00} = -(1 + 2\Phi/c^2)$ to first order. Not established: the spatial part. The dots hide $g_{ij}$, and the equivalence principle alone cannot fix it — the redshift is a statement about clocks only.

That gap has a famous cost: the next slide's light deflection comes out exactly half the true value.

Checks. $\Phi/c^2$ is dimensionless ✓. $\Phi\to0$: $\eta_{\mu\nu}$ back, and unit 26's Minkowski space ✓. Newtonian limit: a slow particle extremising $\int\mathrm d\tau$ in this metric obeys $\ddot{\vec x} = -\nabla\Phi$ — unit 35 does it properly.

30 · consequences

Light bends — and by half the right amount

Back in the rocket. A photon crosses the cabin horizontally, width $L$, in time $L/c$; in that time the cabin has risen by $\tfrac12 g(L/c)^2$. So the photon's path, drawn in the cabin, is bent downward, and the deflection angle over the crossing is $gL/c^2$. In a field that varies along the ray, the same argument applied to each short stretch $\mathrm d\ell$ gives $\mathrm d\theta = (g_\perp/c^2)\,\mathrm d\ell$, with $g_\perp$ the field's component across the ray.

g inertial frame: the cabin rises photon goes straight gL/c² cabin frame: the photon falls L ½g(L/c)²

The same crossing seen twice, at four equal instants (exaggerated). Left, in the inertial frame: the photon goes straight and the cabin rises under it. Right, in the cabin: the cabin is still, so the photon's path is the parabola $y = -gx^2/2c^2$, leaving at the angle $gL/c^2$.

30 · consequences

Deflection by the Sun, added up along the ray

deflection by the Sun, from the equivalence principle alone

Adding up $\mathrm d\theta = (g_\perp/c^2)\,\mathrm d\ell$ along a ray grazing a mass $M$ at impact parameter $b$ gives $$\Delta\theta_{\mathrm{EP}} = \frac{2GM}{c^2 b}.$$ For the Sun: $2GM_\odot/c^2 = 2953.25$ m, $R_\odot = 6.957\times10^8$ m, so $\Delta\theta = 4.245\times10^{-6}$ rad $= \mathbf{0.876''}$.

The integrand is largest at closest approach and falls off as $|x|^{-3}$ either side, so almost all of the bend happens within a few $b$ of the Sun: the ray is straight, then turns, then is straight again.

Sun b ray g⊥ −2 −1 0 1 2 x / b along the ray area 2 g⊥ b²/GM

Top: a ray passing the Sun at impact parameter $b$ (not to scale), with the field's component across it. Bottom: that component along the ray, in units of $GM/b^2$, against $x/b$. The area under the whole curve, tails included, is $2$: that is the whole calculation.

30 · consequences

The factor of two, and 1919

the factor of two

Einstein published $0.83''$ on this argument in 1911 (solar data of the day) and $1.75''$ in 1915. The true value is $$\Delta\theta = \frac{4GM_\odot}{c^2R_\odot} = \mathbf{1.751''} .$$ The missing half comes from $g_{ij}$ — the spatial part of the metric that the clocks slide could not determine.

Eddington's 1919 eclipse expedition measured $1.98\pm0.12''$ (Sobral, four-inch) and $1.61\pm0.30''$ (Príncipe).

why this is good news

The equivalence principle is exactly strong enough to predict the effects that involve only clocks, and exactly too weak for the ones that involve space. That is a sharp, falsifiable boundary, and 1919 is where it was drawn.

0.0 0.5 1.0 1.5 2.0 deflection at the limb (″) equivalence principle 0.876″ general relativity 1.751″ Sobral 4-inch Príncipe Sobral astrographic radio interferometry discarded

Deflection at the Sun's limb: the two predictions (lines) against the 1919 plates and modern radio interferometry (points, one-sigma bars). Both sets of plates that were kept disfavour the equivalence-principle value.

section 3

Rindler: a varying metric on a flat spacetime

Take unit 27's hyperbola seriously as a laboratory floor, and see how much of gravity comes for free.

30 · rindler

What a metric in arbitrary coordinates is

the definition

$(V,\eta)$ is unit 26's vector space with its symmetric bilinear form. Let $x^\mu \mapsto y^\alpha(x)$ be a smooth invertible change of coordinates on a region. At each point the coordinate basis is $$e_{(\alpha)} := \frac{\partial x^\mu}{\partial y^\alpha}\,\hat e_\mu ,$$ the columns of unit 03's Jacobian — a basis of $V$ that varies from point to point.

