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Möbius transformation

From Wikipedia, the free encyclopedia
Rational function of the form (az + b)/(cz + d)
Not to be confused withMöbius transform orMöbius function.

Ingeometry andcomplex analysis, aMöbius transformation of thecomplex plane is arational function of the formf(z)=az+bcz+d{\displaystyle f(z)={\frac {az+b}{cz+d}}}of onecomplex variablez; here the coefficientsa,b,c,d are complex numbers satisfyingadbc ≠ 0.

Geometrically, a Möbius transformation can be obtained by first applying the inversestereographic projection from the plane to the unitsphere, 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 theprojective transformations of thecomplex projective line. They form agroup called theMöbius group, which is theprojective linear groupPGL(2,C). Together with itssubgroups, 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 ofAugust Ferdinand Möbius; they are an example ofhomographies,linear fractional transformations, bilinear transformations, and spin transformations (in relativity theory).[2]

Overview

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Möbius transformations are defined on theextended complex planeC^=C{}{\displaystyle {\widehat {\mathbb {C} }}=\mathbb {C} \cup \{\infty \}} (i.e., thecomplex plane augmented by thepoint at infinity).

Stereographic projection identifiesC^{\displaystyle {\widehat {\mathbb {C} }}} with a sphere, which is then called theRiemann sphere; alternatively,C^{\displaystyle {\widehat {\mathbb {C} }}} can be thought of as the complexprojective lineCP1{\displaystyle \mathbb {C} \mathbb {P} ^{1}}. The Möbius transformations are exactly thebijectiveconformal maps from the Riemann sphere to itself, i.e., theautomorphisms of the Riemann sphere as acomplex manifold; alternatively, they are the automorphisms ofCP1{\displaystyle \mathbb {C} \mathbb {P} ^{1}} as an algebraic variety. Therefore, the set of all Möbius transformations forms agroup undercomposition. This group is called the Möbius group, and is sometimes denotedAut(C^){\displaystyle \operatorname {Aut} ({\widehat {\mathbb {C} }})}.

The Möbius group isisomorphic to the group of orientation-preservingisometries ofhyperbolic 3-space and therefore plays an important role when studyinghyperbolic 3-manifolds.

Inphysics, theidentity component of theLorentz group acts on thecelestial 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 oftwistor theory.

Certainsubgroups of the Möbius group form the automorphism groups of the othersimply-connected Riemann surfaces (thecomplex plane and thehyperbolic plane). As such, Möbius transformations play an important role in the theory ofRiemann surfaces. Thefundamental group of every Riemann surface is adiscrete subgroup of the Möbius group (seeFuchsian group andKleinian group). A particularly important discrete subgroup of the Möbius group is themodular group; it is central to the theory of manyfractals,modular forms,elliptic curves andPellian equations.

Möbius transformations can be more generally defined in spaces of dimensionn > 2 as the bijective conformal orientation-preserving maps from then-sphere to then-sphere. Such a transformation is the most general form of conformal mapping of a domain. According toLiouville's theorem a Möbius transformation can be expressed as a composition of translations,similarities, orthogonal transformations and inversions.

Definition

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The general form of a Möbius transformation is given byf(z)=az+bcz+d,{\displaystyle f(z)={\frac {az+b}{cz+d}},}wherea,b,c,d are anycomplex numbers that satisfyadbc ≠ 0.

In casec ≠ 0, this definition is extended to the wholeRiemann sphere by definingf(dc)=,f()=ac.{\displaystyle {\begin{aligned}f\left({\frac {-d}{c}}\right)&=\infty ,\\f(\infty )&={\frac {a}{c}}.\end{aligned}}}

Ifc = 0, we definef()=.{\displaystyle f(\infty )=\infty .}

Thus a Möbius transformation is always a bijectiveholomorphic function from the Riemann sphere to the Riemann sphere.

The set of all Möbius transformations forms agroup undercomposition. This group can be given the structure of acomplex manifold in such a way that composition and inversion areholomorphic maps. The Möbius group is then acomplex Lie group. The Möbius group is usually denotedAut(C^){\displaystyle \operatorname {Aut} ({\widehat {\mathbb {C} }})} as it is theautomorphism group of the Riemann sphere.

Ifad =bc, the rational function defined above is a constant (unlessc =d = 0, when it is undefined):az+bcz+d=ac=bd,{\displaystyle {\frac {az+b}{cz+d}}={\frac {a}{c}}={\frac {b}{d}},}where a fraction with a zero denominator is ignored. A constant function is not bijective and is thus not considered a Möbius transformation.

An alternative definition is given as the kernel of theSchwarzian derivative.

Fixed points

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Every non-identity Möbius transformation has twofixed pointsγ1,γ2{\displaystyle \gamma _{1},\gamma _{2}} on the Riemann sphere. The fixed points are counted here withmultiplicity; theparabolic 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

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The fixed points of the transformationf(z)=az+bcz+d{\displaystyle f(z)={\frac {az+b}{cz+d}}}are obtained by solving the fixed point equationf(γ) =γ. Forc ≠ 0, this has two roots obtained by expanding this equation tocγ2(ad)γb=0 ,{\displaystyle c\gamma ^{2}-(a-d)\gamma -b=0\ ,}and applying thequadratic formula. The roots areγ1,2=(ad)±(ad)2+4bc2c=(ad)±Δ2c{\displaystyle \gamma _{1,2}={\frac {(a-d)\pm {\sqrt {(a-d)^{2}+4bc}}}{2c}}={\frac {(a-d)\pm {\sqrt {\Delta }}}{2c}}}with discriminantΔ=(trH)24detH=(a+d)24(adbc),{\displaystyle \Delta =(\operatorname {tr} {\mathfrak {H}})^{2}-4\det {\mathfrak {H}}=(a+d)^{2}-4(ad-bc),}where the matrixH=(abcd){\displaystyle {\mathfrak {H}}={\begin{pmatrix}a&b\\c&d\end{pmatrix}}}represents the transformation.Parabolic transforms have coincidental fixed points due to zero discriminant. Forc nonzero and nonzero discriminant the transform is elliptic or hyperbolic.

