Affine map Created 2026-10-07 Updated 2026-10-14
An affine map combines a linear map with a translation. After choosing coordinate origins, it has the form , , where the matrix is its linear part of an affine map and is a fixed vector. Equivalently, it preserves every affine combination. [ref]
An original planar example is
It stretches horizontally, applies a shear mapping, and then translates. The vertices , and become , and . A square grid becomes a grid of parallelograms; straight edges and their weighted points still fit together.
Figure 1.
An affine map preserves straightness while changing lengths and angles
. An original triangle and finite window of a square grid, followed by their images under . The right-hand grid is the transformed left-hand grid. Equal axis scales make the altered lengths and angles visible. Details.
This map is not a linear map with respect to the displayed origins, because rather than zero. It also is not a Euclidean similarity: has length and has length , while the right angle at becomes . Its determinant is , so it doubles planar area. These metric changes explain why affine geometry studies straightness, incidence and weighted points rather than treating every transformation as an isometry.
The linear part is an invertible matrix, giving the concise inverse . More generally an affine map is bijective exactly when its linear part of an affine map is bijective. Between equal finite-dimensional spaces, this means an invertible matrix; the translation cannot repair a loss of rank of a linear map.
A smooth nondegenerate component of the fixed-point set of an isometry is a totally geodesic submanifold. If a geodesic starts tangent to the fixed component, its image under the isometry has identical position and tangent. Uniqueness of the geodesic equation makes the two geodesics coincide throughout their common domain, so the original geodesic stays in the fixed set.
The Möbius transformation fixes the antipodal pair under stereographic projection. But , so it multiplies infinitesimal spherical lengths at that fixed point by two, as follows from the round line element . It is not an isometry and hence not a sphere rotation. Fixing an antipodal pair is therefore necessary for a nontrivial rotational Möbius transformation, but is not sufficient.
If distinct points of a dynamical system on a compact metric space satisfy in one compatible metric, no compatible metric can make an isometry. On a compact space, all compatible metrics give the same asymptotic-pair property by uniform continuity, whereas an isometry preserves the strictly positive distance between distinct points. In a full shift, a constant sequence and a sequence differing at just one coordinate converge to each other under forward shifts, proving this obstruction directly in the product topology.
Banach–Stone theorem 2026-10-05
A surjective linear isometry between compact Hausdorff function spaces has the form , where is a homeomorphism and is continuous with modulus one. Thus the Banach space structure of determines up to homeomorphism.
Basis-copying isometry 2026-10-31
Relative to a fixed orthonormal basis, the displayed linear map is an isometry because its basis images are orthonormal. Its adjoint obeys . If vectors are described by coefficient functions, this adjoint maps to , where the product is pointwise. Although copies every basis quantum state, it does not copy arbitrary superpositions. For example it sends to , whereas two copies would also contain the cross terms and .
Bi-invariant group metric 2026-10-14
A group distance is bi-invariant when both left and right translations are isometries. Conjugation then fixes the identity element and is an isometry, so each metric ball there is invariant under every inner automorphism. A compatible bi-invariant group metric therefore requires arbitrarily small conjugation-invariant neighbourhoods. This concerns a distance function, not merely a bi-invariant Riemannian metric tensor.
A linear isometry between tangent spaces of complete simply connected Riemannian manifolds extends to a global isometry when parallel transport along corresponding broken geodesics identifies their Riemann curvature tensors. In particular, complete simply connected manifolds of the same dimension and constant sectional curvature are isometric: their curvature tensors are determined by that common constant and their Riemannian metrics. This is the constant-curvature form often called Cartan's theorem.
Cayley graph Created 2026-09-24 Updated 2026-10-14
A Cayley graph turns multiplication in a group into travel: the chosen generators of a group are the allowed one-step moves, and a word over an alphabet becomes a route. This lets us study a finitely generated group using graph distances, closed balls, and geodesics, rather than only equations between products.