The metric components are the matrix of $\eta$ in that basis: $$g_{\alpha\beta}(y) := \eta\big(e_{(\alpha)}, e_{(\beta)}\big) = \frac{\partial x^\mu}{\partial y^\alpha}\frac{\partial x^\nu}{\partial y^\beta}\,\eta_{\mu\nu}.$$

this is unit 16, unchanged

$\eta$ is a $(0,2)$-tensor: a bilinear map $V\times V\to\mathbb R$. Unit 16 proved that the matrix of such a map transforms as $g' = S^{\!\top}\!gS$ under a change of basis. The only new thing here is that $S$ is a function of position.

So $g_{\alpha\beta}(y)$ is not a new object. It is the same $\eta$, written in a basis that moves.

30 · rindler

Polar coordinates: a basis that moves

the trap this whole section is about

Non-constant $g_{\alpha\beta}$ therefore proves nothing about the spacetime. Polar coordinates on the Euclidean plane give $\mathrm dl^2 = \mathrm dr^2 + r^2\mathrm d\phi^2$, and the plane is flat.

The coordinate basis of polar coordinates is $e_{(r)} = (\cos\phi, \sin\phi)$ and $e_{(\phi)} = (-r\sin\phi,\, r\cos\phi)$ — the columns of the Jacobian of $(r,\phi)\mapsto(r\cos\phi, r\sin\phi)$. So $$g_{rr} = |e_{(r)}|^2 = 1,\qquad g_{r\phi} = 0,\qquad g_{\phi\phi} = |e_{(\phi)}|^2 = r^2 .$$

The component $r^2$ is the length of a basis vector, squared. The plane did nothing; the basis grew.

r = 1 r = 2 r = 3 e(φ), length 1 e(φ), length 2 e(φ), length 3 e(r), length 1

The coordinate basis at three points of the Euclidean plane. $e_{(r)}$ always has length $1$; $e_{(\phi)}$ has length $r$, so it grows as the point moves out. That growth, not any property of the plane, is the varying $g_{\phi\phi}$.

30 · rindler

The Rindler chart

Unit 27's Born-rigid family: one hyperbola per label $X \gt 0$, of constant proper acceleration $c^2/X$, all sharing the same lines of simultaneity through the origin. Take them as a static laboratory.

Rindler coordinates

With a reference acceleration $g$ and $X_0 := c^2/g$, $$ct = X\sinh\frac{gT}{c},\qquad x = X\cosh\frac{gT}{c},$$ for $X \gt 0$, $T\in\mathbb R$. $X$ labels the observer; $T$ is the proper time of the one at $X_0$.

the Rindler metric $$\mathrm ds^2 = -\Big(\frac{gX}{c}\Big)^{\!2}\mathrm dT^2 + \mathrm dX^2 + \mathrm dy^2 + \mathrm dz^2 .$$

Checks. $(gX/c)\,\mathrm dT$ is in metres ✓. At $X = X_0$ the coefficient is $c^2$, so $T$ is proper time there ✓. Small $gT/c$ near $X_0$: Minkowski back ✓.

two lines

Write $\theta := gT/c$. Then $$\mathrm d(ct) = \sinh\theta\,\mathrm dX + X\cosh\theta\,\tfrac gc\mathrm dT,$$ $$\mathrm dx = \cosh\theta\,\mathrm dX + X\sinh\theta\,\tfrac gc\mathrm dT.$$ Form $-\mathrm d(ct)^2 + \mathrm dx^2$. The cross terms cancel exactly ($-2\sinh\cosh + 2\cosh\sinh$), $\mathrm dX^2$ keeps $\cosh^2-\sinh^2 = 1$, and $\mathrm dT^2$ keeps $(gX/c)^2(\sinh^2-\cosh^2) = -(gX/c)^2$. $\square$

The coefficient $gX/c$ is $\sqrt{-g_{TT}}$, and it fixes the lapse function — the rate at which a static observer's proper time runs per unit of coordinate time, $\mathrm d\tau/\mathrm dT = gX/c^2 = X/X_0$. It depends on position — and the spacetime is exactly Minkowski.

