Part III · General Relativity — Chapter 3.4
Curvature
A test for curvature that can be run from inside, with no outside to look in from. It measures the tide.
Chapter 3.3 built two objects and issued one warning. The metric measures. The connection compares. The warning was that neither position-dependent metric components nor non-zero connection coefficients count as evidence of curvature. The flat plane in polar coordinates has both, and it is the flat plane. So no test for curvature yet exists, and this chapter builds one.
The test has to satisfy a hard constraint that Chapter 3.2 §1.2 imposed and never relaxed. It must be conducted entirely from within the space. Nothing may refer to an ambient room, a normal vector sticking out, or a picture drawn from outside. That rules out every intuitive definition of curvature anyone arrives with, and it leaves exactly one available instrument, which Chapter 3.3 §6 has just finished building. Carry a vector around a closed loop and see whether it comes back the way it left. Every step of that procedure stays inside the space. Transport is intrinsic, a closed loop is intrinsic, and the comparison at the end is between two vectors at the same point, which is what makes it legitimate. If the answer is ever "no", the space is curved, and how badly is a number.
Here is the route, announced in advance. Section 1 sets up the loop test and runs it on a sphere. The answer is derived analytically from Chapter 3.3's Christoffel symbols and measured numerically in the figure. The two agree, and what they agree on is the enclosed area divided by the square of the radius. Section 2 is the longest computation in this book so far: the commutator of two covariant derivatives, which is the loop test made infinitesimal. Section 3 collects the payoff. The pieces of the connection that are not tensorial cancel, and what is left is a genuine tensor. Section 4 is the centre of Part III. Two nearby geodesics drift apart at a rate set by that tensor, and setting the result beside Chapter 3.1's Newtonian tidal equation shows they are the same equation. Sections 5 and 6 work out the symmetries, derive the count of twenty independent components in four dimensions, and take the traces. Section 7 derives an identity whose contracted form produces a tensor with zero divergence, and that single fact dictates the shape of the field equations in Chapter 3.6. Section 8 closes the loop opened in Chapter 3.3 §2.
Sign convention, stated loudly and once. This book defines the Riemann tensor by
with signature throughout. Books differ, in both places independently. Some define Riemann with the opposite overall sign. Some contract the first and third indices in the other order. With the conventions above, a sphere has positive Ricci scalar and matter has positive energy density on the right-hand side of Einstein's equations, which is the combination we want. Before importing a formula from anywhere else, check both signs. and remain explicit.
Tools you'll need. Chapter 3.3 throughout: the covariant derivative of its §5, its extension to tensors (3.3.31) and (3.3.32), the inhomogeneous transformation law (3.3.26) of the connection, parallel transport (3.3.35), the Christoffel formula (3.3.50), the geodesic equation (3.3.57) and the sphere's connection coefficients from §9. Chapter 3.1 §4 in detail, meaning the tidal equation, the point-mass tidal matrix, its traceless character in vacuum, and the ring that deforms into an ellipse. Section 4 below is where all of that is collected. Chapter 3.2 §8, the commutator of vector fields, whose second-derivative cancellation is the template for §2, and §7 for the tensor transformation law. Chapter 2.4 §5.1 (contraction), §6 (a tensor equation true in one chart is true in all) and §7.2 (counting independent components of a symmetric or antisymmetric array). Chapter 0.6 §6.1, Clairaut's theorem, used four separate times below. Chapter 0.5 §6, the spectral theorem, used once in §5.
1 · The loop test, and the sphere
Here is the test in full. Take a closed path, plant a vector at a point on it, carry the vector all the way round by the parallel-transport equation (3.3.35), and compare the arrival with the departure. Both vectors live in the same tangent space, so the comparison is legitimate in the strict sense of Chapter 3.2 §5.1. Transport preserves length by metric compatibility, so the only thing that can have happened along the way is a rotation. The angle of that rotation is the measurement.
Check first that the test gives nothing where it should. In flat space with Cartesian coordinates the connection vanishes, so (3.3.35) reads and the vector comes back identical. The angle is zero for every loop. Any non-zero answer is therefore a fact about the space and not about the chart, provided we also check that flat space still gives zero when the chart is curvilinear. Section 8 runs that check.
1.1 · A loop on a sphere, computed by hand
Here is where we are going, announced before we set off. We choose a closed path on a sphere of radius , integrate the transport equation along it in three pieces, and find that the vector returns rotated through an angle exactly equal to the area enclosed divided by . Everything we need comes from the Christoffel symbols computed in Chapter 3.3 §9, which were
with the angle from the north pole and the azimuth.
A convenient pair of numbers. Before integrating anything we should choose components that are easy to read. Components carry the length of their basis vector, and here the two basis vectors have different lengths: and . So define the orthonormal components
That last equality is just regrouped. In this pair, is how much of the vector points south and how much points east, each measured in ordinary length.
Leg one, along a circle of latitude , from to . The tangent to this leg has only a component, so in (3.3.35) the sum over keeps only the term :
Those are equations for and , and what we want are equations for and , so rewrite them. Since is constant along this leg, the factors and are constants and pass straight through the derivative:
In each line the constant was regrouped to build the other orthonormal component. In the first, . In the second, splits as , using .
Let's take two readings of (3.4.4) before integrating it. The first reading is that is constant, since . That is metric compatibility showing up as a conserved quantity, exactly as Chapter 3.3 §7.1 said it would.
The second reading is that the pair obeys precisely the equations of a rotation. To see it, write a rotation through angle as , and differentiate, which gives and . Matching that against (3.4.4) gives , so over the whole leg the vector turns through
a rotation measured positively from the southward direction toward the eastward one.
Legs two and three, along meridians. Now the tangent has only a component, so (3.3.35) keeps only the term :
The first of those vanishes because both and are zero in (3.4.1). So is constant outright. The second equation separates into , and integrating both sides gives , that is . Hence is constant too. Along a meridian, nothing rotates, and that is what we should expect. A meridian is a great circle and therefore a geodesic, and Chapter 3.3 §8 built geodesics to be the curves along which the angle to the direction of travel is held fixed.
The one subtlety, which is the frames at the pole. If the loop passes through the north pole we must be careful, because is not a single frame there. Watch what happens to it. As along the meridian of azimuth , the southward direction becomes the horizontal direction pointing away from the pole at azimuth . In the ambient description, used here only to name directions, and . So the frame belonging to azimuth is the frame belonging to azimuth turned through . The consequence is the piece we need. A single fixed vector at the pole, described first in the frame of azimuth and then in the frame of azimuth , has its component pair rotated by between the two descriptions.
Assemble the loop. Start at . Go east along the latitude circle to , then north up that meridian to the pole, then south down the meridian of azimuth back to . Now add the rotations in the order they were picked up:
The area enclosed. To make anything of that angle we need the area of the region the loop bounds, so compute it next. The region is the wedge of the polar cap between azimuths and , running from the pole down to colatitude . The area element on the sphere is , since the metric is diagonal with . Integrating over the wedge,
Both numbers are now in hand, and each of them is the same product , once with a factor in front and once without. So the ratio of (3.4.7) to (3.4.8) carries no trace of the loop at all, and rearranging that ratio gives the result in its usual form:
In: the sphere's Christoffel symbols, the parallel-transport equation, one separable first-order equation, and care about which frame is being used at the pole.