Whenc = 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. Whenad the second fixed point is finite and is given byγ=bad.{\displaystyle \gamma =-{\frac {b}{a-d}}.}

In this case the transformation will be a simple transformation composed oftranslations,rotations, anddilations:zαz+β.{\displaystyle z\mapsto \alpha z+\beta .}

Ifc = 0 anda =d, then both fixed points are at infinity, and the Möbius transformation corresponds to a pure translation:zz+β.{\displaystyle z\mapsto z+\beta .}

Topological proof

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Topologically, the fact that (non-identity) Möbius transformations fix 2 points (with multiplicity) corresponds to theEuler characteristic of the sphere being 2:χ(C^)=2.{\displaystyle \chi ({\hat {\mathbb {C} }})=2.}

Firstly, theprojective linear groupPGL(2,K) issharply 3-transitive – 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 (essentiallydimension counting, as the group is 3-dimensional). Thus any map that fixes at least 3 points is the identity.

Next, one can see by identifying the Möbius group withPGL(2,C){\displaystyle \mathrm {PGL} (2,\mathbb {C} )} that any Möbius function is homotopic to the identity. Indeed, any member of thegeneral linear group can be reduced to the identity map byGauss-Jordan elimination, this shows that the projective linear group is path-connected as well, providing a homotopy to the identity map. TheLefschetz–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 theLefschetz 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(1+x)/(1x){\displaystyle (1+x)/(1-x)} 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 fixed-point theorem says only that it must fix at least 0 points, but possibly more.

Normal form

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Möbius transformations are also sometimes written in terms of their fixed points in so-callednormal form. We first treat the non-parabolic case, for which there are two distinct fixed points.

Non-parabolic case:

Every non-parabolic transformation isconjugate to a dilation/rotation, i.e., a transformation of the formzkz{\displaystyle z\mapsto kz}(kC) with fixed points at 0 and ∞. To see this define a mapg(z)=zγ1zγ2{\displaystyle g(z)={\frac {z-\gamma _{1}}{z-\gamma _{2}}}}which sends the points (γ1,γ2) to (0, ∞). Here we assume thatγ1 andγ2 are distinct and finite. If one of them is already at infinity theng can be modified so as to fix infinity and send the other point to 0.

Iff has distinct fixed points (γ1,γ2) then the transformationgfg1{\displaystyle gfg^{-1}} has fixed points at 0 and ∞ and is therefore a dilation:gfg1(z)=kz{\displaystyle gfg^{-1}(z)=kz}. The fixed point equation for the transformationf can then be writtenf(z)γ1f(z)γ2=kzγ1zγ2.{\displaystyle {\frac {f(z)-\gamma _{1}}{f(z)-\gamma _{2}}}=k{\frac {z-\gamma _{1}}{z-\gamma _{2}}}.}

Solving forf gives (in matrix form):H(k;γ1,γ2)=(γ1kγ2(k1)γ1γ21kkγ1γ2){\displaystyle {\mathfrak {H}}(k;\gamma _{1},\gamma _{2})={\begin{pmatrix}\gamma _{1}-k\gamma _{2}&(k-1)\gamma _{1}\gamma _{2}\\1-k&k\gamma _{1}-\gamma _{2}\end{pmatrix}}}or, if one of the fixed points is at infinity:H(k;γ,)=(k(1k)γ01).{\displaystyle {\mathfrak {H}}(k;\gamma ,\infty )={\begin{pmatrix}k&(1-k)\gamma \\0&1\end{pmatrix}}.}

From the above expressions one can calculate the derivatives off at the fixed points:f(γ1)=k{\displaystyle f'(\gamma _{1})=k} andf(γ2)=1/k.{\displaystyle f'(\gamma _{2})=1/k.}

Observe that, given an ordering of the fixed points, we can distinguish one of the multipliers (k) off as thecharacteristic constant off. Reversing the order of the fixed points is equivalent to taking the inverse multiplier for the characteristic constant:H(k;γ1,γ2)=H(1/k;γ2,γ1).{\displaystyle {\mathfrak {H}}(k;\gamma _{1},\gamma _{2})={\mathfrak {H}}(1/k;\gamma _{2},\gamma _{1}).}

For loxodromic transformations, whenever|k| > 1, one says thatγ1 is therepulsive fixed point, andγ2 is theattractive fixed point. For|k| < 1, the roles are reversed.

Parabolic case:

In the parabolic case there is only one fixed pointγ. The transformation sending that point to ∞ isg(z)=1zγ{\displaystyle g(z)={\frac {1}{z-\gamma }}}or the identity ifγ is already at infinity. The transformationgfg1{\displaystyle gfg^{-1}} fixes infinity and is therefore a translation:gfg1(z)=z+β.{\displaystyle gfg^{-1}(z)=z+\beta \,.}

Here,β is called thetranslation length. The fixed point formula for a parabolic transformation is then1f(z)γ=1zγ+β.{\displaystyle {\frac {1}{f(z)-\gamma }}={\frac {1}{z-\gamma }}+\beta .}