30 · rindler

The wedge, and the horizon

what the chart covers

$(T,X)\mapsto(ct,x)$ with $X\gt0$ is a bijection onto the Rindler wedge $\;x \gt |ct|$, and onto nothing else.

proof

$x^2 - c^2t^2 = X^2 \gt 0$ and $x = X\cosh \gt 0$, so the image lies in the wedge. Conversely, given $x\gt|ct|$, set $X := \sqrt{x^2-c^2t^2} \gt 0$ and $\theta := \operatorname{artanh}(ct/x)$, which is defined because $|ct/x| \lt 1$; these invert the map, and both are unique. $\square$

At $X\to0$ the lapse $gX/c\to0$ and the proper acceleration $c^2/X\to\infty$. The boundary $x = |ct|$ is the Rindler horizon of unit 27.

x ct X = X₀ T const horizon horizon future wedge past wedge left wedge

Hyperbolae are the static observers, $X = $ const; rays from the origin are $T = $ const. The chart fills the right wedge and stops at the null lines $x = |ct|$, the horizon.

30 · rindler

The redshift again, exactly

static redshift in a static metric

If $g_{\alpha\beta}$ does not depend on the time coordinate $T$, then for two static observers at $X_1$, $X_2$, $$\frac{\nu_2}{\nu_1} = \frac{\sqrt{-g_{TT}(X_1)}}{\sqrt{-g_{TT}(X_2)}} .$$ For the Rindler metric $\sqrt{-g_{TT}} = gX/c$, so $\;\nu_2/\nu_1 = X_1/X_2$, exactly.

proof

A light signal from $X_1$ to $X_2$ is a curve $T(X)$ with $\mathrm ds^2 = 0$. Because the metric has no $T$-dependence, a signal emitted at $T_1+\Delta T$ is the $T$-translate of one emitted at $T_1$, so it arrives at $T_2+\Delta T$: the coordinate interval is preserved. Proper times are $\Delta\tau_i = \sqrt{-g_{TT}(X_i)}\,\Delta T/c$, and frequencies are their reciprocals. $\square$

horizon gT/c X₁ = X₀/2 X₂ = 3X₀/2 ΔT ΔT light 2 ticks per gap 6 ticks per gap

Light signals between two static observers, drawn in the Rindler chart. Every signal is the same curve slid up in $T$, so equal gaps in $T$ leave and arrive. The clocks' ticks (equal proper time) are wider apart in $T$ low down.

30 · rindler

The tower, exactly

the running example, exactly

Floor at $X_1$, ceiling at $X_2 = X_1 + h$. Then $$\frac{\nu_2}{\nu_1} = \frac{X_1}{X_1+h} = \frac1{1 + g_1h/c^2},$$ with $g_1 = c^2/X_1$ the floor's proper acceleration. Expanding: $\Delta\nu/\nu = -g_1h/c^2 + O((g_1h/c^2)^2)$.

Section 2's three-line argument was right to first order and no further, and now we know exactly what it dropped: for the tower, $(gh/c^2)^2 = 6.0\times10^{-30}$.

Check. $h\to0$: ratio $1$ ✓. $X_1\to\infty$ at fixed $h$: $g_1\to0$, no shift ✓. $X_1\to0$: the floor approaches the horizon and $\nu_2/\nu_1\to0$ — infinite redshift ✓.

0 0.5 1 1 2 3 g₁h/c² (height over distance to horizon) ν₂ / ν₁ exact: 1/(1 + u) first order: 1 − u the tower: u = 2.5×10⁻¹⁵

The received frequency ratio against $g_1h/c^2$: exact (solid) and section 2's first-order answer (dashed). They agree where the tower lives, at the far left; the first-order line reaches zero at $g_1h/c^2 = 1$ and goes negative, while the exact ratio only tends to zero, as the floor nears the horizon.

30 · rindler · example

Worked example 3 — the tower as a Rindler wedge

the Harvard tower, re-derived

1. Model the laboratory floor as the Rindler observer with proper acceleration $g$: $X_1 = c^2/g = 9.1648\times10^{15}$ m.

2. In light years, $X_1 = 9.1648\times10^{15}/9.4607\times10^{15} = 0.9687$ ly.

3. Ceiling: $X_2 = X_1 + 22.5$ m. Exact ratio $$\frac{\nu_1}{\nu_2} = \frac{X_2}{X_1} = 1 + \frac{gh}{c^2} = 1 + 2.4551\times10^{-15}.$$

4. So section 2's answer is exact here, read the right way: $\nu_1/\nu_2 = 1 + g_1h/c^2$ with the floor's proper acceleration, or $\Delta\nu/\nu = -g_2h/c^2$ with the ceiling's. Only $\Delta\nu/\nu = -g_1h/c^2$ stops at first order — P4 sorts the three out.

