In geometry and complex analysis, a Möbius transformation of the complex plane is a rational function of the form
Geometrically, a Möbius transformation can be obtained by first applying the inverse stereographic projection from the plane to the unit sphere, moving and rotating the sphere to a new location and orientation in space, and then applying a stereographic projection to map from the sphere back to the plane.^{[1]} These transformations preserve angles, map every straight line to a line or circle, and map every circle to a line or circle.
The Möbius transformations are the projective transformations of the complex projective line. They form a group called the Möbius group, which is the projective linear group PGL(2, C). Together with its subgroups, it has numerous applications in mathematics and physics.
Möbius geometries and their transformations generalize this case to any number of dimensions over other fields.
Möbius transformations are named in honor of August Ferdinand Möbius; they are an example of homographies, linear fractional transformations, bilinear transformations, and spin transformations (in relativity theory).^{[2]}
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Möbius transformation

Conformal Mapping  Möbius Transformation  Complex Analysis #25

Mod05 Lec11 Möbius transformations (Part I)
Transcription
Overview
Möbius transformations are defined on the extended complex plane (i.e., the complex plane augmented by the point at infinity).
Stereographic projection identifies with a sphere, which is then called the Riemann sphere; alternatively, can be thought of as the complex projective line . The Möbius transformations are exactly the bijective conformal maps from the Riemann sphere to itself, i.e., the automorphisms of the Riemann sphere as a complex manifold; alternatively, they are the automorphisms of as an algebraic variety. Therefore, the set of all Möbius transformations forms a group under composition. This group is called the Möbius group, and is sometimes denoted .
The Möbius group is isomorphic to the group of orientationpreserving isometries of hyperbolic 3space and therefore plays an important role when studying hyperbolic 3manifolds.
In physics, the identity component of the Lorentz group acts on the celestial sphere in the same way that the Möbius group acts on the Riemann sphere. In fact, these two groups are isomorphic. An observer who accelerates to relativistic velocities will see the pattern of constellations as seen near the Earth continuously transform according to infinitesimal Möbius transformations. This observation is often taken as the starting point of twistor theory.
Certain subgroups of the Möbius group form the automorphism groups of the other simplyconnected Riemann surfaces (the complex plane and the hyperbolic plane). As such, Möbius transformations play an important role in the theory of Riemann surfaces. The fundamental group of every Riemann surface is a discrete subgroup of the Möbius group (see Fuchsian group and Kleinian group). A particularly important discrete subgroup of the Möbius group is the modular group; it is central to the theory of many fractals, modular forms, elliptic curves and Pellian equations.
Möbius transformations can be more generally defined in spaces of dimension n > 2 as the bijective conformal orientationpreserving maps from the nsphere to the nsphere. Such a transformation is the most general form of conformal mapping of a domain. According to Liouville's theorem a Möbius transformation can be expressed as a composition of translations, similarities, orthogonal transformations and inversions.
Definition
The general form of a Möbius transformation is given by
In case c ≠ 0, this definition is extended to the whole Riemann sphere by defining
If c = 0, we define
Thus a Möbius transformation is always a bijective holomorphic function from the Riemann sphere to the Riemann sphere.
The set of all Möbius transformations forms a group under composition. This group can be given the structure of a complex manifold in such a way that composition and inversion are holomorphic maps. The Möbius group is then a complex Lie group. The Möbius group is usually denoted as it is the automorphism group of the Riemann sphere.
If ad = bc, the rational function defined above is a constant (unless c = d = 0, when it is undefined):
Fixed points
Every nonidentity Möbius transformation has two fixed points on the Riemann sphere. The fixed points are counted here with multiplicity; the parabolic transformations are those where the fixed points coincide. Either or both of these fixed points may be the point at infinity.
Determining the fixed points
The fixed points of the transformation
When c = 0, the quadratic equation degenerates into a linear equation and the transform is linear. This corresponds to the situation that one of the fixed points is the point at infinity. When a ≠ d the second fixed point is finite and is given by
In this case the transformation will be a simple transformation composed of translations, rotations, and dilations:
If c = 0 and a = d, then both fixed points are at infinity, and the Möbius transformation corresponds to a pure translation:
Topological proof
Topologically, the fact that (nonidentity) Möbius transformations fix 2 points (with multiplicity) corresponds to the Euler characteristic of the sphere being 2:
Firstly, the projective linear group PGL(2, K) is sharply 3transitive – for any two ordered triples of distinct points, there is a unique map that takes one triple to the other, just as for Möbius transforms, and by the same algebraic proof (essentially dimension counting, as the group is 3dimensional). Thus any map that fixes at least 3 points is the identity.