Solving forf (in matrix form) givesH(β;γ)=(1+γββγ2β1γβ){\displaystyle {\mathfrak {H}}(\beta ;\gamma )={\begin{pmatrix}1+\gamma \beta &-\beta \gamma ^{2}\\\beta &1-\gamma \beta \end{pmatrix}}}Note thatdetH(β;γ)=|H(β;γ)|=det(1+γββγ2β1γβ)=1γ2β2+γ2β2=1{\displaystyle \det {\mathfrak {H}}(\beta ;\gamma )=|{\mathfrak {H}}(\beta ;\gamma )|=\det {\begin{pmatrix}1+\gamma \beta &-\beta \gamma ^{2}\\\beta &1-\gamma \beta \end{pmatrix}}=1-\gamma ^{2}\beta ^{2}+\gamma ^{2}\beta ^{2}=1}

Ifγ = ∞:H(β;)=(1β01){\displaystyle {\mathfrak {H}}(\beta ;\infty )={\begin{pmatrix}1&\beta \\0&1\end{pmatrix}}}

Note thatβ isnot the characteristic constant off, which is always 1 for a parabolic transformation. From the above expressions one can calculate:f(γ)=1.{\displaystyle f'(\gamma )=1.}

Poles of the transformation

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The pointz=dc{\textstyle z_{\infty }=-{\frac {d}{c}}} is called thepole ofH{\displaystyle {\mathfrak {H}}}; it is that point which is transformed to the point at infinity underH{\displaystyle {\mathfrak {H}}}.

The inverse poleZ=ac{\textstyle Z_{\infty }={\frac {a}{c}}} 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:γ1+γ2=z+Z.{\displaystyle \gamma _{1}+\gamma _{2}=z_{\infty }+Z_{\infty }.}

These four points are the vertices of aparallelogram which is sometimes called thecharacteristic parallelogram of the transformation.

A transformH{\displaystyle {\mathfrak {H}}} can be specified with two fixed pointsγ1,γ2 and the polez{\displaystyle z_{\infty }}.

H=(Zγ1γ21z),Z=γ1+γ2z.{\displaystyle {\mathfrak {H}}={\begin{pmatrix}Z_{\infty }&-\gamma _{1}\gamma _{2}\\1&-z_{\infty }\end{pmatrix}},\;\;Z_{\infty }=\gamma _{1}+\gamma _{2}-z_{\infty }.}

This allows us to derive a formula for conversion betweenk andz{\displaystyle z_{\infty }} givenγ1,γ2{\displaystyle \gamma _{1},\gamma _{2}}:z=kγ1γ21k{\displaystyle z_{\infty }={\frac {k\gamma _{1}-\gamma _{2}}{1-k}}}k=γ2zγ1z=Zγ1Zγ2=acγ1acγ2,{\displaystyle k={\frac {\gamma _{2}-z_{\infty }}{\gamma _{1}-z_{\infty }}}={\frac {Z_{\infty }-\gamma _{1}}{Z_{\infty }-\gamma _{2}}}={\frac {a-c\gamma _{1}}{a-c\gamma _{2}}},}which reduces down tok=(a+d)+(ad)2+4bc(a+d)(ad)2+4bc.{\displaystyle k={\frac {(a+d)+{\sqrt {(a-d)^{2}+4bc}}}{(a+d)-{\sqrt {(a-d)^{2}+4bc}}}}.}

The last expression coincides with one of the (mutually reciprocal)eigenvalue ratiosλ1λ2{\textstyle {\frac {\lambda _{1}}{\lambda _{2}}}} ofH{\displaystyle {\mathfrak {H}}} (compare the discussion in the preceding section about the characteristic constant of a transformation). Itscharacteristic polynomial is equal todet(λI2H)=λ2trHλ+detH=λ2(a+d)λ+(adbc){\displaystyle \det(\lambda I_{2}-{\mathfrak {H}})=\lambda ^{2}-\operatorname {tr} {\mathfrak {H}}\,\lambda +\det {\mathfrak {H}}=\lambda ^{2}-(a+d)\lambda +(ad-bc)}which has rootsλi=(a+d)±(ad)2+4bc2=(a+d)±(a+d)24(adbc)2=cγi+d.{\displaystyle \lambda _{i}={\frac {(a+d)\pm {\sqrt {(a-d)^{2}+4bc}}}{2}}={\frac {(a+d)\pm {\sqrt {(a+d)^{2}-4(ad-bc)}}}{2}}=c\gamma _{i}+d\,.}

Simple Möbius transformations and composition

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A Möbius transformation can becomposed as a sequence of simple transformations.

The following simple transformations are also Möbius transformations:

Composition of simple transformations

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Ifc0{\displaystyle c\neq 0}, let:

Then these functions can becomposed, showing that, iff(z)=az+bcz+d,{\displaystyle f(z)={\frac {az+b}{cz+d}},}one hasf=f4f3f2f1.{\displaystyle f=f_{4}\circ f_{3}\circ f_{2}\circ f_{1}.}In other terms, one hasaz+bcz+d=ac+ez+dc,{\displaystyle {\frac {az+b}{cz+d}}={\frac {a}{c}}+{\frac {e}{z+{\frac {d}{c}}}},}withe=bcadc2.{\displaystyle e={\frac {bc-ad}{c^{2}}}.}

This decomposition makes many properties of the Möbius transformation obvious.

Elementary properties

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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

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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 functionsg1,g2,g3,g4 such that eachgi is the inverse offi. Then the compositiong1g2g3g4(z)=f1(z)=dzbcz+a{\displaystyle g_{1}\circ g_{2}\circ g_{3}\circ g_{4}(z)=f^{-1}(z)={\frac {dz-b}{-cz+a}}}gives a formula for the inverse.

Preservation of angles and generalized circles

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From this decomposition, we see that Möbius transformations carry over all non-trivial properties ofcircle inversion. For example, the preservation of angles is reduced to proving that circle inversion preserves angles since the other types of transformations are dilations andisometries (translation, reflection, rotation), which trivially preserve angles.

Furthermore, Möbius transformations mapgeneralized 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.