5. The horizon lies at $X = 0$: proper distance $0.9687$ light years below the floor.

what the model gets wrong, and by how much

The Earth's field is not the Rindler field. Rindler has $g(X) = c^2/X$, so over $22.5$ m it varies by a fractional $2.5\times10^{-15}$; the Earth's $g = GM/r^2$ varies by $2h/R_\oplus = 7.1\times10^{-6}$ — nine orders of magnitude more.

That difference is the tidal tensor, and it is the subject of section 5. The redshift does not notice it, because the redshift only sees $\int g\,\mathrm d\ell$.

checks

$c^2/g$: $\mathrm{(m^2s^{-2})/(m\,s^{-2})} = \mathrm m$ ✓. $X_2/X_1 - 1 = h/X_1 = hg/c^2$ ✓ — the same number as section 2, not merely close to it.

30 · rindler

The inoculation

the belief this section exists to destroy

"The metric components depend on position, therefore spacetime is curved, therefore there is gravity."

exhibit A

Polar coordinates on the plane: $g_{\phi\phi} = r^2$. Flat.

exhibit B

Rindler: $g_{TT} = -(gX/c)^2$, a lapse varying with height, an infinite redshift surface, a horizon, and observers who feel weight. Minkowski space.

exhibit C

Rotating coordinates (section 4): non-Euclidean spatial geometry. Minkowski space.

what does distinguish them

In every example above there exists a global coordinate change bringing $g_{\alpha\beta}$ to $\eta_{\mu\nu}$ everywhere at once. Section 5 shows that near the Earth there is not — and identifies exactly what obstructs it.

section 4

The rotating disc

A frame in flat spacetime whose space is already not Euclidean — the observation Einstein said pushed him to Riemann.

30 · disc

Rotating coordinates, and their metric

Minkowski space in cylindrical coordinates: $$\mathrm ds^2 = -c^2\mathrm dt^2 + \mathrm d\rho^2 + \rho^2\mathrm d\phi^2 + \mathrm dz^2 .$$ Pass to a frame rotating at angular velocity $\omega$ by $\phi = \phi' + \omega t$, so $\mathrm d\phi = \mathrm d\phi' + \omega\,\mathrm dt$.

the rotating metric $$\begin{aligned}\mathrm ds^2 = \;&-\Big(1 - \frac{\omega^2\rho^2}{c^2}\Big)c^2\mathrm dt^2 + 2\omega\rho^2\,\mathrm d\phi'\,\mathrm dt\\ &+ \mathrm d\rho^2 + \rho^2\mathrm d\phi'^2 + \mathrm dz^2 .\end{aligned}$$

Two new features at once: the lapse $\sqrt{1-\omega^2\rho^2/c^2}$ again depends on position, and there is now a cross term $g_{0\phi'}\ne0$ — the metric is not diagonal.

ρφ ct inertial co-rotating t = const rider's own “now” e(0) e(φ′)

The cylinder of radius $\rho$, cut and unrolled: arc length $\rho\phi$ across, $ct$ up. A co-rotating observer is a tilted line; the new time axis tilts with it, but the slices $t = $ const do not. That mismatch is $g_{0\phi'}$.

Checks. $\omega\rho/c$ dimensionless ✓; $\omega\to0$ gives cylindrical Minkowski back ✓; $g_{\phi'\phi'} = \rho^2$ unchanged, because the substitution does not touch $\mathrm d\phi'^2$'s coefficient ✓.

30 · disc

The light cylinder

the light cylinder

$g_{tt}$ vanishes at $\rho = c/\omega$ and is positive beyond. There, and outside, no observer can co-rotate: the curve $\rho,\phi',z$ constant is null, then spacelike.

For a millisecond pulsar at $716$ Hz the light cylinder is at $66.6$ km — a few stellar radii out, and where its magnetosphere is believed to end.

The co-rotating observer at radius $\rho$ moves, in the inertial frame, at $\omega\rho$. The lapse $\sqrt{1-\omega^2\rho^2/c^2}$ is unit 26's $1/\gamma$ at that speed, and it reaches zero exactly where the speed reaches $c$.

c/4 c/2 3c/4 ρ = c/ω outside: no co-rotating observer

Co-rotating observers seen from above, each with its speed $\omega\rho$ in the inertial frame (arrows to scale with one another). The speed grows linearly outward and reaches $c$ on the dashed circle $\rho = c/\omega$; beyond it, no observer can keep up.