Next, one can see by identifying the Möbius group with that any Möbius function is homotopic to the identity. Indeed, any member of the general linear group can be reduced to the identity map by GaussJordan elimination, this shows that the projective linear group is pathconnected as well, providing a homotopy to the identity map. The Lefschetz–Hopf theorem states that the sum of the indices (in this context, multiplicity) of the fixed points of a map with finitely many fixed points equals the Lefschetz number of the map, which in this case is the trace of the identity map on homology groups, which is simply the Euler characteristic.
By contrast, the projective linear group of the real projective line, PGL(2, R) need not fix any points – for example has no (real) fixed points: as a complex transformation it fixes ±i^{[note 1]} – while the map 2x fixes the two points of 0 and ∞. This corresponds to the fact that the Euler characteristic of the circle (real projective line) is 0, and thus the Lefschetz fixedpoint theorem says only that it must fix at least 0 points, but possibly more.
Normal form
Möbius transformations are also sometimes written in terms of their fixed points in socalled normal form. We first treat the nonparabolic case, for which there are two distinct fixed points.
Nonparabolic case:
Every nonparabolic transformation is conjugate to a dilation/rotation, i.e., a transformation of the form
If f has distinct fixed points (γ_{1}, γ_{2}) then the transformation has fixed points at 0 and ∞ and is therefore a dilation: . The fixed point equation for the transformation f can then be written
Solving for f gives (in matrix form):
From the above expressions one can calculate the derivatives of f at the fixed points:
Observe that, given an ordering of the fixed points, we can distinguish one of the multipliers (k) of f as the characteristic constant of f. Reversing the order of the fixed points is equivalent to taking the inverse multiplier for the characteristic constant:
For loxodromic transformations, whenever k > 1, one says that γ_{1} is the repulsive fixed point, and γ_{2} is the attractive fixed point. For k < 1, the roles are reversed.
Parabolic case:
In the parabolic case there is only one fixed point γ. The transformation sending that point to ∞ is
Here, β is called the translation length. The fixed point formula for a parabolic transformation is then
Solving for f (in matrix form) gives
If γ = ∞:
Note that β is not the characteristic constant of f, which is always 1 for a parabolic transformation. From the above expressions one can calculate:
Poles of the transformation
The point is called the pole of ; it is that point which is transformed to the point at infinity under .
The inverse pole is that point to which the point at infinity is transformed. The point midway between the two poles is always the same as the point midway between the two fixed points:
These four points are the vertices of a parallelogram which is sometimes called the characteristic parallelogram of the transformation.
A transform can be specified with two fixed points γ_{1}, γ_{2} and the pole .
This allows us to derive a formula for conversion between k and given :
The last expression coincides with one of the (mutually reciprocal) eigenvalue ratios of the matrix
Simple Möbius transformations and composition
A Möbius transformation can be composed as a sequence of simple transformations.
The following simple transformations are also Möbius transformations:
 is a translation.
 is a combination of a homothety and a rotation. If then it is a rotation, if then it is a homothety.
 (inversion and reflection with respect to the real axis)
Composition of simple transformations
If , let:
 (translation by d/c)
 (inversion and reflection with respect to the real axis)
 (homothety and rotation)
 (translation by a/c)
Then these functions can be composed, showing that, if
This decomposition makes many properties of the Möbius transformation obvious.
Elementary properties
A Möbius transformation is equivalent to a sequence of simpler transformations. The composition makes many properties of the Möbius transformation obvious.
Formula for the inverse transformation
The existence of the inverse Möbius transformation and its explicit formula are easily derived by the composition of the inverse functions of the simpler transformations. That is, define functions g_{1}, g_{2}, g_{3}, g_{4} such that each g_{i} is the inverse of f_{i}. Then the composition
Preservation of angles and generalized circles
From this decomposition, we see that Möbius transformations carry over all nontrivial properties of circle inversion. For example, the preservation of angles is reduced to proving that circle inversion preserves angles since the other types of transformations are dilations and isometries (translation, reflection, rotation), which trivially preserve angles.
Furthermore, Möbius transformations map generalized circles to generalized circles since circle inversion has this property. A generalized circle is either a circle or a line, the latter being considered as a circle through the point at infinity. Note that a Möbius transformation does not necessarily map circles to circles and lines to lines: it can mix the two. Even if it maps a circle to another circle, it does not necessarily map the first circle's center to the second circle's center.
