Book 10A

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Course 10Book 10A: Three-Manifolds and GeometrizationChapter 1

A Zoo of Three-Manifolds

The 3-sphere, lens spaces, the Poincaré sphere, the Hopf fibration and the shape of space.

17 min read · Updated Oct 3, 2026

Read with Thurston's Three-Dimensional Geometry and Topology, Volume 1, chapter 1 (what is a manifold? gluing polyhedra, the 3-torus and the dodecahedral spaces), and Weeks's The Shape of Space for an accurate popular account. Hatcher's Notes on Basic 3-Manifold Topology is the reference for the rest of this book.

In this chapter · 6 sections
  1. 1.1The shape of space
  2. 1.2The 3-sphere and the Hopf fibration
  3. 1.3Flat, product and quotient examples
  4. 1.4Dodecahedral spaces
  5. 1.5History
  6. 1.6Exercises

Book 7A stated the Poincaré conjecture: a closed, simply connected 3-manifold is the 3-sphere. Book 10A asks the broader question that Thurston's geometrization conjecture answers: what are all the closed 3-manifolds, and what do they look like? The Ricci flow with surgery is a machine that takes any closed 3-manifold and returns pieces. This book describes the pieces, how they fit together and the geometries they carry, so that when the machine runs in Books 11A–12C you know what it must produce.

This first chapter is a zoo: the 3-sphere and its Hopf fibration, the 3-torus, S2×S1S^2\times S^1, lens spaces and the other spherical space forms, the Poincaré homology sphere in three guises, and the Seifert–Weber space. Each will reappear as an example of a piece, a geometry or a fate under the flow.

By the end of this chapter you will be able to:

  • describe S3S^3 as the unit quaternions and as two solid tori, and compute the fibres of the Hopf fibration;
  • build the 3-torus, RP3\mathbb{RP}^3 and the lens spaces as quotients, and compute their fundamental groups;
  • state which groups act freely on S3S^3, and recognise spherical space forms;
  • construct the Poincaré homology sphere and the Seifert–Weber space by gluing the faces of a dodecahedron;
  • explain how one could test whether the universe is a nontrivial 3-manifold.

The shape of space

In the world Data Which 3-manifold do we live in?

On large scales, space is close to flat (9A.6 The Laplacian and the Bochner Formula), but flatness does not decide topology: a flat universe could be infinite R3\mathbb{R}^3, or a finite 3-torus, or one of the other closed flat 3-manifolds (10A.5 Thurston’s Eight Geometries). If space were finite and smaller than the distance light has travelled since recombination, light from the same region would reach us from different directions. The sphere from which the cosmic microwave background was emitted would intersect its own translated copies, and the sky would contain pairs of matched circles with the same temperature pattern. Neil Cornish, David Spergel and Glenn Starkman proposed this test in 1998. In 2003 Jean-Pierre Luminet and colleagues suggested that a deficit of large-scale power in the WMAP data might be explained if space were the Poincaré dodecahedral space, a positively curved quotient of S3S^3.

Later searches did not find matched circles. The Planck collaboration ("Planck 2015 results XVIII: Background geometry and topology of the Universe", Astronomy & Astrophysics, 2016) found no evidence of nontrivial topology. For a cubic 3-torus, it showed that the largest ball fitting in the fundamental domain must have radius at least 0.970.97 of the distance to the last-scattering surface (99% confidence). If the universe is a nontrivial 3-manifold, it is too large for us to see its topology. Even so, this is a genuine experiment asking which closed 3-manifold we inhabit.

The 3-sphere and the Hopf fibration

The unit sphere S3={(z,w)∈C2:∣z∣2+∣w∣2=1}S^3 = \{(z, w) \in \mathbb{C}^2 : |z|^2 + |w|^2 = 1\} has several faces (7A.2 Compactness and Compactification, 8A.5 Lie Groups and Group Actions): the one-point compactification of R3\mathbb{R}^3, via stereographic projection; the group SU(2)SU(2) of unit quaternions; and the union of two solid tori {∣z∣≤∣w∣}\{|z| \leq |w|\} and {∣z∣≥∣w∣}\{|z| \geq |w|\} glued along the torus ∣z∣=∣w∣=12|z| = |w| = \frac{1}{\sqrt2}, with the meridian of each glued to the longitude of the other.