Out: a vector carried round that loop returns rotated, in the same sense as the loop was circulated, through an angle equal to the enclosed area divided by .
What is remarkable about it. The rotation depends on the loop only through the area it encloses. Not its shape, not its position on the sphere, not how the transport was parametrised. So the quantity that belongs to the space rather than to the loop is the ratio , which survives as the loop shrinks to nothing. That number is what we are going to call curvature, and §9 recovers exactly from the tensor built in §2.
Every intuitive account of curvature smuggles in a viewpoint from outside — a rubber surface seen to sag, a ball seen to bulge, a direction sticking into a surrounding room. None is available here, since there is no room and no outside, and the difficulty of this chapter is finding a test a creature confined to the surface could run. One instrument survives the restriction, and the previous chapter finished building it: carry a direction around a closed circuit and see whether it comes home pointing the way it left.
Everything about that procedure stays inside. The circuit lies on the surface, the carrying rule refers only to the surface, and the final comparison is between two directions at one and the same place, which was always the one permitted comparison. Since carrying preserves lengths, the only thing that can have happened is a turn, whose size anyone on the surface can measure.
Running the test on a globe with pencil and paper gives an answer of startling neatness. The turn depends on the circuit only through the area it surrounds, not on its shape or position. So the quantity belonging to the surface rather than to any circuit is the turn divided by the area, and that ratio survives as the circuit shrinks to a point. It is the reciprocal of the radius squared, and this chapter turns it into a proper object.
2 · The commutator, and the tensor it produces
This is the longest computation in the book so far. The plan comes first, so that you can follow the whole argument without opening a single grind box.
Why this object. Section 1's loop had two directions in it. You go one way, then the other, then back the first way, then back the second. Shrink that loop and what is left is precisely the difference between differentiating along then and differentiating along then . So the infinitesimal loop test is the commutator applied to a vector, and that is what we compute.
Three steps. First, is a tensor with one upper and one lower index, so name it and put it aside. Second, apply to that object, which by Chapter 3.3 (3.3.32) needs a derivative and one connection term per index, and then expand the derivative of the product inside. That gives six terms in all. Third, subtract the same expression with and exchanged, and identify which terms are symmetric in and therefore die.
What to watch for. Every term containing a derivative of cancels. That is the surprise. What is left is proportional to itself with no derivatives on it. That is what makes the answer a tensor rather than a differential operator, and it is what §3 cashes in.
2.1 · The computation
Step one. Write . This is a type tensor by the construction of Chapter 3.3 §5.
Step two. Now differentiate that object covariantly. Equation (3.3.32) gives one for the upper index and one for the lower one:
Step three. Put back in. In the first term the product rule of Chapter 0.1 §4 acts on and produces two pieces. In the third term the bracket is exactly , and we leave it that way, which keeps the expression short and makes the cancellation visible. Labelling the six terms for reference:
The grind box below writes that out with nothing folded away, for anyone who wants to see every index in place. The argument does not need it.
Grind box — the same six terms, with every substitution written out
Start from (3.4.10) and substitute in all three places, being careful to rename the summed index in each so that no letter does two jobs.
The first term.
where the product rule was applied to , both factors being functions of position. These are , and .
The second term. Here , so
which are and . Note that is summed inside the double product. It is the index shared by the two connection factors, and it is what makes a matrix product rather than an entry-by-entry one.
The third term. is by definition , and we deliberately do not expand it, because the whole term is about to vanish for a reason that has nothing to do with its contents. Written out it would be , which is seven terms in total rather than six. Folding that pair back into is the only compression made anywhere in this computation.
Collecting gives (3.4.11) exactly.
2.2 · Antisymmetrising, one term at a time
Now write the same expression with and exchanged and subtract. We go through the six terms in order. Each one is a separate small argument, and each is named.
dies by Clairaut. The term is , an ordinary second partial derivative of a set of smooth functions. Clairaut's theorem (Chapter 0.6 §6.1) says mixed partials commute, so exchanging and leaves it unchanged and the subtraction kills it. This is the same cancellation that Chapter 3.2 §8.3 used to build the Lie bracket.
survives. Exchanging and turns into , which is a genuinely different object. The difference is .
and die together. This is the one that needs a moment. Individually neither is symmetric, but their sum is. Exchange and in to get . Now relabel the summed index , which changes nothing since it is a dummy, and the result is , which is exactly. By the same two moves, exchanging in gives . So the pair maps to and is symmetric, and the subtraction removes it.
survives. Exchanging gives , and the two connection factors do not commute as index objects, so the difference is .
dies by vanishing torsion. The term is . Exchanging and affects only the two lower indices of the connection, and Chapter 3.3's Demand 2 made those symmetric: . So the term is unchanged and the subtraction kills it. Had we allowed torsion, this term would have survived and contributed to the answer, which is exactly how the general formula reads in books that keep torsion.
Two terms have survived, and . Collect them, and give the array they multiply a name:
That equation defines the symbol by what it does. The two terms that survived the subtraction say what its components are:
This is the Riemann curvature tensor. Before doing anything else with (3.4.13), notice its shape. It is antisymmetric in by construction, since swapping those two letters exchanges the first two terms with each other and the last two with each other, reversing the sign of the whole. And it is built from the connection and its first derivatives, hence from the metric and its first and second derivatives.
In: the covariant derivative of a tensor, the product rule, Clairaut's theorem, one relabelling of a dummy index, and the symmetry of the connection in its lower indices.
Out: the difference between differentiating in two orders is not a differential operator at all. It is multiplication by an array. Four of the six terms cancelled, and they were precisely the four containing derivatives of .
Cost: nothing was assumed beyond Chapter 3.3's two demands, and torsion is the only place a different choice would change the answer.
Shrinking the circuit test to a point converts it into a question about the order of two operations. Going a short way in one direction and then a short way in another, against the same two moves in the opposite order, traces out a small closed circuit, so the failure of the two orders to agree is exactly what the circuit measures. In the language now available, that failure is the difference between differentiating one way then the other and the other way then the first.
Computing it is the longest piece of algebra in the book so far, and it is worth knowing what to look for. Six terms appear. One is an ordinary second derivative and disappears because the order of those never matters. Two more form a pair that swaps into itself when the directions are exchanged, so the pair cancels against its mirror image. A fourth goes because those coefficients were required to be symmetric in their lower slots.
What matters is not the algebra but what survives it. Every term carrying a derivative of the transported field has vanished, and what remains is proportional to the field itself. An operation that looked certain to produce a differential operator has produced plain multiplication by an array of numbers, and that array depends on the geometry alone. It is the object this chapter is about.
3 · Why the result is a tensor
Now the payoff for §2's length. Look at what (3.4.13) is made of. Every ingredient on the right-hand side is a badly behaved object.
- The connection is not a tensor, by Chapter 3.3 §5.3.