30 · disc

What "the distance between two rotating observers" means

radar distance

An observer at fixed spatial coordinates bounces a light signal off a neighbour at $y^i + \mathrm dy^i$ and measures the round-trip proper time $\Delta\tau$. Define $\mathrm dl := c\,\Delta\tau/2$.

the spatial metric $$\gamma_{ij} = g_{ij} - \frac{g_{0i}g_{0j}}{g_{00}} ,\qquad \mathrm dl^2 = \gamma_{ij}\,\mathrm dy^i\mathrm dy^j .$$

A symmetric bilinear form on each observer's orthogonal complement of their four-velocity — positive definite, by the signature.

When $g_{0i} = 0$ this is just $g_{ij}$, and no one notices the definition is needed. When $g_{0i}\ne0$ — a rotating frame — it is not, and the correction is the whole effect.

rider neighbour out: dy/(1−β) back: dy/(1+β) Δx⁰ dashed: no rotation dy along the rim

Radar between two neighbouring riders on the rim, in the rotating chart (exaggerated: $\omega\rho/c = 0.4$). Both are vertical lines. Light takes longer going with the rotation than against it, but only the round trip $\Delta x^0$ enters $\mathrm dl$.

30 · disc

Radar distance, from one quadratic

proof

Set $\mathrm ds^2 = 0$ and solve for $\mathrm dx^0$: a quadratic $$g_{00}(\mathrm dx^0)^2 + 2g_{0i}\mathrm dx^0\mathrm dy^i$$ $$+\ g_{ij}\mathrm dy^i\mathrm dy^j = 0,$$ whose two roots are the outward and return legs, with difference $\Delta x^0 = 2\sqrt D/(-g_{00})$ for $$D := (g_{0i}\mathrm dy^i)^2 - g_{00}\,g_{ij}\mathrm dy^i\mathrm dy^j .$$ The waiting observer's proper time is $\Delta\tau = \sqrt{-g_{00}}\,\Delta x^0/c$, so $\mathrm dl = c\Delta\tau/2 = \sqrt{D}/\sqrt{-g_{00}}$, and $\mathrm dl^2 = D/(-g_{00})$ is the boxed form. $\square$

0 2πρ arc length round the rim same line same line ct rider back to the rider, late rider's “now”

The rim unrolled, its two ends the same place. The riders' local "now" (dashed), carried once round, returns to the same rider later than it left.

The catch. Each rider's spatial metric is fine, but the slices do not join up: carried round the rim, the riders' simultaneity returns late by $\Delta x^0 = 2\pi\omega\rho^2c/(c^2-\omega^2\rho^2)$ — the Sagnac effect.

30 · disc

Circumference over diameter is $\pi\gamma$

Apply $\gamma_{ij} = g_{ij} - g_{0i}g_{0j}/g_{00}$ to the rotating metric. Radially, $g_{0\rho} = 0$, so $\gamma_{\rho\rho} = 1$. Around the rim, $$\gamma_{\phi'\phi'} = \rho^2 - \frac{(\omega\rho^2/c)^2}{-(1-\omega^2\rho^2/c^2)} = \frac{\rho^2}{1 - \omega^2\rho^2/c^2} .$$

the Ehrenfest paradox, resolved as geometry

Radius measured by rotating rulers: $R = \rho$. Circumference measured by rotating rulers: $$C = \int_0^{2\pi}\frac{\rho\,\mathrm d\phi'}{\sqrt{1-\omega^2\rho^2/c^2}} = 2\pi\gamma\rho,\qquad \gamma = \big(1-\tfrac{\omega^2\rho^2}{c^2}\big)^{-1/2}.$$ So $C/2R = \pi\gamma \gt \pi$: the rotating observers' space is not Euclidean.

The bare $\gamma$ is unit 26's Lorentz factor at the rim speed $\omega\rho$; the spatial metric $\gamma_{ij}$ always carries indices. They meet here: $\gamma_{\phi'\phi'} = \gamma^2\rho^2$.

at rest: 16 fit spinning: 20 fit 0.6c radius: 2.55 rulers radius: still 2.55

The lab's view of the riders' rulers (exaggerated: rim speed $0.6c$, $\gamma = 1.25$). Rulers along the rim move along their length and are contracted; rulers along a radius move sideways and are not. More rim rulers fit: $20$ where $16$ fitted at rest.

30 · disc

How big the excess is

how big

Rim speed $0.1c$: $\gamma = 1.005038$, so $C/2R = 1.005\pi$ — a half-per-cent excess.

Rim speed $0.18c$ (a $12$ km sphere at $716$ Hz): $\gamma = 1.01660$.