The Hopf fibration is the map

h:S3→S2⊂C×R,h(z,w)=(2zwˉ,∣z∣2−∣w∣2).h : S^3 \to S^2 \subset \mathbb{C}\times\mathbb{R}, \qquad h(z, w) = \big(2z\bar w, |z|^2 - |w|^2\big).

Its fibres are the circles {(eiθz,eiθw)}\{(e^{i\theta}z, e^{i\theta}w)\}: each is the intersection of S3S^3 with a complex line through the origin, hence a great circle (Exercise 1.1). So S3S^3 is a union of disjoint great circles, one for each point of S2S^2, and any two of them are linked once. Under stereographic projection to R3\mathbb{R}^3 the picture is famous (Figure 1.1): one fibre is a vertical line through infinity, one is the unit circle around it, and the rest fill nested tori, each torus made of circles that wind once around each way. The Berger spheres of 9A.5 Computing Curvature and 9B.3 Collapsing and Noncollapsing are S3S^3 with these circles shrunk.

Figure 1.1. Fibres of the Hopf fibration, stereographically projected from S3S^3 to R3\mathbb{R}^3 (computed). The fibres over the poles of S2S^2 are the vertical axis (through infinity) and the unit circle. The fibres over a circle of latitude lie on a torus; ten fibres on one such torus are shown, each a circle winding once around each way. Every pair of fibres is linked once.
In the world Model The Bloch sphere

In quantum computing, the state of a qubit is a unit vector (z,w)∈C2(z, w) \in \mathbb{C}^2, ∣z∣2+∣w∣2=1|z|^2 + |w|^2 = 1: a point of S3S^3. Two state vectors that differ by an overall phase eiθe^{i\theta} describe the same physical state, so the physical states form the quotient of S3S^3 by the circle action, which is S2S^2, the Bloch sphere. The map from state vectors to points of the Bloch sphere is exactly the Hopf map, and the fibres are the phase circles. The third coordinate ∣z∣2−∣w∣2|z|^2 - |w|^2 is the difference of the two measurement probabilities.

Flat, product and quotient examples

The 3-torus T3=R3/Z3T^3 = \mathbb{R}^3/\mathbb{Z}^3, a cube with opposite faces glued. It has a flat metric and π1=Z3\pi_1 = \mathbb{Z}^3. Someone living inside a small 3-torus would see copies of themselves repeated in a cubic lattice in every direction (Figure 1.2), which is what the matched-circles test looks for on a cosmic scale.

S2×S1S^2\times S^1, with π1=Z\pi_1 = \mathbb{Z}. It is the prime manifold that is not irreducible (10A.3 The Prime Decomposition): the sphere S2×{∗}S^2\times\{\ast\} does not bound a ball. Its product metric is the neck geometry S2×RS^2\times\mathbb{R} wrapped up.

Lens spaces. For coprime p>q≥1p > q \geq 1, the cyclic group generated by (z,w)↦(ζz,ζqw)(z, w) \mapsto (\zeta z, \zeta^qw), ζ=e2πi/p\zeta = e^{2\pi i/p}, acts freely on S3S^3 by isometries, and the quotient is the lens space L(p,q)L(p, q), with π1=Z/p\pi_1 = \mathbb{Z}/p (7A.6 Covering Spaces). L(2,1)=RP3L(2, 1) = \mathbb{RP}^3. Lens spaces are classified by Reidemeister's theorem (1935, extended from piecewise-linear equivalence to homeomorphism by Brody in 1960): L(p,q)L(p, q) and L(p,q′)L(p, q') are homeomorphic if and only if q′≡±q±1(modp)q' \equiv \pm q^{\pm1} \pmod p. Homotopy equivalence is weaker, qq′≡±n2(modp)qq' \equiv \pm n^2 \pmod p for some nn, so L(7,1)L(7, 1) and L(7,2)L(7, 2) are homotopy equivalent but not homeomorphic (Exercise 1.3): the fundamental group, even with homotopy type, does not determine a 3-manifold in general. The Poincaré conjecture is the claim that it does when the group is trivial.