- A derivative of a non-tensor is not a tensor either.
- A product of two non-tensors is not a tensor.
Yet the combination of them is perfectly well behaved. Here is the argument, which takes three lines because §2 did the work.
The left side is a tensor. Chapter 3.3 §5 established that maps tensors to tensors, one rank higher. So is a tensor, and is a tensor. A difference of two tensors of the same type is a tensor of that type (Chapter 2.4 §5.1). Hence is a tensor, whatever is.
The right side has no derivatives of . That is what §2's four cancellations bought. If even one of , , , had survived, the right side would depend on how varies near the point and the next step would be unavailable.
Therefore the array is a tensor. We have a quantity such that is a tensor for every vector field . That is the hypothesis of the quotient theorem of Chapter 2.4 §5.1, and its conclusion is that is itself a tensor, of type . The same thing can be said in the language of Chapter 3.2's Problem 3. The map is function-linear, meaning that if you multiply by any function the answer is multiplied by , with no leftover term in . Function-linearity is exactly what distinguishes a tensor from a differential operator.
Four separately non-tensorial objects have been combined so that all their bad behaviour cancels. The four are in two orderings and in two orderings. This is the second time the book has done this, and the first time was a rehearsal. Chapter 3.2 §8 found that is not a tensor while the antisymmetric combination is, and its recap said explicitly that the trick would recur "much more consequentially, in Chapter 3.4". This is that recurrence.
The mechanism is the same both times. The offending piece of the transformation law is symmetric in the two indices being antisymmetrised, so antisymmetrising annihilates it. For the connection that offending piece carries , which is symmetric by Clairaut. Curvature is what is left of the connection after the part that depends on the chart has been subtracted away.
3.1 · A concrete demonstration: the flat plane in polar coordinates
Argument by quotient theorem is airtight and slightly bloodless. Here is the cancellation happening in a case where every number is known. Chapter 3.3 §7.8 found that the flat plane in polar coordinates has
and Chapter 3.3 §9's second worked example showed that every one of those numbers is the inhomogeneous term of the transformation law, since the connection vanishes in the Cartesian chart. So this connection is entirely made of the part that is not tensorial. If §3's claim is right, the curvature must be exactly zero. Compute it.
Take , , , in (3.4.13) and write the four terms out:
Evaluate the four in turn, using (3.4.14). The first is . The second is zero, because . The third is zero, because both and vanish. The fourth has two values of : gives , and gives , entering with the minus sign in front. So
The derivative term and the quadratic term are equal and opposite. Do it once more with the other index assignment, , , , :
Again exactly. Every remaining component vanishes term by term for the same kind of reason, and the whole tensor is identically zero. (Confirmed by computer algebra: all sixteen components of for this metric are identically zero as functions of and .) A connection made entirely of chart-dependent junk produces exactly no curvature, which is what a tensor built to discard chart-dependent junk had better do.
Length in a derivation should buy something, and the long computation just finished bought this. The comparison coefficients of the last chapter were notoriously not honest measuring devices: a good choice of description makes them vanish everywhere and a bad one brings them back. Anything built naively from them inherits that disease. The array produced by the two-order calculation does not, because the two orders differ by an antisymmetry while the diseased part of the coefficients is symmetric in exactly the slots being antisymmetrised.
There is a short and airtight way to see it that avoids the algebra altogether. The thing computed was a difference of two honest objects, so it is honest. It turned out proportional to the carried field itself, with no derivatives of that field anywhere. Something that turns any field into an honest object by plain multiplication must itself be honest, and that is a theorem from the tensor chapter rather than a hopeful remark.
The flat page in circular labels makes the cancellation visible with actual numbers. There the coefficients are non-zero and consist of nothing but chart-dependent junk, since they vanish in square labels. Compute the new array from them and the derivative piece and the quadratic piece come out equal and opposite in every component, leaving zero. That is the third and final form of the previous chapter's warning, now a calculation rather than a promise.
4 · Geodesic deviation, and where Part III's thesis lands
Everything so far has been mathematics. This section is where it becomes physics, and it is the section the whole of Part III has been walking toward, so it goes slowly.
Chapter 3.1 §4 derived, from Newton alone, that two nearby freely falling particles accelerate relative to one another at a rate proportional to their separation and to the second derivatives of the gravitational potential. It then said, in §4.6: "Chapter 3.4 constructs exactly such an object … and Chapter 3.4 §4 will derive an equation of the form that is the tidal equation written covariantly. When the two are set side by side, the identification is unavoidable."
Here is that section. We take two neighbouring geodesics, derive how their separation evolves, and find the Riemann tensor sitting where Newton had the second derivatives of the potential.
4.1 · The setup, and one identity
Consider a one-parameter family of geodesics . For each fixed , the curve traced out as varies is a geodesic parametrised by its own proper time, and is the label saying which geodesic we are on. Two vector fields live naturally on the two-dimensional surface those curves sweep out, so define them both now:
Because and are coordinates on that surface, and are coordinate vector fields, and Chapter 3.2 §8.4 proved that coordinate vector fields commute:
One identity is needed before starting, and it is short. Compute the components of directly:
In the last term, relabel the two summed indices, exchanging the names and . That is free, since both are dummies. It becomes , and now use the symmetry of the connection in its lower indices to write . The last two terms of (3.4.20) are then identical and cancel. What remains is the Lie bracket of Chapter 3.2 (3.2.32), so
4.2 · The derivation, in four lines
We want the second derivative of the separation along the geodesic, which is what "relative acceleration" means. Write for the derivative along the curve.
Line 1. Apply twice and use (3.4.21) to swap the inner pair:
Line 2. What we want on the right is §2's commutator, so rewrite that expression as the opposite ordering plus the difference between the two orderings:
Line 3. The first term on the right is zero. That is the only place the geodesic property is used, and it is used exactly once: is the geodesic equation (3.3.57), so differentiating it in any direction still gives zero.
Line 4. Convert the remaining commutator of directional derivatives into the commutator of coordinate derivatives. Expanding with the Leibniz rule and subtracting the other ordering gives
and the first bracket vanishes by (3.4.21). Setting and using the definition (3.4.12) of the Riemann tensor:
Tidy the indices. Rearrange the factors, which are just numbers, and then use the antisymmetry of in its last two indices, , noted under (3.4.13). Renaming , , gives the standard form:
This is the equation of geodesic deviation. Read it before comparing it with anything. Take two particles, each moving as freely as it is possible to move, with no forces acting and no potentials anywhere, each following the straightest path available to it. They nevertheless accelerate relative to one another, and the rate is fixed by the curvature of the space they are in, linearly in their separation. In flat space , and neighbouring straight lines drift apart at a constant rate and no faster, which is what straight lines do.
In: a family of geodesics, the fact that coordinate vector fields commute, vanishing torsion (used once, in (3.4.21)), the geodesic equation (used once, in Line 3), and §2's commutator.
Out: the relative acceleration of two neighbouring free particles is minus the Riemann tensor contracted with two velocities and one separation.
Worth noticing: not one word of this derivation mentioned gravity, mass, or force. It is a statement about geodesics on any manifold with a metric.