Let be a group with a finite generating set of a group satisfying and . Such a symmetric subset of a group includes the inverse element of every allowed move. The Cayley graph has vertex set and joins to for each . We choose right multiplication for these moves. Reversing the move uses , so for graph distance we regard and as the two orientations of one undirected edge. An involution therefore gives one edge, not two parallel edges. Each edge has length one, regardless of its length in a drawing.[ref]
A sequence labels the walk
It ends at exactly when . Thus the Cayley graph is a connected graph precisely because generates , and its graph distance on vertices is the word metric. Left multiplication by sends the edge from to to the edge from to , preserving its generator label: this is a group action by graph automorphisms and isometries. Viewing groups as symmetries of geometric objects is the motivation of Clay and Margalit's introduction.[ref]
The useful geometric object includes its allowed moves, not just its drawing. Cayley graphs of the integers show how changing the moves adds shortcuts; word metric balls in the integer lattice show how the same group can acquire visibly different closed balls. Meier's book develops this passage from group operations to graphs as its central motivation.[ref]
Cayley transform between the half-plane and disk Created 2026-10-03 Updated 2026-10-14
The Cayley transform gives a conformal bijection between an unbounded half-plane and the unit disc. Two conventions are useful. For the right half-plane, use
For the upper half-plane, use
Rotating the upper half-plane onto the right half-plane by explains the relationship . The factors of distinguish which half-plane is mapped onto the unit disc. [ref]
Figure 1.
The upper half-plane Cayley transform bends a rectangular grid into the unit disc while preserving angles at intersections
. Details.
In particular, , and . The whole positive imaginary axis becomes the real diameter: for . Horizontal grid lines become circles tangent to the unit circle at when completed by their endpoint at infinity; they are not hyperbolic geodesics.
On the Riemann sphere, maps the extended real line onto the unit circle:
Every finite real has ; the remaining point corresponds to infinity. The pole is outside the upper half-plane, and the pole of at is on the boundary of the unit disc. Neither pole obstructs the interior conformal bijection.
For a short verification, subtract the squared moduli:
These identities put each interior image in the required domain; solving gives the stated inverse function. Both maps are holomorphic, with , so the conformal bijection preserves Euclidean angles between tangent directions.
Euclidean distance is not preserved: and are one unit apart, whereas and are only one third of a unit apart. The striking feature is that does preserve length for the hyperbolic metrics of the Poincaré half-plane model and Poincaré disk model:
Consequently it is an isometry for these hyperbolic metrics, including their induced hyperbolic distances. For the same example, the corresponding hyperbolic geodesic segments have equal length:
Thus the Cayley transform lets us choose the most convenient picture: a straight boundary for calculations, or a bounded unit disc for visualization. It also transports automorphisms of the unit disk into upper half-plane automorphisms by function composition .
Character space of an Abelian L1 group algebra Created 2026-10-14 Updated 2026-10-31
For a locally compact Hausdorff Abelian group, each continuous unitary character defines an algebra character by . Conversely, if is a nonzero algebra character and , the ratio is independent of , continuous and multiplicative. Translation isometries bound all its integer powers, so its modulus is one. The convolution formula recovers . The Gelfand topology corresponds to the compact-open topology on the Pontryagin dual group; conjugating the characters gives the alternative Fourier sign convention.
For a connected complete Riemannian manifold of dimension and constant sectional curvature , its complete simply connected universal cover is the round sphere of radius . This is the constant-curvature case of Cartan-Ambrose-Hicks theorem. Thus the manifold is a quotient by a finite group of isometries acting freely. In even dimension, the determinant embeds this group in : every determinant-one orthogonal transformation in odd ambient dimension has eigenvalue one and therefore a fixed point. The only possible nonidentity element is the antipodal involution, giving Real projective space. In odd dimensions, free cyclic scalar actions on complex unit spheres instead produce lens spaces.
Two horocycles have a unique common orthogonal hyperbolic line when their ideal centres of horocycles differ: it is the line with those two ideal endpoints. If the centres agree, an isometry puts both horocycles on horizontal lines; every vertical hyperbolic line meets both orthogonally, so there are infinitely many. This classification remains valid for intersecting or tangent horocycles.