Crossratio preservation
Crossratios are invariant under Möbius transformations. That is, if a Möbius transformation maps four distinct points to four distinct points respectively, then
If one of the points is the point at infinity, then the crossratio has to be defined by taking the appropriate limit; e.g. the crossratio of is
The cross ratio of four different points is real if and only if there is a line or a circle passing through them. This is another way to show that Möbius transformations preserve generalized circles.
Conjugation
Two points z_{1} and z_{2} are conjugate with respect to a generalized circle C, if, given a generalized circle D passing through z_{1} and z_{2} and cutting C in two points a and b, (z_{1}, z_{2}; a, b) are in harmonic crossratio (i.e. their cross ratio is −1). This property does not depend on the choice of the circle D. This property is also sometimes referred to as being symmetric with respect to a line or circle.^{[3]}^{[4]}
Two points z, z^{∗} are conjugate with respect to a line, if they are symmetric with respect to the line. Two points are conjugate with respect to a circle if they are exchanged by the inversion with respect to this circle.
The point z^{∗} is conjugate to z when L is the line determined by the vector based upon e^{iθ}, at the point z_{0}. This can be explicitly given as
The point z^{∗} is conjugate to z when C is the circle of a radius r, centered about z_{0}. This can be explicitly given as
Since Möbius transformations preserve generalized circles and crossratios, they also preserve the conjugation.
Projective matrix representations
Isomorphism between the Möbius group and PGL(2, C)
The natural action of PGL(2, C) on the complex projective line CP^{1} is exactly the natural action of the Möbius group on the Riemann sphere
Correspondance between the complex projective line and the Riemann sphere
Here, the projective line CP^{1} and the Riemann sphere are identified as follows:
Here [z_{1}:z_{2}] are homogeneous coordinates on CP^{1}; the point [1:0] corresponds to the point ∞ of the Riemann sphere. By using homogeneous coordinates, many calculations involving Möbius transformations can be simplified, since no case distinctions dealing with ∞ are required.
Action of PGL(2, C) on the complex projective line
Every invertible complex 2×2 matrix
The result is therefore
Which, using the above identification, corresponds to the following point on the Riemann sphere :
Equivalence with a Möbius transformation on the Riemann sphere
Since the above matrix is invertible if and only if its determinant ad − bc is not zero, this induces an identification of the action of the group of Möbius transformations with the action of PGL(2, C) on the complex projective line. In this identification, the above matrix corresponds to the Möbius transformation
This identification is a group isomorphism, since the multiplication of by a non zero scalar does not change the element of PGL(2, C), and, as this multiplication consists of multiplying all matrix entries by this does not change the corresponding Möbius transformation.
Other groups
For any field K, one can similarly identify the group PGL(2, K) of the projective linear automorphisms with the group of fractional linear transformations. This is widely used; for example in the study of homographies of the real line and its applications in optics.
If one divides by a square root of its determinant, one gets a matrix of determinant one. This induces a surjective group homomorphism from the special linear group SL(2, C) to PGL(2, C), with as its kernel.
This allows showing that the Möbius group is a 3dimensional complex Lie group (or a 6dimensional real Lie group), which is a semisimple and noncompact, and that SL(2,C) is a double cover of PSL(2, C). Since SL(2, C) is simplyconnected, it is the universal cover of the Möbius group, and the fundamental group of the Möbius group is Z_{2}.
Specifying a transformation by three points
Given a set of three distinct points on the Riemann sphere and a second set of distinct points , there exists precisely one Möbius transformation with for . (In other words: the action of the Möbius group on the Riemann sphere is sharply 3transitive.) There are several ways to determine from the given sets of points.
Mapping first to 0, 1, ∞
It is easy to check that the Möbius transformation
If is similarly defined to map to then the matrix which maps to becomes
The stabilizer of (as an unordered set) is a subgroup known as the anharmonic group.
Explicit determinant formula
The equation
Subgroups of the Möbius group
If we require the coefficients of a Möbius transformation to be real numbers with , we obtain a subgroup of the Möbius group denoted as PSL(2, R). This is the group of those Möbius transformations that map the upper halfplane H = {x + iy : y > 0} to itself, and is equal to the group of all biholomorphic (or equivalently: bijective, conformal and orientationpreserving) maps H → H. If a proper metric is introduced, the upper halfplane becomes a model of the hyperbolic plane H^{2}, the Poincaré halfplane model, and PSL(2, R) is the group of all orientationpreserving isometries of H^{2} in this model.