Cross-ratio preservation

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Cross-ratios are invariant under Möbius transformations. That is, if a Möbius transformation maps four distinct pointsz1,z2,z3,z4{\displaystyle z_{1},z_{2},z_{3},z_{4}} to four distinct pointsw1,w2,w3,w4{\displaystyle w_{1},w_{2},w_{3},w_{4}} respectively, then(z1z3)(z2z4)(z2z3)(z1z4)=(w1w3)(w2w4)(w2w3)(w1w4).{\displaystyle {\frac {(z_{1}-z_{3})(z_{2}-z_{4})}{(z_{2}-z_{3})(z_{1}-z_{4})}}={\frac {(w_{1}-w_{3})(w_{2}-w_{4})}{(w_{2}-w_{3})(w_{1}-w_{4})}}.}

If one of the pointsz1,z2,z3,z4{\displaystyle z_{1},z_{2},z_{3},z_{4}} is the point at infinity, then the cross-ratio has to be defined by taking the appropriate limit; e.g. the cross-ratio ofz1,z2,z3,{\displaystyle z_{1},z_{2},z_{3},\infty } is(z1z3)(z2z3).{\displaystyle {\frac {(z_{1}-z_{3})}{(z_{2}-z_{3})}}.}

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

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Two pointsz1 andz2 areconjugate with respect to a generalized circleC, if, given a generalized circleD passing throughz1 andz2 and cuttingC in two pointsa andb,(z1,z2;a,b) are inharmonic cross-ratio (i.e. their cross ratio is −1). This property does not depend on the choice of the circleD. This property is also sometimes referred to as beingsymmetric with respect to a line or circle.[3][4]

Two pointsz,z are conjugate with respect to a line, if they aresymmetric with respect to the line. Two points are conjugate with respect to a circle if they are exchanged by theinversion with respect to this circle.

The pointz is conjugate toz whenL is the line determined by the vector based upone, at the pointz0. This can be explicitly given asz=e2iθzz0¯+z0.{\displaystyle z^{*}=e^{2i\theta }\,{\overline {z-z_{0}}}+z_{0}.}

The pointz is conjugate toz whenC is the circle of a radiusr, centered aboutz0. This can be explicitly given asz=r2zz0¯+z0.{\displaystyle z^{*}={\frac {r^{2}}{\overline {z-z_{0}}}}+z_{0}.}

Since Möbius transformations preserve generalized circles and cross-ratios, they also preserve the conjugation.

Projective matrix representations

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Isomorphism between the Möbius group andPGL(2, C)

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The naturalaction ofPGL(2,C) on thecomplex projective lineCP1 is exactly the natural action of the Möbius group on the Riemann sphere

Correspondance between the complex projective line and the Riemann sphere

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Here, the projective lineCP1 and the Riemann sphere are identified as follows:[z1:z2] z1z2.{\displaystyle [z_{1}:z_{2}]\ \thicksim {\frac {z_{1}}{z_{2}}}.}

Here [z1:z2] arehomogeneous coordinates onCP1; 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

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Everyinvertible complex 2×2 matrixH=(abcd){\displaystyle {\mathfrak {H}}={\begin{pmatrix}a&b\\c&d\end{pmatrix}}}acts on the projective line asz=[z1:z2]w=[w1:w2],{\displaystyle z=[z_{1}:z_{2}]\mapsto w=[w_{1}:w_{2}],}where(w1w2)=(abcd)(z1z2)=(az1+bz2cz1+dz2).{\displaystyle {\begin{pmatrix}w_{1}\\w_{2}\end{pmatrix}}={\begin{pmatrix}a&b\\c&d\end{pmatrix}}{\begin{pmatrix}z_{1}\\z_{2}\end{pmatrix}}={\begin{pmatrix}az_{1}+bz_{2}\\cz_{1}+dz_{2}\end{pmatrix}}.}

The result is thereforew=[w1:w2]=[az1+bz2:cz1+dz2]{\displaystyle w=[w_{1}:w_{2}]=[az_{1}+bz_{2}:cz_{1}+dz_{2}]}

Which, using the above identification, corresponds to the following point on the Riemann sphere :

w=[az1+bz2:cz1+dz2]az1+bz2cz1+dz2=az1z2+bcz1z2+d.{\displaystyle w=[az_{1}+bz_{2}:cz_{1}+dz_{2}]\thicksim {\frac {az_{1}+bz_{2}}{cz_{1}+dz_{2}}}={\frac {a{\frac {z_{1}}{z_{2}}}+b}{c{\frac {z_{1}}{z_{2}}}+d}}.}

Equivalence with a Möbius transformation on the Riemann sphere

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Since the above matrix is invertible if and only if itsdeterminantadbc is not zero, this induces an identification of the action of the group of Möbius transformations with the action ofPGL(2,C) on the complex projective line. In this identification, the above matrixH{\displaystyle {\mathfrak {H}}} corresponds to the Möbius transformationzaz+bcz+d.{\displaystyle z\mapsto {\frac {az+b}{cz+d}}.}

This identification is agroup isomorphism, since the multiplication ofH{\displaystyle {\mathfrak {H}}} by a non zero scalarλ{\displaystyle \lambda } does not change the element ofPGL(2,C), and, as this multiplication consists of multiplying all matrix entries byλ,{\displaystyle \lambda ,} this does not change the corresponding Möbius transformation.

Other groups

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For anyfieldK, one can similarly identify the groupPGL(2,K) of the projective linear automorphisms with the group of fractional linear transformations. This is widely used; for example in the study ofhomographies of thereal line and its applications inoptics.

If one dividesH{\displaystyle {\mathfrak {H}}} by a square root of its determinant, one gets a matrix of determinant one. This induces a surjective group homomorphism from thespecial linear groupSL(2,C) toPGL(2,C), with±I{\displaystyle \pm I} as its kernel.