Conformal automorphism of the upper half-plane Created 2026-10-06 Updated 2026-10-14
Every conformal automorphism of the upper half-plane is a Möbius transformation with real coefficients and positive determinant, and conversely every such map is a conformal bijection of the upper half-plane to itself:
The real-coefficient and sign conditions matter. The complex Möbius transformation sends to on the boundary, while the real Möbius transformation has negative determinant and sends to in the lower half-plane. [ref]
For two concrete upper half-plane automorphisms, take
Both matrices have determinant one. Here , , and . On the extended real line, fixes infinity and exchanges zero and infinity. On the unit disc, the same maps become and ; the second is simply .
Multiplying all four coefficients by a nonzero real scalar leaves unchanged. Dividing them by normalizes the determinant to one; the two remaining representatives and give the same map. Thus the group under function composition is the projective special linear group
where is the real special linear group of degree two. Composition of the Möbius transformations corresponds to multiplication of their matrices. [ref]
On the boundary,
So preserves the cyclic boundary orientation of the extended real line; when , its pole at prevents treating it as a single increasing function across that point on the ordinary real line. Three distinct boundary images determine a Möbius transformation uniquely, but an upper half-plane automorphism can realize only triples with matching cyclic boundary orientation.
A brief proof outline starts with the identities
They show that and its inverse function preserve the upper half-plane. For completeness of the classification, conjugate an arbitrary conformal bijection by the Cayley transform. Normalize its image of zero with an automorphism of the unit disk, then apply the Schwarz lemma to the resulting map and its inverse function; both inequalities force a rotation. Conjugating back gives the real Möbius transformation above.
Finally, and the displayed imaginary part identity show that . Every upper half-plane automorphism is therefore also an isometry of the Poincaré half-plane model. The same formulas describe both holomorphic coordinate symmetries and motions of the hyperbolic plane.
C-star homomorphism Created 2026-10-05 Updated 2026-10-06
A C-star homomorphism is a complex linear multiplicative map between C-star algebras that preserves the involution. Such maps are contractive; an injective one is an isometry.
For a finite isometric group action on a closed Riemannian surface, choose a disk in the free locus whose translates are disjoint. Modify the Riemannian metric there, and identically on its translates, by small supported changes with three distinguished high Gaussian curvature maxima. Give their heights distinct values occurring nowhere else, arrange them as a tight noncollinear cluster, and keep separate clusters far apart. Such markers can be made by local conformal bump functions controlling curvature and its derivatives. Every quotient isometry must send an entire labelled cluster to another. After identifying the marked disks with the original one, an isometry fixes its three noncollinear points and is therefore the identity locally. If are free finite quotients, any quotient isometry consequently makes on an open disk for some element of the original group. Two local isometries agreeing on an open set agree on the connected surface, by propagation along geodesics. The equality therefore holds globally and implies , hence equality for equal subgroup orders. Nonconjugate equal-order subgroups thus have nonisometric quotients for this marked invariant metric; constant curvature is not required.
If two simple base geodesics meet once, their lift components correspond to the cycles of their monodromy permutations. A lifted crossing belongs to the sheet labels common to both cycles, giving the displayed geometric intersection count. When their relevant lifted lengths identify these components independently of the covering map, different multisets of intersection counts obstruct an isometry between the covering surfaces.
Cyclic transitive point set Created 2026-09-24 Updated 2026-09-24
A finite point set is cyclic transitive when a cyclic group of isometries acts transitively on it.
Decay of autocorrelation implies weak convergence of an observable Created 2026-10-05 Updated 2026-10-06
For a probability measure-preserving system, if , then converges weakly in to . Centre ; its autocorrelations tend to zero. The isometry identity gives the same decay against each , hence by approximation against their closed forward span. Against its orthogonal complement the correlations are exactly zero. Orthogonal decomposition by a closed subspace finishes the proof without invertibility.
Diffeomorphism invariance of general relativity Created 2026-10-06 Updated 2026-10-07
Transforming a metric tensor and all matter fields together by the pullback of a diffeomorphism preserves the Einstein field equations and covariant matter equations. Passive coordinate changes only change the description of the fields; active pullbacks produce another representative of the geometry. The treatment of transformations acting on a boundary depends on the boundary conditions and possible charges. A diffeomorphism is not necessarily an isometry of a fixed metric.