The subgroup of all Möbius transformations that map the open disk D = {z : z < 1} to itself consists of all transformations of the form
Since both of the above subgroups serve as isometry groups of H^{2}, they are isomorphic. A concrete isomorphism is given by conjugation with the transformation
Alternatively, consider an open disk with radius r, centered at r i. The Poincaré disk model in this disk becomes identical to the upperhalfplane model as r approaches ∞.
A maximal compact subgroup of the Möbius group is given by (Tóth 2002)^{[5]}
Icosahedral groups of Möbius transformations were used by Felix Klein to give an analytic solution to the quintic equation in (Klein 1913); a modern exposition is given in (Tóth 2002).^{[6]}
If we require the coefficients a, b, c, d of a Möbius transformation to be integers with ad − bc = 1, we obtain the modular group PSL(2, Z), a discrete subgroup of PSL(2, R) important in the study of lattices in the complex plane, elliptic functions and elliptic curves. The discrete subgroups of PSL(2, R) are known as Fuchsian groups; they are important in the study of Riemann surfaces.
Classification
In the following discussion we will always assume that the representing matrix is normalized such that .
Nonidentity Möbius transformations are commonly classified into four types, parabolic, elliptic, hyperbolic and loxodromic, with the hyperbolic ones being a subclass of the loxodromic ones. The classification has both algebraic and geometric significance. Geometrically, the different types result in different transformations of the complex plane, as the figures below illustrate.
The four types can be distinguished by looking at the trace . The trace is invariant under conjugation, that is,
Parabolic transforms
A nonidentity Möbius transformation defined by a matrix of determinant one is said to be parabolic if
The set of all parabolic Möbius transformations with a given fixed point in , together with the identity, forms a subgroup isomorphic to the group of matrices
Characteristic constant
All nonparabolic transformations have two fixed points and are defined by a matrix conjugate to
Elliptic transforms
The transformation is said to be elliptic if it can be represented by a matrix whose trace is real with
A transform is elliptic if and only if λ = 1 and λ ≠ ±1. Writing , an elliptic transform is conjugate to
For any with characteristic constant k, the characteristic constant of is k^{n}. Thus, all Möbius transformations of finite order are elliptic transformations, namely exactly those where λ is a root of unity, or, equivalently, where α is a rational multiple of π. The simplest possibility of a fractional multiple means α = π/2, which is also the unique case of , is also denoted as a circular transform; this corresponds geometrically to rotation by 180° about two fixed points. This class is represented in matrix form as:
Hyperbolic transforms
The transform is said to be hyperbolic if it can be represented by a matrix whose trace is real with
A transform is hyperbolic if and only if λ is real and λ ≠ ±1.
Loxodromic transforms
The transform is said to be loxodromic if is not in [0, 4]. A transformation is loxodromic if and only if .
Historically, navigation by loxodrome or rhumb line refers to a path of constant bearing; the resulting path is a logarithmic spiral, similar in shape to the transformations of the complex plane that a loxodromic Möbius transformation makes. See the geometric figures below.
General classification
Transformation  Trace squared  Multipliers  Class representative  

Circular  σ = 0  k = −1  z ↦ −z  
Elliptic  0 ≤ σ < 4  k = 1  z ↦ e^{iθ} z  
Parabolic  σ = 4  k = 1  z ↦ z + a  
Hyperbolic  4 < σ < ∞  z ↦ e^{θ} z  
Loxodromic  σ ∈ C \ [0,4]  z ↦ kz 
The real case and a note on terminology
Over the real numbers (if the coefficients must be real), there are no nonhyperbolic loxodromic transformations, and the classification is into elliptic, parabolic, and hyperbolic, as for real conics. The terminology is due to considering half the absolute value of the trace, tr/2, as the eccentricity of the transformation – division by 2 corrects for the dimension, so the identity has eccentricity 1 (tr/n is sometimes used as an alternative for the trace for this reason), and absolute value corrects for the trace only being defined up to a factor of ±1 due to working in PSL. Alternatively one may use half the trace squared as a proxy for the eccentricity squared, as was done above; these classifications (but not the exact eccentricity values, since squaring and absolute values are different) agree for real traces but not complex traces. The same terminology is used for the classification of elements of SL(2, R) (the 2fold cover), and analogous classifications are used elsewhere. Loxodromic transformations are an essentially complex phenomenon, and correspond to complex eccentricities.