This allows showing that the Möbius group is a 3-dimensional complexLie group (or a 6-dimensional real Lie group), which is asemisimple and non-compact, and that SL(2,C) is adouble cover ofPSL(2,C). SinceSL(2,C) issimply-connected, it is theuniversal cover of the Möbius group, and thefundamental group of the Möbius group is Z2.

Specifying a transformation by three points

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Given a set of three distinct pointsz1,z2,z3{\displaystyle z_{1},z_{2},z_{3}} on the Riemann sphere and a second set of distinct pointsw1,w2,w3{\displaystyle w_{1},w_{2},w_{3}}, there exists precisely one Möbius transformationf(z){\displaystyle f(z)} withf(zj)=wj{\displaystyle f(z_{j})=w_{j}} forj=1,2,3{\displaystyle j=1,2,3}. (In other words: theaction of the Möbius group on the Riemann sphere issharply 3-transitive.) There are several ways to determinef(z){\displaystyle f(z)} from the given sets of points.

Mapping first to 0, 1,

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It is easy to check that the Möbius transformationf1(z)=(zz1)(z2z3)(zz3)(z2z1){\displaystyle f_{1}(z)={\frac {(z-z_{1})(z_{2}-z_{3})}{(z-z_{3})(z_{2}-z_{1})}}}with matrixH1=(z2z3z1(z2z3)z2z1z3(z2z1)){\displaystyle {\mathfrak {H}}_{1}={\begin{pmatrix}z_{2}-z_{3}&-z_{1}(z_{2}-z_{3})\\z_{2}-z_{1}&-z_{3}(z_{2}-z_{1})\end{pmatrix}}}mapsz1,z2 and z3{\displaystyle z_{1},z_{2}{\text{ and }}z_{3}} to0,1, and {\displaystyle 0,1,\ {\text{and}}\ \infty }, respectively. If one of thezj{\displaystyle z_{j}} is{\displaystyle \infty }, then the proper formula forH1{\displaystyle {\mathfrak {H}}_{1}} is obtained from the above one by first dividing all entries byzj{\displaystyle z_{j}} and then taking the limitzj{\displaystyle z_{j}\to \infty }.

IfH2{\displaystyle {\mathfrak {H}}_{2}} is similarly defined to mapw1,w2,w3{\displaystyle w_{1},w_{2},w_{3}} to0,1, and ,{\displaystyle 0,1,\ {\text{and}}\ \infty ,} then the matrixH{\displaystyle {\mathfrak {H}}} which mapsz1,2,3{\displaystyle z_{1,2,3}} tow1,2,3{\displaystyle w_{1,2,3}} becomesH=H21H1.{\displaystyle {\mathfrak {H}}={\mathfrak {H}}_{2}^{-1}{\mathfrak {H}}_{1}.}

The stabilizer of{0,1,}{\displaystyle \{0,1,\infty \}} (as an unordered set) is a subgroup known as theanharmonic group.

Explicit determinant formula

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The equationw=az+bcz+d{\displaystyle w={\frac {az+b}{cz+d}}}is equivalent to the equation of a standardhyperbolacwzaz+dwb=0{\displaystyle cwz-az+dw-b=0}in the(z,w){\displaystyle (z,w)}-plane. The problem of constructing a Möbius transformationH(z){\displaystyle {\mathfrak {H}}(z)} mapping a triple(z1,z2,z3){\displaystyle (z_{1},z_{2},z_{3})} to another triple(w1,w2,w3){\displaystyle (w_{1},w_{2},w_{3})} is thus equivalent to finding the coefficientsa,b,c,d{\displaystyle a,b,c,d} of the hyperbola passing through the points(zi,wi){\displaystyle (z_{i},w_{i})}. An explicit equation can be found by evaluating thedeterminant|zwzw1z1w1z1w11z2w2z2w21z3w3z3w31|{\displaystyle {\begin{vmatrix}zw&z&w&1\\z_{1}w_{1}&z_{1}&w_{1}&1\\z_{2}w_{2}&z_{2}&w_{2}&1\\z_{3}w_{3}&z_{3}&w_{3}&1\end{vmatrix}}\,}by means of aLaplace expansion along the first row, resulting in explicit formulae,a=z1w1(w2w3)+z2w2(w3w1)+z3w3(w1w2),b=z1w1(z2w3z3w2)+z2w2(z3w1z1w3)+z3w3(z1w2z2w1),c=w1(z3z2)+w2(z1z3)+w3(z2z1),d=z1w1(z2z3)+z2w2(z3z1)+z3w3(z1z2){\displaystyle {\begin{aligned}a&=z_{1}w_{1}(w_{2}-w_{3})+z_{2}w_{2}(w_{3}-w_{1})+z_{3}w_{3}(w_{1}-w_{2}),\\[5mu]b&=z_{1}w_{1}(z_{2}w_{3}-z_{3}w_{2})+z_{2}w_{2}(z_{3}w_{1}-z_{1}w_{3})+z_{3}w_{3}(z_{1}w_{2}-z_{2}w_{1}),\\[5mu]c&=w_{1}(z_{3}-z_{2})+w_{2}(z_{1}-z_{3})+w_{3}(z_{2}-z_{1}),\\[5mu]d&=z_{1}w_{1}(z_{2}-z_{3})+z_{2}w_{2}(z_{3}-z_{1})+z_{3}w_{3}(z_{1}-z_{2})\end{aligned}}}for the coefficientsa,b,c,d{\displaystyle a,b,c,d} of the representing matrixH{\displaystyle {\mathfrak {H}}}. The constructed matrixH{\displaystyle {\mathfrak {H}}} has determinant equal to(z1z2)(z1z3)(z2z3)(w1w2)(w1w3)(w2w3){\displaystyle (z_{1}-z_{2})(z_{1}-z_{3})(z_{2}-z_{3})(w_{1}-w_{2})(w_{1}-w_{3})(w_{2}-w_{3})}, which does not vanish if thezj{\displaystyle z_{j}} resp.wj{\displaystyle w_{j}} are pairwise different thus the Möbius transformation is well-defined. If one of the pointszj{\displaystyle z_{j}} orwj{\displaystyle w_{j}} is{\displaystyle \infty }, then we first divide all four determinants by this variable and then take the limit as the variable approaches{\displaystyle \infty }.