Spherical space forms. More generally, a spherical space form is a quotient S3/ΓS^3/\Gamma by a finite group Γ⊂SO(4)\Gamma \subset SO(4) acting freely. The possible groups were classified by Hopf (1926) and later work: cyclic groups, as for lens spaces, and products of cyclic groups with the binary dihedral, binary tetrahedral, binary octahedral and binary icosahedral groups (the preimages in SU(2)SU(2) of the rotation groups of regular solids), in suitable combinations. These are exactly the closed 3-manifolds with a metric of constant positive curvature (10A.5 Thurston’s Eight Geometries).

Mapping tori and knot complements. Gluing the ends of Σ×[0,1]\Sigma\times[0, 1] by a diffeomorphism ϕ\phi of a surface gives the mapping torus of ϕ\phi, a 3-manifold fibring over the circle. Removing an open tubular neighbourhood of a knot in S3S^3 gives a knot complement, a compact 3-manifold with torus boundary; the trefoil and figure-eight complements are the first examples of 10A.4 Seifert Spaces and the JSJ Decomposition and 10A.6 Hyperbolic Three-Manifolds.

Figure 1.2. A two-dimensional slice of the idea. Left: a flat torus, a square with opposite sides glued, containing one object. Right: what an inhabitant sees. Light leaving the object wraps around, so it appears repeated in a square lattice, as in the universal cover R2\mathbb{R}^2. In a 3-torus the copies form a cubic lattice; on the cosmic scale they would produce the matched circles.

Dodecahedral spaces

Take a solid regular dodecahedron and glue each face to the opposite face. A face is a pentagon, and the opposite face is rotated relative to it, so a twist is needed.

  • Gluing with a 110\frac{1}{10} turn (36°36°) gives the Poincaré homology sphere, also described as S3/I∗S^3/I^*, the quotient by the binary icosahedral group of order 120120 (7A.6 Covering Spaces), and as the link of the singularity x2+y3+z5=0x^2 + y^3 + z^5 = 0 (the Brieskorn sphere Σ(2,3,5)\Sigma(2, 3, 5)). Its fundamental group is perfect and nontrivial, so it has the homology of S3S^3 but is not S3S^3: the example that made Poincaré state his conjecture with π1\pi_1 instead of homology.
  • Gluing with a 310\frac{3}{10} turn (108°108°) gives the Seifert–Weber space (Weber and Seifert, 1933), which carries a hyperbolic metric.

The edges of the dodecahedron fall into classes under the gluing, and the angles around each glued edge must add up to 2π2\pi. In the Poincaré gluing the edges come in classes of 33, so the dihedral angle must be 120°120°, slightly more than the Euclidean 116.57°116.57°: the dodecahedron must be spherical, one of the 120120 cells of the regular 120-cell in S3S^3. In the Seifert–Weber gluing they come in classes of 55, so the angle must be 72°72°: the dodecahedron must be hyperbolic (Exercise 1.4). The gluing determines the geometry. This is the first glimpse of geometrization.

Where this goes The zoo, sorted

10A.2 Building Three-Manifolds shows how all closed 3-manifolds can be built (Heegaard splittings, surgery). 10A.3 The Prime Decomposition and 10A.4 Seifert Spaces and the JSJ Decomposition cut them along spheres and tori into pieces. 10A.5 Thurston’s Eight Geometries lists the eight geometries the pieces carry: S3S^3 and its quotients, E3\mathbb{E}^3 (the 3-torus), S2×RS^2\times\mathbb{R}, and five more, including hyperbolic geometry (the Seifert–Weber space) and Nil (circle bundles over tori). 10A.7 Geometrization and Ricci Flow says what the Ricci flow does to each.