Geometric interpretation of the characteristic constant
The following picture depicts (after stereographic transformation from the sphere to the plane) the two fixed points of a Möbius transformation in the nonparabolic case:
The characteristic constant can be expressed in terms of its logarithm:
Elliptic transformations
If ρ = 0, then the fixed points are neither attractive nor repulsive but indifferent, and the transformation is said to be elliptic. These transformations tend to move all points in circles around the two fixed points. If one of the fixed points is at infinity, this is equivalent to doing an affine rotation around a point.
If we take the oneparameter subgroup generated by any elliptic Möbius transformation, we obtain a continuous transformation, such that every transformation in the subgroup fixes the same two points. All other points flow along a family of circles which is nested between the two fixed points on the Riemann sphere. In general, the two fixed points can be any two distinct points.
This has an important physical interpretation. Imagine that some observer rotates with constant angular velocity about some axis. Then we can take the two fixed points to be the North and South poles of the celestial sphere. The appearance of the night sky is now transformed continuously in exactly the manner described by the oneparameter subgroup of elliptic transformations sharing the fixed points 0, ∞, and with the number α corresponding to the constant angular velocity of our observer.
Here are some figures illustrating the effect of an elliptic Möbius transformation on the Riemann sphere (after stereographic projection to the plane):
These pictures illustrate the effect of a single Möbius transformation. The oneparameter subgroup which it generates continuously moves points along the family of circular arcs suggested by the pictures.
Hyperbolic transformations
If α is zero (or a multiple of 2π), then the transformation is said to be hyperbolic. These transformations tend to move points along circular paths from one fixed point toward the other.
If we take the oneparameter subgroup generated by any hyperbolic Möbius transformation, we obtain a continuous transformation, such that every transformation in the subgroup fixes the same two points. All other points flow along a certain family of circular arcs away from the first fixed point and toward the second fixed point. In general, the two fixed points may be any two distinct points on the Riemann sphere.
This too has an important physical interpretation. Imagine that an observer accelerates (with constant magnitude of acceleration) in the direction of the North pole on his celestial sphere. Then the appearance of the night sky is transformed in exactly the manner described by the oneparameter subgroup of hyperbolic transformations sharing the fixed points 0, ∞, with the real number ρ corresponding to the magnitude of his acceleration vector. The stars seem to move along longitudes, away from the South pole toward the North pole. (The longitudes appear as circular arcs under stereographic projection from the sphere to the plane.)
Here are some figures illustrating the effect of a hyperbolic Möbius transformation on the Riemann sphere (after stereographic projection to the plane):
These pictures resemble the field lines of a positive and a negative electrical charge located at the fixed points, because the circular flow lines subtend a constant angle between the two fixed points.
Loxodromic transformations
If both ρ and α are nonzero, then the transformation is said to be loxodromic. These transformations tend to move all points in Sshaped paths from one fixed point to the other.
The word "loxodrome" is from the Greek: "λοξος (loxos), slanting + δρόμος (dromos), course". When sailing on a constant bearing – if you maintain a heading of (say) northeast, you will eventually wind up sailing around the north pole in a logarithmic spiral. On the mercator projection such a course is a straight line, as the north and south poles project to infinity. The angle that the loxodrome subtends relative to the lines of longitude (i.e. its slope, the "tightness" of the spiral) is the argument of k. Of course, Möbius transformations may have their two fixed points anywhere, not just at the north and south poles. But any loxodromic transformation will be conjugate to a transform that moves all points along such loxodromes.
If we take the oneparameter subgroup generated by any loxodromic Möbius transformation, we obtain a continuous transformation, such that every transformation in the subgroup fixes the same two points. All other points flow along a certain family of curves, away from the first fixed point and toward the second fixed point. Unlike the hyperbolic case, these curves are not circular arcs, but certain curves which under stereographic projection from the sphere to the plane appear as spiral curves which twist counterclockwise infinitely often around one fixed point and twist clockwise infinitely often around the other fixed point. In general, the two fixed points may be any two distinct points on the Riemann sphere.
You can probably guess the physical interpretation in the case when the two fixed points are 0, ∞: an observer who is both rotating (with constant angular velocity) about some axis and moving along the same axis, will see the appearance of the night sky transform according to the oneparameter subgroup of loxodromic transformations with fixed points 0, ∞, and with ρ, α determined respectively by the magnitude of the actual linear and angular velocities.
Stereographic projection
These images show Möbius transformations stereographically projected onto the Riemann sphere. Note in particular that when projected onto a sphere, the special case of a fixed point at infinity looks no different from having the fixed points in an arbitrary location.