4.3 · Setting it beside Newton
Now take (3.4.26) to the Newtonian limit, under exactly the three assumptions of Chapter 3.3 §8.3: slow motion, a static field, and a weak one.
Slow motion makes , since and the spatial components are smaller by . It also makes . The separation between two particles at the same coordinate time is purely spatial, .
Substituting into (3.4.26), the sums over and collapse to the single value and the sum over to spatial values:
And here is Chapter 3.1's equation (3.1.14), derived there from Newton's law of gravitation and one linearisation, with no relativity anywhere in it:
Put (3.4.27) and (3.4.28) side by side. They are the same equation. The separation vector plays the same role, the second time derivative plays the same role, and in the place where Newton has the matrix of second derivatives of the potential, general relativity has
4.4 · The identification, checked rather than assumed
Two equations having the same shape is suggestive, not conclusive. So compute directly from the weak-field metric and see whether (3.4.29) comes out. Everything needed is already derived: Chapter 3.1 §6.5 obtained from the accelerating cabin and the Doppler effect, using no general relativity, and Chapter 3.3 §8.3 turned that into
With that connection coefficient in hand we can compute the curvature component directly. Take (3.4.13), the definition from §2, and set , , and :
The second term vanishes because nothing depends on time. The two quadratic terms are products of two connection coefficients, each of which is first order in , so they are second order and are dropped at this accuracy. What survives is the first term, and by (3.4.30),
which is (3.4.29) exactly. (Confirmed symbolically for a general potential , all nine components at once.) The identification was not fitted to make the two equations match. It was computed, from a metric component that Chapter 3.1 obtained without using any of this machinery.
Chapter 3.1 established that the gravitational field can be deleted at any point by a change of coordinates, and that what cannot be deleted is the relative acceleration of two nearby freely falling bodies. It called that residue the entire physical content of gravity.
Equation (3.4.29) says what the residue is.
Tidal force is curvature, and curvature is what gravity is.
Not "is described by", not "is analogous to". The array of numbers you would measure by watching two neighbouring falling specks drift, and the array of numbers you compute by carrying a vector around an infinitesimal loop and asking how far it has turned, are the same array. The ocean going out twice a day and the failure of parallel transport to be path-independent are one phenomenon measured two ways.
4.5 · Three things that follow immediately
(i) The trace, and Laplace's equation. Contract (3.4.29) on and . On the left, the sum is nearly the Ricci tensor: by the definition stated in this chapter's conventions,
where vanishes because is antisymmetric in its last two indices and they are equal. Poisson's equation (Chapter 0.7 §7) then gives
Chapter 3.1 §4.4 promised that its tracelessness result "is the covariant descendant of ". Equation (3.4.34) is that descendant, and Chapter 3.6 will promote it to the full field equations.
(ii) The ellipse. Chapter 3.1 §4.5 said: "that shape is what a tidal field is, and Chapter 3.4 will recover this very ellipse from the curvature tensor." Worked example 2 below does exactly that, computing for a point mass and finding the eigenvalues that produce the stretch-and-squeeze.
(iii) The units are right. has dimensions , so has dimensions . Curvature is one over a length squared, which is what §1's also was. For the Earth's surface field, and dividing by gives a curvature of about : a radius of curvature of roughly metres, which is why nobody noticed.
Take two specks of dust released near each other, each moving as freely as anything can move, each following the straightest path its surroundings allow, with nothing pushing either. Ask how their separation changes. The answer, derived here from geometry alone with no mention of gravity or mass or force, is that the separation accelerates at a rate proportional to itself, the constant supplied by the array the previous sections built out of the circuit test.
Now set that beside a result obtained at the start of this part from Newton alone. Two specks in free fall were shown there to drift apart or together at a rate proportional to their separation, the constant supplied by how the pull varies with place. The two statements are one statement. Where the older physics wrote the way the pull varies, the new geometry writes the amount by which a direction fails to come home unchanged, and computing the second from the first confirms it rather than suggesting it.
So the thing you feel as gravity when the tide comes in, and the thing curvature measures, are one object. The ocean rising, two falling specks separating, and a direction coming back turned after a trip around a small loop are three descriptions of one feature of the world. That sentence is what this whole part has been walking toward, and everything after it is bookkeeping by comparison.
5 · The symmetries, and how many numbers there really are
The array has components in four dimensions. Almost all of them are redundant. This section derives the symmetries, then counts.
5.1 · The four symmetries, derived
Work with the fully lowered version , which is legitimate and unambiguous by Chapter 3.3's Problem 2.
(S1) Antisymmetry in the last pair: . Immediate from (3.4.13), as noted there: exchanging and exchanges the first two terms and the last two, flipping the overall sign. Lowering an index does not touch .
(S2) Antisymmetry in the first pair: . This one needs an argument, and the argument is pretty. We get at it by first extending the commutator to covectors. For any covector and vector , the contraction is a scalar, and annihilates scalars, which is Chapter 3.3 (3.3.40) with vanishing torsion. Apply Leibniz to that vanishing expression:
We want to strip off both terms, so relabel the summed indices in the second one, exchanging and , and both terms then carry . Since is arbitrary, the coefficients must match:
Iterating Leibniz once more gives the rule for a tensor: one such term per lower index,
Now put . The left side is zero, because identically and so is any further derivative of it. The right side becomes, on lowering,
which is (S2). So metric compatibility, the very demand that fixed the connection in Chapter 3.3, is what makes the curvature antisymmetric in its first pair.
(S3) The first Bianchi identity: . Cyclic in the last three indices. Derive it directly from (3.4.13). Write the three terms out with the upper index kept:
Add the three lines and go through the six derivative terms first. Take from the first line and from the third: the two connections have their lower indices in opposite orders, and Chapter 3.3's Demand 2 says the order does not matter, so the pair cancels. The same argument pairs from the first line with from the second, and from the second with from the third. All six derivative terms are gone, in three pairs.
Now the six quadratic terms, by exactly the same mechanism. Pair from the first line with from the third: identical after using the symmetry of , so they cancel. Pair with , and with . All six vanish. The cyclic sum is zero, and every single cancellation used the same one fact, that the connection is symmetric in its lower indices.
(S4) Pair exchange: . This is a consequence of the first three rather than an independent fact, and the proof is a four-line combinatorial manoeuvre with no new ingredient in it. It sits in the grind box, and the conclusion is what we use.
Grind box — pair exchange from (S1), (S2) and (S3)
Write the first Bianchi identity four times, each time cycling the last three indices of a different starting arrangement. Abbreviate the four indices as .
Form the combination (i) − (ii) − (iii) + (iv). Each of the four is separately zero, so the combination is zero. Now sort its twelve terms into two groups, using only (S1) and (S2) to move indices about. The first Bianchi identity is not used again from here.
Group one: four terms that cancel in pairs.
- from (i) against from (iii). Apply (S2) to the first, , and then (S1) to the last pair, . The two terms are equal and oppositely signed, so they cancel.
- from (i) against from (iv). Here (S2) alone gives , so the sum is zero.