History

Heinz Hopf introduced his fibration in 1931. Heinrich Tietze defined lens spaces in 1908; Kurt Reidemeister classified them in 1935. Poincaré constructed his homology sphere in 1904; its dodecahedral description is due to Weber and Seifert (1933), as is the hyperbolic space with the 310\frac{3}{10} twist. Cornish, Spergel and Starkman proposed the circles-in-the-sky test in 1998; the Planck collaboration's topology analysis appeared in 2014 and 2016.

Recall Where we stand

S3S^3 is the unit quaternions, the compactified R3\mathbb{R}^3, or two solid tori; the Hopf fibration fills it with linked great circles, one for each point of S2S^2, and it is the map from qubit states to the Bloch sphere. The 3-torus is flat with π1=Z3\pi_1 = \mathbb{Z}^3; S2×S1S^2\times S^1 has π1=Z\pi_1 = \mathbb{Z}; lens spaces L(p,q)L(p, q) are quotients of S3S^3 with π1=Z/p\pi_1 = \mathbb{Z}/p, classified by q′≡±q±1q' \equiv \pm q^{\pm1}; spherical space forms are S3S^3 modulo finite groups acting freely. Gluing a dodecahedron's opposite faces with a 110\frac{1}{10} turn gives the Poincaré homology sphere (spherical), with a 310\frac{3}{10} turn the Seifert–Weber space (hyperbolic). Matched-circle searches test whether the universe is such a manifold, and have found none at observable scales. 10A.2 Building Three-Manifolds builds every closed 3-manifold from simple pieces.

Exercises

Exercise 1.1 Hopf fibres

(a) Show that h(z,w)=(2zwˉ,∣z∣2−∣w∣2)h(z, w) = (2z\bar w, |z|^2 - |w|^2) maps S3S^3 to the unit sphere in C×R\mathbb{C}\times\mathbb{R}, and that h(z,w)=h(z′,w′)h(z, w) = h(z', w') if and only if (z′,w′)=eiθ(z,w)(z', w') = e^{i\theta}(z, w). (b) Show that each fibre is a great circle. (c) The fibres over the poles (0,±1)(0, \pm1) are {w=0}\{w = 0\} and {z=0}\{z = 0\}; show that after stereographic projection from (0,i)∈S3(0, i) \in S^3 they become the unit circle in the horizontal plane and the vertical axis, which are linked.

Solution

(a) ∣2zwˉ∣2+(∣z∣2−∣w∣2)2=(∣z∣2+∣w∣2)2=1|2z\bar w|^2 + (|z|^2 - |w|^2)^2 = (|z|^2 + |w|^2)^2 = 1. If hh agrees, then ∣z∣=∣z′∣|z| = |z'|, ∣w∣=∣w′∣|w| = |w'| and zwˉ=z′wˉ′z\bar w = z'\bar w', which forces a common phase. (b) The fibre is S3∩{λ(z,w):λ∈C}S^3\cap\{\lambda(z, w) : \lambda \in \mathbb{C}\}, the unit circle of a real 2-plane. (c) Writing w=x3+ix4w = x_3 + ix_4 and projecting from x4=1x_4 = 1, {w=0}\{w = 0\} is the unit circle x12+x22=1x_1^2 + x_2^2 = 1 in x3=0x_3 = 0, and {z=0}\{z = 0\} is the circle x32+x42=1x_3^2 + x_4^2 = 1, which projects to the x3x_3-axis together with the point at infinity. The axis passes through the disc bounded by the unit circle once.

Exercise 1.2 Fundamental groups

Compute π1\pi_1 of T3T^3, S2×S1S^2\times S^1, L(p,q)L(p, q) and RP3\mathbb{RP}^3 from covering spaces (7A.6 Covering Spaces). Which of these are simply connected after passing to the universal cover, and what is the cover in each case?

Solution

T3=R3/Z3T^3 = \mathbb{R}^3/\mathbb{Z}^3: π1=Z3\pi_1 = \mathbb{Z}^3, cover R3\mathbb{R}^3. S2×S1S^2\times S^1: cover S2×RS^2\times\mathbb{R}, deck group Z\mathbb{Z}. L(p,q)=S3/(Z/p)L(p, q) = S^3/(\mathbb{Z}/p): π1=Z/p\pi_1 = \mathbb{Z}/p, cover S3S^3. RP3=L(2,1)\mathbb{RP}^3 = L(2, 1): Z/2\mathbb{Z}/2, cover S3S^3. All universal covers are simply connected; only S3S^3 is compact among R3\mathbb{R}^3, S2×RS^2\times\mathbb{R}, S3S^3.