Subgroups of the Möbius group

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If we require the coefficientsa,b,c,d{\displaystyle a,b,c,d} of a Möbius transformation to be real numbers withadbc=1{\displaystyle ad-bc=1}, we obtain a subgroup of the Möbius group denoted asPSL(2,R). This is the group of those Möbius transformations that map theupper half-planeH = {x + iy :y > 0} to itself, and is equal to the group of allbiholomorphic (or equivalently:bijective,conformal and orientation-preserving) mapsHH. If a propermetric is introduced, the upper half-plane becomes a model of thehyperbolic planeH2, thePoincaré half-plane model, andPSL(2,R) is the group of all orientation-preserving isometries ofH2 in this model.

The subgroup of all Möbius transformations that map the open diskD = {z : |z| < 1} to itself consists of all transformations of the formf(z)=eiϕz+bb¯z+1{\displaystyle f(z)=e^{i\phi }{\frac {z+b}{{\bar {b}}z+1}}}withϕ{\displaystyle \phi }R,bC and|b| < 1. This is equal to the group of all biholomorphic (or equivalently: bijective, angle-preserving and orientation-preserving) mapsDD. By introducing a suitable metric, the open disk turns into another model of the hyperbolic plane, thePoincaré disk model, and this group is the group of all orientation-preserving isometries ofH2 in this model.

Since both of the above subgroups serve as isometry groups ofH2, they are isomorphic. A concrete isomorphism is given byconjugation with the transformationf(z)=z+iiz+1{\displaystyle f(z)={\frac {z+i}{iz+1}}}which bijectively maps the open unit disk to the upper half plane.

Alternatively, consider an open disk with radiusr, centered atri. The Poincaré disk model in this disk becomes identical to the upper-half-plane model asr approaches ∞.

Amaximal compact subgroup of the Möbius groupM{\displaystyle {\mathcal {M}}} is given by (Tóth 2002)[5]M0:={zuzv¯vz+u¯:|u|2+|v|2=1},{\displaystyle {\mathcal {M}}_{0}:=\left\{z\mapsto {\frac {uz-{\bar {v}}}{vz+{\bar {u}}}}:|u|^{2}+|v|^{2}=1\right\},}and corresponds under the isomorphismMPSL(2,C){\displaystyle {\mathcal {M}}\cong \operatorname {PSL} (2,\mathbb {C} )} to theprojective special unitary groupPSU(2,C) which is isomorphic to thespecial orthogonal group SO(3) of rotations in three dimensions, and can be interpreted as rotations of the Riemann sphere. Every finite subgroup is conjugate into this maximal compact group, and thus these correspond exactly to the polyhedral groups, thepoint groups in three dimensions.

Icosahedral groups of Möbius transformations were used byFelix Klein to give an analytic solution to thequintic equation in (Klein 1913); a modern exposition is given in (Tóth 2002).[6]

If we require the coefficientsa,b,c,d of a Möbius transformation to beintegers withadbc = 1, we obtain themodular groupPSL(2,Z), a discrete subgroup ofPSL(2,R) important in the study oflattices in the complex plane,elliptic functions andelliptic curves. The discrete subgroups ofPSL(2,R) are known asFuchsian groups; they are important in the study ofRiemann surfaces.

Classification

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A hyperbolic transformation is shown. Pre-images of the unit circle arecircles of Apollonius with distance ratioc/a and foci at −b/a and −d/c .
For the same foci −b/a and −d/c the red circles map to rays through the origin.

In the following discussion we will always assume that the representing matrixH{\displaystyle {\mathfrak {H}}} is normalized such thatdetH=adbc=1{\displaystyle \det {\mathfrak {H}}=ad-bc=1}.

Non-identity Möbius transformations are commonly classified into four types,parabolic,elliptic,hyperbolic andloxodromic, 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 thetracetrH=a+d{\displaystyle \operatorname {tr} {\mathfrak {H}}=a+d}. The trace is invariant underconjugation, that is,trGHG1=trH,{\displaystyle \operatorname {tr} \,{\mathfrak {GHG}}^{-1}=\operatorname {tr} \,{\mathfrak {H}},}and so every member of a conjugacy class will have the same trace. Every Möbius transformation can be written such that its representing matrixH{\displaystyle {\mathfrak {H}}} has determinant one (by multiplying the entries with a suitable scalar). Two Möbius transformationsH,H{\displaystyle {\mathfrak {H}},{\mathfrak {H}}'} (both not equal to the identity transform) withdetH=detH=1{\displaystyle \det {\mathfrak {H}}=\det {\mathfrak {H}}'=1} are conjugate if and only iftr2H=tr2H.{\displaystyle \operatorname {tr} ^{2}{\mathfrak {H}}=\operatorname {tr} ^{2}{\mathfrak {H}}'.}

Parabolic transforms

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A non-identity Möbius transformation defined by a matrixH{\displaystyle {\mathfrak {H}}} of determinant one is said to beparabolic iftr2H=(a+d)2=4{\displaystyle \operatorname {tr} ^{2}{\mathfrak {H}}=(a+d)^{2}=4}(so the trace is plus or minus 2; either can occur for a given transformation sinceH{\displaystyle {\mathfrak {H}}} is determined only up to sign). In fact one of the choices forH{\displaystyle {\mathfrak {H}}} has the samecharacteristic polynomialX2 − 2X + 1 as the identity matrix, and is thereforeunipotent. A Möbius transform is parabolic if and only if it has exactly one fixed point in theextended complex planeC^=C{}{\displaystyle {\widehat {\mathbb {C} }}=\mathbb {C} \cup \{\infty \}}, which happens if and only if it can be defined by a matrixconjugate to(1101){\displaystyle {\begin{pmatrix}1&1\\0&1\end{pmatrix}}}which describes a translation in the complex plane.