A laboratory ultracentrifuge rim at $1000\ \mathrm{m\,s^{-1}}$: $\gamma - 1 = 5.6\times10^{-12}$.

and the spacetime is still flat

Every event here is an event of Minkowski space. The non-Euclidean geometry belongs to a family of observers, not to the spacetime — the lesson of the tower as a Rindler wedge, in the spatial slot instead of the temporal one.

Checks. $\omega\to0$: $\gamma\to1$, $C = 2\pi R$ ✓. $\rho\to c/\omega$: $C\to\infty$ ✓, consistent with the light cylinder.

10⁻¹² 10⁻⁹ 10⁻⁶ 10⁻³ 1 10⁻⁶ 10⁻⁴ 10⁻² 1 rim speed / c γ − 1 centrifuge rim, 1 km/s 0.1c pulsar, 0.18c β²/2

The excess $C/2\pi R - 1 = \gamma - 1$ against rim speed, both axes logarithmic. It grows as $\beta^2/2$ — a straight line of slope two — until near $c$, where it runs away. The three examples on the left are marked.

section 5

What no coordinate change can remove

The tidal tensor of unit 05, met again as the first curvature invariant — and the end of Part D.

30 · tides

How much of a metric a freely falling frame can flatten

Fix an event $p$. Expand a coordinate change about it: $$y^\mu = A^\mu{}_\nu x^\nu + \tfrac12 B^\mu{}_{\nu\rho}x^\nu x^\rho + \tfrac16 C^\mu{}_{\nu\rho\sigma}x^\nu x^\rho x^\sigma + \dots$$ and count what each order of coefficients can buy, order by order, against the Taylor coefficients of $g_{\mu\nu}$ at $p$.

10 16 set g(p) A: 4 × 4 6 spare 40 40 kill ∂g(p) B: 4 × 10 exact 100 80 kill ∂∂g(p) C: 4 × 20 20 survive must adjust (metric) can adjust (coordinates)

At each order, what the coordinate change can adjust (solid) against what it must adjust (hollow). First order has $6$ to spare, second order matches exactly, third order is $20$ short.

the count, read

The $6$ spare at first order are the Lorentz group: unit 26's $3$ boosts and $3$ rotations.

The exact match at second order is the freely falling frame: every first derivative of the metric can be set to zero at a point, which is the equivalence principle written in components.

The $20$ left at third order are unremovable. Unit 33 shows they are exactly the components of the Riemann tensor in four dimensions, $n^2(n^2-1)/12 = 20$.

Cited. That the linear systems at each order are actually solvable — not merely of the right size — is proved in unit 32, by constructing normal coordinates. The count is what is proved here.

30 · tides

The Newtonian version, proved in three lines

what a freely falling frame removes, and what it does not

Let $\vec x_0(t)$ be any twice-differentiable curve, and change to the frame $\vec x' = \vec x - \vec x_0(t)$. In it a free particle obeys $$\ddot{\vec x}' = -\nabla\Phi(\vec x_0+\vec x') - \ddot{\vec x}_0 .$$ Choosing $\ddot{\vec x}_0 = -\nabla\Phi(\vec x_0)$ kills the field at $\vec x' = 0$, for all $t$.

but the second derivatives are untouched

$\partial'_i\partial'_j$ of the new potential $\Phi(\vec x_0(t)+\vec x') + \ddot{\vec x}_0\cdot\vec x'$ is $$\partial_i\partial_j\Phi + \partial'_i\partial'_j\big(\ddot{\vec x}_0\cdot\vec x'\big) = \partial_i\partial_j\Phi ,$$ because the added term is linear in $\vec x'$. $\square$

−0.8 −0.6 −0.4 1.5 2 2.5 3 3.5 distance from the centre / R⊕ Φ in units of GM/R⊕ chosen point inertial frame falling frame

The Earth's potential along a vertical line (solid), and the same potential seen from the falling frame (dashed): a straight line has been added. It flattens the slope at the chosen point, and cannot touch the bend.

30 · tides

What the falling observer still measures

observer to the Earth's centre stretched: eigenvalue −2k squeezed: +k

A ring of free test particles released at rest around a falling observer, and the same particles a moment later (exaggerated). Along the line to the Earth's centre the ring stretches; across it, it squeezes — at half the rate, eigenvalues $(-2, 1, 1)$.

so the tidal tensor is the invariant

Unit 05's $T_{ij} = \partial_i\partial_j\Phi$ survives every change to a freely falling frame, and unit 05's deviation equation $\ddot\xi_i = -T_{ij}\xi_j$ is what the falling observer still measures.