Exercise 1.3 Lens spaces with the same group

Using Reidemeister's criterion, show that L(5,1)L(5, 1) and L(5,2)L(5, 2) are not homeomorphic, and that L(5,2)L(5, 2) and L(5,3)L(5, 3) are. Using the homotopy criterion qq′≡±n2(modp)qq' \equiv \pm n^2 \pmod p, show that L(7,1)L(7, 1) and L(7,2)L(7, 2) are homotopy equivalent.

Solution

For p=5p = 5: ±1±1={1,4}\pm1^{\pm1} = \{1, 4\}, which does not contain 22; and 3≡−23 \equiv -2, so L(5,2)≅L(5,3)L(5, 2) \cong L(5, 3). For p=7p = 7: 1⋅2=21\cdot2 = 2, and the squares mod 77 are 1,2,41, 2, 4, so 2=32 mod 72 = 3^2 \bmod 7; but ±1±1={1,6}∌2\pm1^{\pm1} = \{1, 6\} \not\ni 2, so they are not homeomorphic.

Exercise 1.4 Counting cells in the dodecahedral spaces

A dodecahedron has 2020 vertices, 3030 edges and 1212 faces. In the Poincaré gluing, the vertices fall into 55 classes of 44 and the edges into 1010 classes of 33; in the Seifert–Weber gluing, the vertices form 11 class and the edges 66 classes of 55. (a) Check that both have Euler characteristic 00, as every closed odd-dimensional manifold must. (b) The regular Euclidean dodecahedron has dihedral angle arccos⁡(−15)≈116.57°\arccos(-\frac{1}{\sqrt5}) \approx 116.57°. Explain why the Poincaré gluing needs a spherical dodecahedron and the Seifert–Weber gluing a hyperbolic one.

Solution

(a) Poincaré: 5−10+6−1=05 - 10 + 6 - 1 = 0. Seifert–Weber: 1−6+6−1=01 - 6 + 6 - 1 = 0. (b) Around a glued edge class the dihedral angles must sum to 2π2\pi: with 33 edges each angle is 120°120°, with 55 edges 72°72°. Spherical polyhedra have larger angles than Euclidean ones of the same shape and hyperbolic ones smaller, and the angle of a regular dodecahedron varies continuously with its size, from the Euclidean value at small size: up to 120°120° (and beyond) in S3S^3, down to 72°72° (and below) in H3\mathbb{H}^3.

Exercise 1.5 Rehearsal: the Hopf map as a Riemannian submersion

At the point (1,0)∈S3(1, 0) \in S^3, the fibre direction is (i,0)(i, 0) and the horizontal vectors are (0,v)(0, v), v∈Cv \in \mathbb{C}. Compute dh(1,0)(0,v)dh_{(1, 0)}(0, v) and show it has length 2∣v∣2|v|. Deduce that 12h\frac12h is a Riemannian submersion onto the sphere S2(12)S^2(\frac12) of radius 12\frac12 at this point (and, by symmetry, everywhere), which is why collapsing Berger spheres converge to S2(12)S^2(\frac12) (9B.3 Collapsing and Noncollapsing).

Solution

h(1,εv)=(2εvˉ,1−ε2∣v∣2)h(1, \varepsilon v) = (2\varepsilon\bar v, 1 - \varepsilon^2|v|^2) to first order, so dh(0,v)=(2vˉ,0)dh(0, v) = (2\bar v, 0), of length 2∣v∣2|v|; also dh(i,0)=0dh(i, 0) = 0, since hh is constant on fibres. So 12h\frac12h maps S3S^3 to S2(12)S^2(\frac12), kills the fibre direction, and is an isometry on horizontal vectors. U(2)U(2) acts transitively on S3S^3 preserving the fibration and the metrics, so the same holds at every point.

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