One fixed point at infinity  
Fixed points diametrically opposite  
Fixed points in an arbitrary location  
Iterating a transformation
If a transformation has fixed points γ_{1}, γ_{2}, and characteristic constant k, then will have .
This can be used to iterate a transformation, or to animate one by breaking it up into steps.
These images show three points (red, blue and black) continuously iterated under transformations with various characteristic constants.
And these images demonstrate what happens when you transform a circle under Hyperbolic, Elliptical, and Loxodromic transforms. In the elliptical and loxodromic images, the value of α is 1/10.
Higher dimensions
In higher dimensions, a Möbius transformation is a homeomorphism of , the onepoint compactification of , which is a finite composition of inversions in spheres and reflections in hyperplanes.^{[7]} Liouville's theorem in conformal geometry states that in dimension at least three, all conformal transformations are Möbius transformations. Every Möbius transformation can be put in the form
The orientationpreserving Möbius transformations form the connected component of the identity in the Möbius group. In dimension n = 2, the orientationpreserving Möbius transformations are exactly the maps of the Riemann sphere covered here. The orientationreversing ones are obtained from these by complex conjugation.^{[9]}
The domain of Möbius transformations, i.e. , is homeomorphic to the ndimensional sphere . The canonical isomorphism between these two spaces is the Cayley transform, which is itself a Möbius transformation of . This identification means that Möbius transformations can also be thought of as conformal isomorphisms of . The nsphere, together with action of the Möbius group, is a geometric structure (in the sense of Klein's Erlangen program) called Möbius geometry.^{[10]}
Applications
Lorentz transformation
An isomorphism of the Möbius group with the Lorentz group was noted by several authors: Based on previous work of Felix Klein (1893, 1897)^{[11]} on automorphic functions related to hyperbolic geometry and Möbius geometry, Gustav Herglotz (1909)^{[12]} showed that hyperbolic motions (i.e. isometric automorphisms of a hyperbolic space) transforming the unit sphere into itself correspond to Lorentz transformations, by which Herglotz was able to classify the oneparameter Lorentz transformations into loxodromic, elliptic, hyperbolic, and parabolic groups. Other authors include Emil Artin (1957),^{[13]} H. S. M. Coxeter (1965),^{[14]} and Roger Penrose, Wolfgang Rindler (1984),^{[15]} Tristan Needham (1997)^{[16]} and W. M. Olivia (2002).^{[17]}
Minkowski space consists of the fourdimensional real coordinate space R^{4} consisting of the space of ordered quadruples (x_{0}, x_{1}, x_{2}, x_{3}) of real numbers, together with a quadratic form
Borrowing terminology from special relativity, points with Q > 0 are considered timelike; in addition, if x_{0} > 0, then the point is called futurepointing. Points with Q < 0 are called spacelike. The null cone S consists of those points where Q = 0; the future null cone N^{+} are those points on the null cone with x_{0} > 0. The celestial sphere is then identified with the collection of rays in N^{+} whose initial point is the origin of R^{4}. The collection of linear transformations on R^{4} with positive determinant preserving the quadratic form Q and preserving the time direction form the restricted Lorentz group SO^{+}(1, 3).
In connection with the geometry of the celestial sphere, the group of transformations SO^{+}(1, 3) is identified with the group PSL(2, C) of Möbius transformations of the sphere. To each (x_{0}, x_{1}, x_{2}, x_{3}) ∈ R^{4}, associate the hermitian matrix
The determinant of the matrix X is equal to Q(x_{0}, x_{1}, x_{2}, x_{3}). The special linear group acts on the space of such matrices via
(1) 
for each A ∈ SL(2, C), and this action of SL(2, C) preserves the determinant of X because det A = 1. Since the determinant of X is identified with the quadratic form Q, SL(2, C) acts by Lorentz transformations. On dimensional grounds, SL(2, C) covers a neighborhood of the identity of SO(1, 3). Since SL(2, C) is connected, it covers the entire restricted Lorentz group SO^{+}(1, 3). Furthermore, since the kernel of the action (1) is the subgroup {±I}, then passing to the quotient group gives the group isomorphism
(2) 
Focusing now attention on the case when (x_{0}, x_{1}, x_{2}, x_{3}) is null, the matrix X has zero determinant, and therefore splits as the outer product of a complex twovector ξ with its complex conjugate:
(3) 
The twocomponent vector ξ is acted upon by SL(2, C) in a manner compatible with (1). It is now clear that the kernel of the representation of SL(2, C) on hermitian matrices is {±I}.