- from (ii) against from (iii). Again (S2): , so the two add to zero.
- from (ii) against from (iv). Apply (S2), , then (S1) on the last pair, . Equal and oppositely signed, so they cancel.
Group two: four terms that double up.
- from (i) and from (ii). By (S2), , so together they give .
- from (iii) and from (iv). By (S2), , so together they give .
Everything has now been accounted for, and what the vanishing combination says is
Notice that the three inputs were used in different places: the first Bianchi identity supplied the four vanishing sums, and the two antisymmetries did all the rearranging. That is why (S4) is a consequence rather than an independent assumption.
Numerical confirmation of the algebra. Taking a random four-index array with (S1) and (S2) imposed and nothing else, the combination (i) − (ii) − (iii) + (iv) was evaluated for all index assignments and compared with . The two agreed to . So the rearrangement above is an identity in (S1) and (S2) alone, exactly as claimed.
Numerical confirmation. A deliberately generic four-dimensional metric was used, one with no symmetry at all, with off-diagonal entries and all four coordinates appearing. The Riemann tensor was computed from (3.4.13) and all four identities checked at a generic point. The largest violation of any of them was against components of size , which is round-off.
5.2 · The count, derived
Now count, in dimensions, and then set . The argument has three stages and each is a sentence.
Stage 1. Treat the index pairs as single labels. By (S1) and (S2), is antisymmetric within and within . An antisymmetric pair of indices in dimensions takes
independent values, which is Chapter 2.4 §7.2's count of an antisymmetric array. In four dimensions . So may be regarded as an array , which is numbers in four dimensions rather than .
Stage 2. Pair exchange makes that array symmetric. By (S4), where and are the pair labels. A symmetric array has independent entries, which for is .
Stage 3. The first Bianchi identity removes exactly one more. Here is the step that has to be done carefully, because most of the cyclic identity is already implied by the other symmetries. The claim is that, given (S1), (S2) and (S4), the cyclic identity (S3) is equivalent to the single statement
the vanishing of the completely antisymmetric part. The reason is that the cyclic sum , once the pair symmetries are imposed, is itself totally antisymmetric in all four indices, and any totally antisymmetric four-index array in dimensions has
independent components, again by Chapter 2.4 §7.2. In four dimensions that count is . There is exactly one totally antisymmetric four-index array up to scale, namely the Levi-Civita symbol of Chapter 2.4 §8.1, so (S3) imposes precisely one further condition.
The answer.
The boxed expression is what that difference collapses to once the binomials are written out and simplified. Now put in the number of dimensions we actually live in:
independent components, or directly, .
| independent | |||||
|---|---|---|---|---|---|
| 2 | 1 | 1 | 0 | 1 | 1 |
| 3 | 3 | 6 | 0 | 6 | 6 |
| 4 | 6 | 21 | 1 | 20 | 20 |
| 5 | 10 | 55 | 5 | 50 | 50 |
| 6 | 15 | 120 | 15 | 105 | 105 |
In two dimensions there is a single curvature number at each point, which is why §1's sphere had one answer and why surfaces are so much easier than spacetimes. The whole table was confirmed independently. The four symmetry conditions were written down as linear constraints on a general -component array and the rank of the resulting system computed, and the number of free components came out exactly.
5.3 · The same twenty, counted a completely different way
A number derived once is a number. Derived twice by independent routes, it is a fact. Here is the second route, which also settles two words that will be used together for the rest of Part III. A local inertial frame is a region small enough that gravity has no detectable effect across it. The locally inertial coordinates are the particular coordinates, constructed below, that are adapted to such a region. The frame is the physical situation, and the coordinates are the bookkeeping. Both will be needed again in §7.
At any point one can choose coordinates in which
and therefore . One cannot in general also arrange .
Both halves are constructions rather than assertions.
Getting at . is a real symmetric non-degenerate matrix, so by the spectral theorem (Chapter 0.5 §6) there is an orthogonal change of basis diagonalising it, and rescaling each basis vector by the square root of the modulus of its eigenvalue turns the diagonal entries into . The signature fixes the pattern to . That is a linear change of coordinates, so it is a legitimate chart change.
Getting at . Put at the origin and define new coordinates
Two facts about that substitution matter. At the origin , so the linear part is untouched and is still . And everywhere. Feed those two into Chapter 3.3's transformation law (3.3.26). At every Jacobian is a Kronecker delta, so the law collapses to
This is precisely why had to be a non-tensor: a tensor vanishing in one chart vanishes in all, and no such construction would be possible. And follows at once, since metric compatibility reads and the right side is zero at .
Why the second derivatives cannot all be removed, and where the count comes from. Push the construction to the next order, with a cubic term whose coefficients are symmetric in the three lower indices. Then count what is available against what is demanded, in four dimensions:
- Available. A symmetric triple of indices from four values takes values, and takes , so has free numbers.
- Demanded. Setting is one condition for each symmetric pair (10 values) and each symmetric pair (10 values), so conditions.
Eighty knobs, one hundred demands. Twenty combinations of second derivatives of the metric survive every possible change of coordinates. That is the same twenty as before, arrived at with no mention of Bianchi identities or antisymmetric pairs. It also says what the twenty are. They are the irreducible second-derivative content of the metric, the part no observer can transform away.
The same counting at the two lower orders is worth doing as well, because both answers are ones you have seen. The linear part has free numbers and is conditions, leaving . That is the dimension of the Lorentz group, three boosts and three rotations, exactly as Part II found. The quadratic part has numbers against 's conditions, matching exactly, which is why can always be removed and never more than that.
Chapter 3.1 §5 asked how big a freely falling laboratory may be before tidal effects become detectable, and answered with an explicit bound. Section 5.3 is the same statement made exact. Coordinates exist in which, at one event, the metric is Minkowski's and its first derivatives vanish. Inside such a frame, to first order, physics is the physics of Part II and there is no gravity at all. What cannot be removed is the second derivatives, twenty of them, and §4 identified those with the tidal field. The size of the laboratory is set by how far you can go before the second-order terms matter, which is Chapter 3.1's bound, now with a name for the obstruction.
An array with four slots in four dimensions carries two hundred and fifty-six numbers, almost all duplicates. Three properties cut the list down, and each is derived rather than declared. Swapping the last two slots flips the sign, which was built into the construction. Swapping the first two also flips the sign, and that traces back to the demand that carrying a direction preserves its length. A third relation ties together the three ways of cycling the last three slots.
Counting then goes in three stages. A pair of slots that flips sign under exchange behaves like a single label taking six values, so the array is a six-by-six table. A further symmetry makes that table symmetric. The cyclic relation removes one entry more, since what it says is that the completely antisymmetric part vanishes, and in four dimensions there is only one such part. Twenty survive.
The same twenty appear again by a route with nothing in common with the first. Ask how much of the geometry a well-chosen observer can make disappear near a chosen event. The rule for measuring distances can be made to look flat there, and its rate of change made to vanish, both by explicit construction. The rates of change of those rates cannot: the knobs fall short by exactly twenty. Those twenty are what no viewpoint removes, which is what the first chapter said about the tide.