The set of all parabolic Möbius transformations with agiven fixed point inC^{\displaystyle {\widehat {\mathbb {C} }}}, together with the identity, forms asubgroup isomorphic to the group of matrices{(1b01)bC};{\displaystyle \left\{{\begin{pmatrix}1&b\\0&1\end{pmatrix}}\mid b\in \mathbb {C} \right\};}this is an example of theunipotent radical of aBorel subgroup (of the Möbius group, or ofSL(2,C) for the matrix group; the notion is defined for anyreductive Lie group).

Characteristic constant

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All non-parabolic transformations have two fixed points and are defined by a matrix conjugate to(λ00λ1){\displaystyle {\begin{pmatrix}\lambda &0\\0&\lambda ^{-1}\end{pmatrix}}}with the complex numberλ not equal to 0, 1 or −1, corresponding to a dilation/rotation through multiplication by the complex numberk =λ2, called thecharacteristic constant ormultiplier of the transformation.

Elliptic transforms

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TheSmith chart, used byelectrical engineers for analyzingtransmission lines, is a visual depiction of the elliptic Möbius transformationΓ = (z − 1)/(z + 1). Each point on the Smith chart simultaneously represents both a value ofz (bottom left), and the corresponding value of Γ (bottom right), for |Γ|<1.

The transformation is said to beelliptic if it can be represented by a matrixH{\displaystyle {\mathfrak {H}}} of determinant 1 such that0tr2H<4.{\displaystyle 0\leq \operatorname {tr} ^{2}{\mathfrak {H}}<4.}

A transform is elliptic if and only if|λ| = 1 andλ ≠ ±1. Writingλ=eiα{\displaystyle \lambda =e^{i\alpha }}, an elliptic transform is conjugate to(cosαsinαsinαcosα){\displaystyle {\begin{pmatrix}\cos \alpha &-\sin \alpha \\\sin \alpha &\cos \alpha \end{pmatrix}}}withα real.

ForanyH{\displaystyle {\mathfrak {H}}} with characteristic constantk, the characteristic constant ofHn{\displaystyle {\mathfrak {H}}^{n}} iskn. Thus, all Möbius transformations of finiteorder are elliptic transformations, namely exactly those whereλ is aroot of unity, or, equivalently, whereα is arational multiple ofπ. The simplest possibility of a fractional multiple meansα =π/2, which is also the unique case oftrH=0{\displaystyle \operatorname {tr} {\mathfrak {H}}=0}, is also denoted as acircular transform; this corresponds geometrically to rotation by 180° about two fixed points. This class is represented in matrix form as:(0110).{\displaystyle {\begin{pmatrix}0&-1\\1&0\end{pmatrix}}.}There are 3 representatives fixing {0, 1, ∞}, which are the three transpositions in the symmetry group of these 3 points:1/z,{\displaystyle 1/z,} which fixes 1 and swaps 0 with (rotation by 180° about the points 1 and −1),1z{\displaystyle 1-z}, which fixes and swaps 0 with 1 (rotation by 180° about the points 1/2 and), andz/(z1){\displaystyle z/(z-1)} which fixes 0 and swaps 1 with (rotation by 180° about the points 0 and 2).

Hyperbolic transforms

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The transform is said to behyperbolic if it can be represented by a matrixH{\displaystyle {\mathfrak {H}}} whose trace isreal withtr2H>4.{\displaystyle \operatorname {tr} ^{2}{\mathfrak {H}}>4.}

A transform is hyperbolic if and only ifλ is real andλ ≠ ±1.

Loxodromic transforms

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The transform is said to beloxodromic iftr2H{\displaystyle \operatorname {tr} ^{2}{\mathfrak {H}}} is not in[0, 4]. A transformation is loxodromic if and only if|λ|1{\displaystyle |\lambda |\neq 1}.

Historically,navigation byloxodrome orrhumb line refers to a path of constantbearing; the resulting path is alogarithmic spiral, similar in shape to the transformations of the complex plane that a loxodromic Möbius transformation makes. See the geometric figures below.

General classification

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TransformationTrace squaredMultipliersClass representative
Circularσ = 0k = −1(i00i){\displaystyle {\begin{pmatrix}i&0\\0&-i\end{pmatrix}}}z ↦ −z
Elliptic0 ≤σ < 4
σ=2+2cos(θ){\displaystyle \sigma =2+2\cos(\theta )}
|k| = 1
k=e±iθ1{\displaystyle k=e^{\pm i\theta }\neq 1}
(eiθ/200eiθ/2){\displaystyle {\begin{pmatrix}e^{i\theta /2}&0\\0&e^{-i\theta /2}\end{pmatrix}}}zez
Parabolicσ = 4k = 1(1a01){\displaystyle {\begin{pmatrix}1&a\\0&1\end{pmatrix}}}zz +a
Hyperbolic4 <σ < ∞
σ=2+2cosh(θ){\displaystyle \sigma =2+2\cosh(\theta )}
kR+{\displaystyle k\in \mathbb {R} ^{+}}
k=e±θ1{\displaystyle k=e^{\pm \theta }\neq 1}
(eθ/200eθ/2){\displaystyle {\begin{pmatrix}e^{\theta /2}&0\\0&e^{-\theta /2}\end{pmatrix}}}zeθz
LoxodromicσC \ [0,4]
σ=(λ+λ1)2{\displaystyle \sigma =(\lambda +\lambda ^{-1})^{2}}
|k|1{\displaystyle |k|\neq 1}
k=λ2,λ2{\displaystyle k=\lambda ^{2},\lambda ^{-2}}
(λ00λ1){\displaystyle {\begin{pmatrix}\lambda &0\\0&\lambda ^{-1}\end{pmatrix}}}zkz