The action of PSL(2, C) on the celestial sphere may also be described geometrically using stereographic projection. Consider first the hyperplane in R^{4} given by x_{0} = 1. The celestial sphere may be identified with the sphere S^{+} of intersection of the hyperplane with the future null cone N^{+}. The stereographic projection from the north pole (1, 0, 0, 1) of this sphere onto the plane x_{3} = 0 takes a point with coordinates (1, x_{1}, x_{2}, x_{3}) with
Introducing the complex coordinate
(4) 
The action of SO^{+}(1, 3) on the points of N^{+} does not preserve the hyperplane S^{+}, but acting on points in S^{+} and then rescaling so that the result is again in S^{+} gives an action of SO^{+}(1, 3) on the sphere which goes over to an action on the complex variable ζ. In fact, this action is by fractional linear transformations, although this is not easily seen from this representation of the celestial sphere. Conversely, for any fractional linear transformation of ζ variable goes over to a unique Lorentz transformation on N^{+}, possibly after a suitable (uniquely determined) rescaling.
A more invariant description of the stereographic projection which allows the action to be more clearly seen is to consider the variable ζ = z:w as a ratio of a pair of homogeneous coordinates for the complex projective line CP^{1}. The stereographic projection goes over to a transformation from C^{2} − {0} to N^{+} which is homogeneous of degree two with respect to real scalings
(5) 
which agrees with (4) upon restriction to scales in which The components of (5) are precisely those obtained from the outer product
In summary, the action of the restricted Lorentz group SO^{+}(1,3) agrees with that of the Möbius group PSL(2, C). This motivates the following definition. In dimension n ≥ 2, the Möbius group Möb(n) is the group of all orientationpreserving conformal isometries of the round sphere S^{n} to itself. By realizing the conformal sphere as the space of futurepointing rays of the null cone in the Minkowski space R^{1,n+1}, there is an isomorphism of Möb(n) with the restricted Lorentz group SO^{+}(1,n+1) of Lorentz transformations with positive determinant, preserving the direction of time.
Coxeter began instead with the equivalent quadratic form .
He identified the Lorentz group with transformations for which {x  Q(x) = −1} is stable. Then he interpreted the x's as homogeneous coordinates and {x  Q(x) = 0}, the null cone, as the Cayley absolute for a hyperbolic space of points {x  Q(x) < 0}. Next, Coxeter introduced the variables
Hyperbolic space
As seen above, the Möbius group PSL(2, C) acts on Minkowski space as the group of those isometries that preserve the origin, the orientation of space and the direction of time. Restricting to the points where Q = 1 in the positive light cone, which form a model of hyperbolic 3space H^{3}, we see that the Möbius group acts on H^{3} as a group of orientationpreserving isometries. In fact, the Möbius group is equal to the group of orientationpreserving isometries of hyperbolic 3space. If we use the Poincaré ball model, identifying the unit ball in R^{3} with H^{3}, then we can think of the Riemann sphere as the "conformal boundary" of H^{3}. Every orientationpreserving isometry of H^{3} gives rise to a Möbius transformation on the Riemann sphere and vice versa.
See also
 Bilinear transform
 Conformal geometry
 Fuchsian group
 Generalised circle
 Hyperbolic geometry
 Infinite compositions of analytic functions
 Inversion transformation
 Kleinian group
 Lie sphere geometry
 Linear fractional transformation
 Liouville's theorem (conformal mappings)
 Lorentz group
 Modular group
 Poincaré halfplane model
 Projective geometry
 Projective line over a ring
 Representation theory of the Lorentz group
 Schottky group
 Smith chart
Notes
 ^ Geometrically this map is the stereographic projection of a rotation by 90° around ±i with period 4, which takes
References
Specific
 ^ Arnold & Rogness 2008, Theorem 1.
 ^ Needham, Tristan (2021). Differential Geometry and Forms; A Mathematical Drama in Five Acts. Princeton University Press. p. 77, footnote 16. ISBN 9780691203690.
 ^ Olsen, John, The Geometry of Mobius Transformations (PDF)
 ^ Weisstein, Eric W. "Symmetric Points". MathWorld.
 ^ Tóth 2002, Section 1.2, Rotations and Möbius Transformations, p. 22.
 ^ Tóth 2002, Section 1.6, Additional Topic: Klein's Theory of the Icosahedron, p. 66.