6 · Ricci, the scalar, and what contraction throws away
Twenty numbers per point is a lot to carry into a field equation. Contracting reduces them, and the question is which contraction and at what cost.
6.1 · There is essentially only one contraction
A tensor can be contracted by summing its upper index against any one of its three lower ones. Take them in turn.
Against the first lower index. . The array is antisymmetric in by (S2) and is symmetric, and contracting a symmetric array with an antisymmetric one over both indices gives zero. That is Chapter 2.4 §7's standard argument, since relabelling the two summed indices reproduces the expression with the opposite sign. So this contraction vanishes identically.
Against the third lower index. by (S1), which is minus the remaining case.
Against the second lower index. This is the only one that is both non-zero and not a duplicate:
That object is the Ricci tensor. Its sign is a convention, and this book's is stated in the opening callout.
It is symmetric. Lower the contracted index and use pair exchange:
where the third step relabelled the two summed indices and used the symmetry of . So Ricci has independent components in four dimensions, not .
Contracting once more, with the inverse metric, gives a single number at each point:
the Ricci scalar or scalar curvature. Being a scalar, it is the same number for every observer, which makes it the simplest honest statement about curvature available anywhere.
6.2 · What was discarded
Riemann has components and Ricci has . So contraction throws away exactly components of information in four dimensions. That leftover has a name.
The part of the Riemann tensor not determined by the Ricci tensor is the Weyl tensor : the piece with all its traces removed. In four dimensions it carries the components contraction discards. ⚑ We quote three of its properties and use none of them: it has the same symmetries as Riemann, every contraction of it vanishes, and in the mixed form it is unchanged when the metric is multiplied by an arbitrary positive function of position, so it records the shape of the light cones and not the scale of anything. Chapter 7.3 meets that last property again under the name conformal invariance.
Two consequences of the counting are worth having now. In three dimensions Riemann has components and so does Ricci, so the Weyl tensor vanishes identically and Ricci determines the whole curvature. That is why gravity in three dimensions has no propagating waves. In two dimensions there is one component altogether, and it must be proportional to . Problem 1 works out the constant.
6.3 · Why this matters immediately: vacuum is not flat
Here is the reason the discarded part cannot be dismissed. Section 4.5 derived , so outside a mass, where , the Ricci tensor has a vanishing component, and Chapter 3.6 will show the whole of it vanishes there. Yet the tidal field outside a mass is emphatically not zero. Chapter 3.1 computed it, and §4 identified it with , which by (3.4.29) is and is non-zero at every point outside the body.
Both statements hold because Chapter 3.1 §4.4's tidal matrix is traceless in vacuum and non-zero. The trace is the Ricci part, and the traceless remainder is the Weyl part. So:
Ricci flat is not flat. If it were, there would be no gravity outside any body, no orbits, no tides and no gravitational waves. The whole of Chapter 3.7 lives in a region where and the curvature is what makes Mercury precess.
Twenty numbers at every point is more than a field equation can carry, and there is a standard way of boiling an array down: sum one slot against another. Doing it here is more constrained than it looks, since two of the three summations give either nothing or a copy of the third, for reasons traceable to the antisymmetries. So there is one way, and it gives a symmetric array of ten numbers, which boils once more into a single number everybody agrees on.
The array has fallen apart into independent pieces again, as the toolkit kept promising it would, and the pieces are not equally interesting. Ten numbers went into the pot and ten did not, and the ones left out have every trace removed. They carry the effects surviving where there is no matter, so the omission matters. Outside any body the summed-down array vanishes while the full array does not, and that gap is where orbits, tides and gravitational waves live.
That distinction was visible long before the machinery existed. The first chapter of this part found that a small ball of falling dust changes shape while holding its volume, and identified the volume statement with the law of gravity in empty space. The volume part is what gets summed down; the shape-changing part survives the summation. Empty space is gravitationally empty in the first sense and thoroughly occupied in the second.
7 · The second Bianchi identity, and a tensor with no divergence
This section is short and its result is the most consequential single line in the chapter, so its importance is flagged in advance.
Chapter 2.6 built the energy–momentum tensor and proved it satisfies , which is the local conservation of energy and momentum. On a curved manifold that becomes .
Any field equation of the form (geometry) (constant) therefore requires the geometrical side to have vanishing divergence as an identity, true for every metric whatever, not merely on shell. Otherwise the equation would impose an extra condition on matter that nothing justifies.
This section produces the unique combination of and with that property. Chapter 3.6 does not get to choose the left-hand side of Einstein's equations. This section chooses it.
7.1 · The identity
The identity we are after says something about how the curvature varies from point to point. Here is the claim:
cyclic in the three lower indices , which are the derivative index and the antisymmetric pair together. The proof uses §5.3's locally inertial coordinates and is four lines.
Line 1. Fix a point and adopt coordinates with , which §5.3 constructed. At , and only at , the definition (3.4.13) loses its quadratic terms:
Line 2. The covariant derivative of anything reduces to the ordinary derivative at , since every correction term carries a factor of . Note carefully what is not being claimed: is not zero at , only itself is, which is why (3.4.52) has content. Differentiating,
the derivatives of the quadratic terms also vanishing at because each is and every term carries an undifferentiated .
Line 3. Write the cyclic sum. Each of the three terms contributes two pieces, so there are six, and they cancel in pairs by Clairaut's theorem:
The first term of each line cancels the second term of the line below it. For instance, goes against , and those two are equal because mixed partials commute. The third line's second term goes against the first line's first term after the same move.
Line 4. Equation (3.4.51) is an equation between tensors, since every term in it is a covariant derivative of a tensor. It has just been shown true at in one particular chart. By Chapter 2.4 §6, a tensor equation true in one chart is true in every chart. And was arbitrary. Hence (3.4.51) holds everywhere, in every chart.
(Confirmed numerically: for the generic four-dimensional metric of §5.1's grind box, the largest value of the cyclic sum at a generic point was , against individual terms of size .)
7.2 · Contract it twice
Lower the first index of (3.4.51), which is legitimate because lets the metric pass through the derivative:
First contraction. Multiply by and sum. Take the three terms one at a time, saying what each contraction produces.
Term one: , by the definition (3.4.47). So it becomes .
Term two: the meets the derivative index, giving .
Term three: , which by (S1) is . So it becomes .
Second contraction. Multiply by and sum, again one term at a time.
Term one: , the Ricci scalar.
Term two: . Use (S2) to write , and then the contraction of the first and third indices is the Ricci tensor by (3.4.47), giving . So the term is .
Term three: .
The last step added the two identical terms. They are identical because and are both summed, and the name of a dummy index is private.
7.3 · The Einstein tensor
Our goal now is to write (3.4.57) as a single divergence, so that the whole content sits inside one . The metric passes through the derivative once more, so , and the equation reads . Define
This is the Einstein tensor, and three things about it are worth stating separately.
- It is symmetric, because both and are.
- It is built from the metric and its first two derivatives and nothing else.
- Its divergence vanishes identically, for every metric, as a consequence of (3.4.51) and not of any equation of motion.