Both slogans are true. "Gravity is not a force": $\nabla\Phi$ is frame-dependent and can always be made zero at a point. "Gravity is real": $T_{ij}$ cannot, and in vacuum $\operatorname{tr}T = 0$ forces a stretch for every squeeze.

Checks. $[T] = \mathrm s^{-2}$ ✓ — the square of a frequency. Uniform field $\Phi = gz$: $T = 0$, and indeed a uniform field is entirely removable, which is the elevator ✓.

30 · tides · example

Worked example 4 — how local is "local"?

a cubic metre, for one second, on the Earth

1. $T_{ij} = (GM_\oplus/r^3)(\delta_{ij} - 3n_in_j)$ from unit 05, with $\hat n$ the unit vector from the Earth's centre: eigenvalue $-2GM_\oplus/r^3$ along $\hat n$, and $+GM_\oplus/r^3$ twice across it.

2. $GM_\oplus/R_\oplus^3 = 3.986004\times10^{14}/(6.378137\times10^6)^3 = 1.5362\times10^{-6}\ \mathrm{s^{-2}}$.

3. Two balls $1$ m apart vertically: relative acceleration $2\times1.5362\times10^{-6} = 3.07\times10^{-6}\ \mathrm{m\,s^{-2}}$, separating.

4. After $1$ s the extra separation is $\tfrac12(3.07\times10^{-6})(1)^2 = \mathbf{1.54\ \mu m}$.

5. In the same second both have fallen $4.90$ m. The tidal residue is $3.1\times10^{-7}$ of it.

the Earth (centre far below) separate converge

Two pairs of balls dropped near the Earth (not to scale). Each ball falls towards the centre: the lower of the vertical pair is nearer, so falls faster; the side-by-side pair fall along converging radii.

Check. Horizontally the two balls converge at $1.54\times10^{-6}\ \mathrm{m\,s^{-2}}$ — half the vertical rate, opposite sign, exactly the eigenvalue ratio $(-2,1,1)$ ✓.

30 · tides · example

Local means: below your resolution

what "local" means, quantitatively

The equivalence principle holds in a box of size $L$ for a time $\tau$ to whatever accuracy $(GM/r^3)L\tau^2$ — the vertical pair's extra separation — is below your instrument's resolution. It is a statement with an error bar, not an exact symmetry.

Two balls $1$ m apart, separations resolved to $10^{-18}$ m: the elevator is unmasked in $0.8\ \mu$s.

and this is why it is a principle about points

No box is small enough to make $T_{ij}$ vanish, only small enough to hide it: shrinking $L$ shrinks the effect linearly, never to zero. Over the tower's $22.5$ m it is $6.91\times10^{-5}\ \mathrm{m\,s^{-2}}$, or $7.05\times10^{-6}$ of $g$ — what no Rindler wedge has.

10⁻¹⁸ 10⁻¹⁴ 10⁻¹⁰ 10⁻⁶ 10⁻² 10⁻⁶ 10⁻⁴ 10⁻² 1 time since release (s) extra separation (m) 0.81 μs LIGO-class, 10⁻¹⁸ m 8 ms an atom, 10⁻¹⁰ m 0.81 s a micron

The extra separation of two balls dropped $1$ m apart vertically, against time, both axes logarithmic. Each horizontal line is a resolution; where the curve crosses it, that instrument unmasks the elevator.

30 · tides

There is no global inertial frame

the claim that ends Part D

Suppose gravity were a force field on Minkowski space. Then the inertial frames of unit 26 would exist globally, and in one of them free particles with no force on them move on straight lines.

But the WEP says gravity acts on every body identically, so "no force on them" cannot be arranged, and the frames that make free fall look force-free are the freely falling ones — which differ from place to place, by exactly $T_{ij}\ne0$.

Newtonian version, complete

Suppose a single change $\vec x' = \vec x - \vec x_0(t)$ made every free-fall worldline straight in a region. Then $\nabla\Phi(\vec x) = -\ddot{\vec x}_0(t)$ throughout it, a function of $t$ alone, so $\partial_i\partial_j\Phi \equiv 0$ there. Contrapositive: where $T\ne0$, no such frame exists. $\square$

Earth each box: inertial, to first order

Small freely falling boxes around the Earth, each with its own acceleration (arrows, to scale). Each box is an inertial frame; one frame for the whole ring would need every arrow equal, and no two of them are.

30 · tides

What survives, and what does not

what survives, and what does not

Survives: inertial frames at a point, to first order — the counting argument's first two orders. That is all the equivalence principle ever claimed.