 ^ Iwaniec, Tadeusz and Martin, Gaven, The Liouville theorem, Analysis and topology, 339–361, World Sci. Publ., River Edge, NJ, 1998
 ^ J.B. Wilker (1981) "Inversive Geometry", MR0661793
 ^ Berger, Marcel (1987), Geometry II, Springer (Universitext), p. 18.10
 ^ Akivis, Maks; Goldberg, Vladislav (1992), Conformal differential geometry and its generalizations, WileyInterscience
 ^ Felix Klein (1893), NichtEuklidische Geometrie, Autogr. Vorl., Göttingen;
Robert Fricke & Felix Klein (1897), Autormorphe Funktionen I., Teubner, Leipzig  ^ Herglotz, Gustav (1910) [1909], "Über den vom Standpunkt des Relativitätsprinzips aus als starr zu bezeichnenden Körper" [On bodies that are to be designated as 'rigid' from the relativity principle standpoint], Annalen der Physik (in German), 336 (2): 393–415, Bibcode:1910AnP...336..393H, doi:10.1002/andp.19103360208
 ^ Emil Artin (1957) Geometric Algebra, page 204
 ^ H. S. M. Coxeter (1967) "The Lorentz group and the group of homographies", in L. G. Kovacs & B. H. Neumann (editors) Proceedings of the International Conference on The Theory of Groups held at Australian National University, Canberra, 10—20 August 1965, Gordon and Breach Science Publishers
 ^ Penrose & Rindler 1984, pp. 8–31.
 ^ Needham, Tristan (1997). Visual Complex Analysis (PDF). Oxford: Oxford University Press. pp. 122–124.
 ^ Olivia, Waldyr Muniz (2002). "Appendix B: Möbius transformations and the Lorentz group". Geometric Mechanics. Springer. pp. 195–221. ISBN 3540442421. MR 1990795.
General
 Arnold, Douglas N.; Rogness, Jonathan (2008), "Möbius Transformations Revealed" (PDF), Notices of the AMS, 55 (10): 1226–1231
 Beardon, Alan F. (1995), The Geometry of Discrete Groups, New York: SpringerVerlag, ISBN 9780387907888
 Hall, G. S. (2004), Symmetries and Curvature Structure in General Relativity, Singapore: World Scientific, ISBN 9789810210519 (See Chapter 6 for the classification, up to conjugacy, of the Lie subalgebras of the Lie algebra of the Lorentz group.)
 Katok, Svetlana (1992), Fuchsian Groups, Chicago:University of Chicago Press, ISBN 9780226425832 See Chapter 2.
 Klein, Felix (1913) [1st German ed. 1884], Lectures on the icosahedron and the solution of equations of the fifth degree, translated by Morrice, George Gavin (2nd ed.), London: Kegan Paul, Trench, Trübner, & Co. translated from Vorlesungen über das Ikosaeder und die Auflösung der Gleichungen vom fünften Grade (in German), Teubner, 1884
 Knopp, Konrad (1952), Elements of the Theory of Functions, New York: Dover, ISBN 9780486601540 (See Chapters 3–5 of this classic book for a beautiful introduction to the Riemann sphere, stereographic projection, and Möbius transformations.)
 Mumford, David; Series, Caroline; Wright, David (2002), Indra's Pearls: The Vision of Felix Klein, Cambridge University Press, ISBN 9780521352536 (Aimed at nonmathematicians, provides an excellent exposition of theory and results, richly illustrated with diagrams.)
 Needham, Tristan (1997), Visual Complex Analysis, Oxford: Clarendon Press, ISBN 9780198534464 (See Chapter 3 for a beautifully illustrated introduction to Möbius transformations, including their classification up to conjugacy.)
 Penrose, Roger; Rindler, Wolfgang (1984), Spinors and space–time, Volume 1: Twospinor calculus and relativistic fields, Cambridge University Press, ISBN 9780521245272
 Schwerdtfeger, Hans (1979), Geometry of Complex Numbers, Dover, ISBN 9780486638300 (See Chapter 2 for an introduction to Möbius transformations.)
 Tóth, Gábor (2002), Finite Möbius groups, minimal immersions of spheres, and moduli
Further reading
 Lawson, M. V. (1998). "The Möbius Inverse Monoid". Journal of Algebra. 200 (2): 428. doi:10.1006/jabr.1997.7242.
External links
 "Quasiconformal mapping", Encyclopedia of Mathematics, EMS Press, 2001 [1994]
 Conformal maps gallery
 Weisstein, Eric W. "Linear Fractional Transformation". MathWorld.