(Confirmed numerically for the generic metric: all four components of came out below against derivatives of Ricci of size .)
Put the pieces together. Matter carries a symmetric tensor with . Geometry supplies exactly one symmetric tensor built from and its first two derivatives whose divergence vanishes identically, namely . As Chapter 3.6 will make precise, it also supplies itself, whose divergence vanishes because . So the most general equation of the permitted form is
for constants and . Chapter 3.6 fixes by demanding Newton's limit, quotes ⚑ Lovelock's theorem for the uniqueness, and discusses . The shape of the answer, however, was decided here, by one contracted identity.
Some results earn their place by what they forbid rather than by what they produce, and this is one of them. Differentiating the curvature array and adding up three cyclic arrangements gives exactly zero, always, for every geometry, as an identity rather than as a condition. Proving it is a matter of standing at a point in the frame where the comparison coefficients vanish, at which the curvature is a plain difference of derivatives, and watching six second derivatives cancel in pairs because the order of ordinary differentiation never matters.
Summing that identity down twice turns it into a statement about the boiled-down array: a particular combination of it and the single curvature number has no divergence whatever. Now recall what the previous part established about matter. Energy and momentum are packaged in one symmetric object whose divergence vanishes, and that vanishing is the local statement that nothing is created or destroyed.
Setting those two facts side by side almost writes the law of gravity by itself. If geometry is to be equated with matter, then whatever stands on the geometry side must have vanishing divergence automatically, for every geometry, or else the equation would quietly impose an extra demand on matter that nothing justifies. Exactly one combination qualifies, and three chapters from now it will be sitting on the left of the field equations, put there not by taste but by this identity.
8 · Flat if and only if the curvature vanishes
Chapter 3.3 §2 promised a genuine test and warned that neither varying metric components nor non-zero connection coefficients was one. Here is the test, in the form of a theorem with one easy half and one hard half.
The easy half, proved. Suppose there exist coordinates in which is constant, say equal to . Then everywhere in that chart. By the Christoffel formula (3.3.50), every therefore vanishes everywhere in that chart. By (3.4.13), every component of then vanishes in that chart too, each of the four terms being either a derivative of zero or a product containing zero. And is a tensor by §3, so a tensor vanishing in one chart vanishes in every chart (Chapter 2.4 §6). Hence in all charts.
Note what that argument settles. The flat plane in polar coordinates has non-constant metric components and non-zero connection coefficients, yet it must have zero curvature, because Cartesian coordinates exist for it. Section 3.1's explicit computation was the verification. This is the reason.
If throughout a region that is simply connected, then coordinates exist in which throughout. Simply connected means that every closed loop in the region can be shrunk to a point without leaving it. We quote this result and do not prove it.
The idea is visible from §1 even without the proof. Vanishing curvature makes parallel transport path-independent for loops that can be shrunk away, since the loop test is the integral of the curvature over any surface the loop bounds. Path-independence then lets one transport a chosen basis at one point to every other point unambiguously, producing a frame that is parallel everywhere. The work is in showing that this frame is the coordinate basis of an actual chart.
The topological caveat is not a technicality. Chapter 3.3's Problem 1 built a cone, whose curvature vanishes at every point away from the apex and which is nonetheless not a piece of the plane: a circle around the apex has circumference rather than . The region excluding the apex is not simply connected, loops encircling it cannot be shrunk, and the theorem does not apply. Chapter 3.9 meets the same distinction on cosmological scales, where a universe can be flat everywhere and still closed.
A question raised earlier and left hanging can now be settled. A space is genuinely flat, in the sense that one unbending grid covers all of it, exactly when the array built out of the circuit test vanishes everywhere. One direction is easy: lay down such a grid and the rule for distances has constant entries, so the comparison coefficients vanish and the array vanishes, and since the array is an honest measuring device its vanishing in one description means its vanishing in all.
The other direction is harder and is quoted rather than derived, with the reason for believing it sketched. If the array vanishes then carrying a direction around any circuit that can be shrunk away brings it back unchanged, so a direction chosen at one place can be carried unambiguously to every other place, which is the raw material a flat grid is made of.
One qualification in that sentence does real work rather than decorating the statement. Circuits that cannot be shrunk are exempt, and spaces containing them can be flat everywhere while refusing to be a plain grid. A cone rolled from paper is flat away from its tip, having been made without stretching anything, and yet a circle around the tip has the wrong circumference. Local information does not always add up to global information, and the last chapter of this part turns that on the universe.
9 · Worked examples
Compute the Riemann tensor, the Ricci tensor and the Ricci scalar of the sphere of radius from the Christoffel symbols of Chapter 3.3 §9, and check the result against §1's measured holonomy.
The one independent component. By §5.2 a two-dimensional space has exactly one, and by the symmetries it may be taken to be . From (3.4.13) with , , , :
Take the four terms in order, using (3.4.1).
The first: . Write , whose derivative is , so the term is .
The second: , so the term is zero.
The third: both and vanish, so the term is zero.
The fourth: the sum over keeps only , since . It gives .
Adding: . So
Lower the first index with :
Ricci and the scalar. By (3.4.47), , the term vanishing by antisymmetry in the last two indices. Similarly , which the same computation with the roles exchanged gives as . So
Positive, as promised in this chapter's sign convention. (All of the above was reproduced independently by computer algebra, including the full Riemann tensor.)
The check against §1. Problem 1 below shows that in two dimensions with , and that the holonomy of a small loop is times the area enclosed. Here , so the predicted holonomy is . That is (3.4.9), derived in §1 by integrating the transport equation and measured in the figure to six decimal places. Three routes, one number.
Chapter 3.1 §4.5 promised that "Chapter 3.4 will recover this very ellipse from the curvature tensor". Do so.
The components. By (3.4.32), in the weak static field, . Chapter 3.1 §4.3 computed that Hessian for a point mass, , in two lines of differentiation, obtaining
So the curvature components a falling observer measures are
The eigenvalues. Chapter 3.1's grind box diagonalised exactly this matrix: applying it to gives , and applying it to any vector perpendicular to leaves it alone. So the spectrum is times , whatever direction the mass lies in.
The motion. Feed that into the geodesic deviation equation in the form (3.4.27), . Along the eigenvalue is , so and the separation grows. Across it the eigenvalue is , so and the separation shrinks. Integrating twice from rest gives
which is Chapter 3.1 (3.1.24) character for character: the ring stretched along the field and squeezed across it, the ellipse in that chapter's figure.
What is new, and what is not. The numbers are the same numbers. What has changed is what they are components of. In Chapter 3.1 they were second derivatives of a potential, a quantity with no coordinate-independent meaning and no place in a relativistic theory. Here they are components of a tensor, and the tensor exists whether or not the field is weak, whether or not motion is slow, and whether or not any potential can be defined. The ellipse was always a picture of the curvature, and Chapter 3.1 drew it four chapters before there was a name for what it was drawing.
One number. At the Earth's surface, , so the largest curvature component is . Two objects released one metre apart vertically separate by an extra millimetre after about seconds. The effect is small. The identification is exact.