Does not survive: one flat metric covering a region containing matter. So there is no arena on which to write "gravity is a field", because the arena was supposed to be the thing the field lives on.

what this does not yet prove

It does not prove that spacetime is curved — "curvature" has no definition until unit 33. It proves that flat spacetime with a global inertial frame is inconsistent with $T_{ij}\ne0$, and so that the next unit must build a spacetime without one. That is unit 31.

30 · tides

Why not just put a field on flat spacetime anyway?

The natural objection: electromagnetism is a field on Minkowski space, so write gravity as one — a symmetric tensor field $h_{\mu\nu}$ sourced by mass-energy. Here is why the programme eats itself.

the Newtonian seed, complete

The field has energy. From unit 05's $\nabla^2\Phi = 4\pi G\rho$ and the divergence theorem, $$U = \tfrac12\!\int\!\rho\Phi\,\mathrm dV = -\frac1{8\pi G}\!\int\!|\nabla\Phi|^2\,\mathrm dV ,$$ an energy density $-|\nabla\Phi|^2/8\pi G$. By $E = mc^2$ that energy has mass; by the equivalence principle in its strong form — the only one that speaks about gravitational self-energy at all, as P7 makes precise — it gravitates. So $$\nabla^2\Phi = 4\pi G\Big(\rho - \frac{|\nabla\Phi|^2}{8\pi Gc^2}\Big) ,$$ and the corrected $\Phi$ changes the correction, for ever. A linear theory of gravity is not self-consistent.

Deser's argument — cited

The same for a massless spin-2 field $h_{\mu\nu}$ on Minkowski, coupled to the total stress-energy including its own: the iteration closes, and its sum is the Einstein–Hilbert action of unit 35 for $$g_{\mu\nu} = \eta_{\mu\nu} + h_{\mu\nu} .$$

S. Deser, Gen. Rel. Grav. 1, 9 (1970). Needs units 29 and 35; P7 does the Newtonian half in full.

the punchline

In the resulting theory nothing measures $\eta$: every rod, clock and ray responds to $g$. You have not described gravity on Minkowski space — you have rediscovered general relativity under a misleading name.

30 · closing

The running example, closed

the photon in the tower, three times

Section 2, from the principle alone: a rocket and a Doppler shift give $\Delta\nu/\nu = -gh/c^2 = -2.455\times10^{-15}$.

Section 3, from a metric on flat spacetime: $\nu_1/\nu_2 = X_2/X_1$, exactly $1 + gh/c^2$ — the same number, with the error term now known to be $6\times10^{-30}$.

Unit 36, from the Schwarzschild solution: $\sqrt{(1-r_s/r_1)/(1-r_s/r_2)}$, whose expansion is the same again.

Measured: $(2.57\pm0.26)\times10^{-15}$. And $38.5\ \mu$s/day keeps a satellite fleet honest.

and what it did not prove

The redshift is a clock effect, and flat spacetime can produce it — the Rindler wedge does, with a horizon thrown in. The redshift is therefore evidence for the equivalence principle and not evidence for curvature.

What is evidence for curvature is $T_{ij}\ne0$: the $20$ numbers the counting argument could not remove.

What comes next.
31 builds a spacetime with no global chart: manifolds, tangent spaces, tensor fields.
32 gives it a metric and a connection, and free fall becomes a geodesic.
33 defines curvature and proves the $20$ are the Riemann tensor.
37 finishes the light-bending factor of two, and gets $43''$ per century.

30 · checkpoint

Checkpoint

you can now

Derive the gravitational redshift from the equivalence principle with no geometry and match Pound–Rebka within its error bar; state the weak, Einstein and strong equivalence principles with an experiment that distinguishes them; and exhibit a non-constant metric on flat spacetime — thereby proving that non-constant metric components alone are not gravity.

it is false if

your redshift derivation quotes $mgh$ for a photon; or you cannot name an experiment that bounds SEP but not WEP, or WEP but not EEP; or, handed $\mathrm ds^2 = -(gX/c)^2\mathrm dT^2 + \mathrm dX^2$, you call it a gravitational field.

to check it

Close the deck. On paper: the rocket argument to $2.455\times10^{-15}$, compared with $(2.57\pm0.26)\times10^{-15}$; the three principles with Eöt-Wash, Gravity Probe A and lunar laser ranging against them; and the Rindler metric derived from $ct = X\sinh(gT/c)$, $x = X\cosh(gT/c)$. Then ./mr problems 30.