10 · Your turn
Problem 1 — curvature in two dimensions
(a) Using only (S1), (S2), (S4) and the fact that a two-dimensional space has one independent component, show that for some function . (b) Contract twice to show . (c) Verify on the sphere of radius and on the flat plane in polar coordinates. (d) Assuming the small-loop result of Problem 3, show that the holonomy of a small loop in two dimensions is times the enclosed area, and hence recover §1's answer.
Solution
(a) The right-hand side is the most general array with the required symmetries built from the metric alone: it is antisymmetric in , antisymmetric in , and symmetric under exchanging the pairs, as one checks by inspection. In two dimensions the space of arrays with those symmetries is one-dimensional by §5.2, and the displayed combination is a non-zero member of it, so every member is a multiple of it. The multiple may vary from point to point, hence a function .
(b) Contract with using : the first term gives and the second gives , so . Contract again with : . In that is , so .
(c) Sphere: from Worked example 1, so , constant, as a sphere should be. Checking the formula directly, ✓. Flat polar: §3.1 found every component zero, so and .
(d) By Problem 3 the change in a vector after a small loop of area in the plane spanned by two directions is contracted with the loop's area element. In two dimensions there is only one plane, and substituting the form from (a) gives a rotation by . Adding up over a large region gives , which on a sphere of radius is . That is equation (3.4.9), obtained from the tensor rather than from integrating along the path.
Problem 2 — a space that looks the same everywhere, and what §7 forces
Suppose in dimensions, with a function of position. (a) Compute , and . (b) Impose from §7 and deduce that for the function must be a constant. (c) Say why is exempt, and what that means for the sphere.
Solution
(a) From Problem 1(b), and . Hence
(b) Take the divergence. The metric passes through untouched, so
For the numerical factor is non-zero, so and is the same at every point. This is Schur's lemma, and it is a genuine consequence of §7 rather than an assumption: a space that looks the same in every direction at every point must have the same curvature at every point, and the reason is the contracted Bianchi identity.
(c) In the factor vanishes, so identically and no condition on follows. Two-dimensional surfaces may therefore have curvature that varies from place to place while still having the form of (a). An egg is one. The sphere's constancy is a fact about the sphere, not a theorem. This vanishing of in two dimensions is also why gravity has nothing to say in two dimensions, a point Chapter 7.2 will need.
Problem 3 — the loop test, from the commutator
Transport a vector around a small closed parallelogram whose sides are and . (a) Argue that the change in after the circuit is, to leading order, , using the fact that transporting along then differs from then by the commutator. (b) Check the scaling: the change is second order in the size of the loop, which is first order in its area. Why does that make "curvature per unit area" the right thing to measure? (c) Apply this to a small loop on the sphere near the equator, with sides along and , and confirm the answer agrees with §1.
Solution
(a) Parallel transport along a short displacement is, to first order, the operation acting on the components, so transporting along the four sides in order composes four such operations. Everything at first order cancels, because each side is traversed once in each direction. What survives at order is the commutator of the two transport operations, and §2 computed exactly that commutator: it is , the minus sign arising because transport is generated by while the derivative carries . The overall sign also depends on which way round the circuit is taken, and the antisymmetry of in is exactly what makes the answer reverse when the circuit is reversed, as it must.
(b) The change is proportional to , and the loop's area is also proportional to , while its perimeter is proportional to . So the ratio (change)/(area) approaches a finite non-zero limit as the loop shrinks, whereas (change)/(perimeter) goes to zero. Area is the right denominator, which is why §1's ratio was independent of the loop and why the figure's halve the loop button leaves it unmoved.
(c) Near the equator take and , with and . Using and its partners, the rotation angle works out to , and the area of the same little patch is . The ratio is , matching (3.4.9) and Worked example 1's .
Problem 4 — empty is not flat
(a) In four dimensions, how many components of the Riemann tensor are left undetermined by the statement ? (b) Using §4's weak-field results, show explicitly that outside a point mass while , and identify which of Chapter 3.1's results this is. (c) In how many dimensions would "empty implies flat" be true, and why?
Solution
(a) Riemann has and Ricci has . Setting Ricci to zero imposes conditions, so components remain free. They are the Weyl components of §6.2.
(b) By (3.4.33), , and for Chapter 3.1 §4.4 computed away from the origin. That was its equation (3.1.22), the tracelessness of the tidal matrix. Meanwhile Worked example 2 gives , whose eigenvalues are and are plainly non-zero. So the trace vanishes and the matrix does not. This is exactly Chapter 3.1 §4.4's observation that the tidal matrix of any vacuum region is traceless, seen from the other side.
(c) In three dimensions. There §6.2's counting gives Riemann components and Ricci , so Ricci determines the whole of Riemann and forces . Also trivially in two, where there is one component and it is . In four and above the Weyl part exists and the implication fails, which is the reason gravity in our world has vacuum solutions at all, and hence orbits, tides and waves.
You have a test for curvature that runs entirely from inside. Carry a vector around a closed loop, and the angle it comes back turned through, divided by the area enclosed, is a property of the place. On a sphere of radius that ratio is , derived in §1 by integrating the transport equation along three legs and measured in the figure to six decimals.
Shrinking the loop turns the test into the commutator of two covariant derivatives, and §2 computed it in full. Six terms appear and four of them cancel, and the four that cancel are exactly the ones containing derivatives of the transported vector. What is left is multiplication by the Riemann tensor (3.4.13), which is a genuine tensor even though every ingredient of it is not, because the chart-dependent part of the connection is symmetric in the two indices being antisymmetrised. The flat plane in polar coordinates demonstrates the cancellation with numbers.
The thesis of Part III, landed. Two neighbouring geodesics obey (3.4.26), and in the Newtonian limit that equation is Chapter 3.1's tidal equation with standing where stood. That identification was not fitted but computed, from a metric component Chapter 3.1 obtained with no general relativity at all. Tidal force is curvature, and curvature is what gravity is. Chapter 3.1's ellipse is a picture of , and Worked example 2 draws it again from the tensor.
The tensor has independent components in four dimensions, and we derived that twice, once from the symmetries and once by counting how much of the second derivatives of the metric no choice of coordinates can remove. Contraction gives the Ricci tensor and the Ricci scalar and discards ten components, the Weyl part, which is the part that survives in vacuum and carries the tides outside a mass. And the second Bianchi identity, contracted twice, produces identically.
Where this gets spent. That last identity is the reason Chapter 3.6's field equations look the way they do. The geometry side must be divergence-free for every metric, and is what qualifies. Chapter 3.5 builds the Lie derivative and Killing vectors, whose conserved quantities make Chapter 3.7 tractable. Chapter 3.7 solves outside a spherical mass and finds Mercury's precession and the bending of light, paying Chapter 3.1's factor of two. Chapter 3.9 takes vanishing curvature and non-trivial topology seriously. And in Part VI the commutator of two covariant derivatives is computed again with an internal space in place of the tangent space, at which point (3.4.13) becomes the Yang–Mills field strength and this chapter is read a second time in different clothes.