The real case and a note on terminology

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Over the real numbers (if the coefficients must be real), there are no non-hyperbolic loxodromic transformations, and the classification is into elliptic, parabolic, and hyperbolic, as for realconics. The terminology is due to considering half the absolute value of the trace, |tr|/2, as theeccentricity 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 tracesquared 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 theclassification of elements ofSL(2,R) (the 2-fold cover), andanalogous classifications are used elsewhere. Loxodromic transformations are an essentially complex phenomenon, and correspond to complex eccentricities.

Geometric interpretation of the characteristic constant

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The following picture depicts (after stereographic transformation from the sphere to the plane) the two fixed points of a Möbius transformation in the non-parabolic case:

The characteristic constant can be expressed in terms of itslogarithm:eρ+αi=k.{\displaystyle e^{\rho +\alpha i}=k.}When expressed in this way, the real numberρ becomes an expansion factor. It indicates how repulsive the fixed pointγ1 is, and how attractiveγ2 is. The real numberα is a rotation factor, indicating to what extent the transform rotates the plane anti-clockwise aboutγ1 and clockwise about γ2.

Elliptic transformations

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Ifρ = 0, then the fixed points are neither attractive nor repulsive but indifferent, and the transformation is said to beelliptic. 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 theone-parameter subgroup generated by any elliptic Möbius transformation, we obtain a continuous transformation, such that every transformation in the subgroup fixes thesame 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 one-parameter subgroup of elliptic transformations sharing the fixed points 0, ∞, and with the numberα 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 one-parameter subgroup which it generatescontinuously moves points along the family of circular arcs suggested by the pictures.

Hyperbolic transformations

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Ifα is zero (or a multiple of 2π), then the transformation is said to behyperbolic. These transformations tend to move points along circular paths from one fixed point toward the other.

If we take theone-parameter subgroup generated by any hyperbolic Möbius transformation, we obtain a continuous transformation, such that every transformation in the subgroup fixes thesame two points. All other points flow along a certain family of circular arcsaway from the first fixed point andtoward 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 one-parameter subgroup of hyperbolic transformations sharing the fixed points 0, ∞, with the real numberρ 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

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If bothρ andα are nonzero, then the transformation is said to beloxodromic. These transformations tend to move all points in S-shaped paths from one fixed point to the other.

The word "loxodrome" is from the Greek: "λοξος (loxos),slanting + δρόμος (dromos),course". Whensailing on a constantbearing – if you maintain a heading of (say) north-east, you will eventually wind up sailing around thenorth pole in alogarithmic spiral. On themercator 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 ofk. 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 theone-parameter subgroup generated by any loxodromic Möbius transformation, we obtain a continuous transformation, such that every transformation in the subgroup fixes thesame two points. All other points flow along a certain family of curves,away from the first fixed point andtoward 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 thesame axis, will see the appearance of the night sky transform according to the one-parameter subgroup of loxodromic transformations with fixed points 0, ∞, and withρ,α determined respectively by the magnitude of the actual linear and angular velocities.

Stereographic projection

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These images show Möbius transformationsstereographically projected onto theRiemann 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
Elliptic
Hyperbolic
Loxodromic
Fixed points diametrically opposite
Elliptic
Hyperbolic
Loxodromic
Fixed points in an arbitrary location
Elliptic
Hyperbolic
Loxodromic

Iterating a transformation

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See also:Iterated function system

If a transformationH{\displaystyle {\mathfrak {H}}} has fixed pointsγ1,γ2, and characteristic constantk, thenH=Hn{\displaystyle {\mathfrak {H}}'={\mathfrak {H}}^{n}} will haveγ1=γ1,γ2=γ2,k=kn{\displaystyle \gamma _{1}'=\gamma _{1},\gamma _{2}'=\gamma _{2},k'=k^{n}}.

This can be used toiterate 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 ofα is 1/10.

Higher dimensions

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In higher dimensions, aMöbius transformation is ahomeomorphism ofRn¯{\displaystyle {\overline {\mathbb {R} ^{n}}}}, theone-point compactification ofRn{\displaystyle \mathbb {R} ^{n}}, which is a finite composition ofinversions in spheres andreflections inhyperplanes.[7]Liouville's theorem in conformal geometry states that in dimension at least three, allconformal transformations are Möbius transformations. Every Möbius transformation can be put in the formf(x)=b+αA(xa)|xa|ε,{\displaystyle f(x)=b+{\frac {\alpha A(x-a)}{|x-a|^{\varepsilon }}},}wherea,bRn{\displaystyle a,b\in \mathbb {R} ^{n}},αR{\displaystyle \alpha \in \mathbb {R} },A{\displaystyle A} is anorthogonal matrix, andε{\displaystyle \varepsilon } is 0 or 2. The group of Möbius transformations is also called theMöbius group.[8]

The orientation-preserving Möbius transformations form the connected component of the identity in the Möbius group. In dimensionn = 2, the orientation-preserving Möbius transformations are exactly the maps of the Riemann sphere covered here. The orientation-reversing ones are obtained from these by complex conjugation.[9]

The domain of Möbius transformations, i.e.Rn¯{\displaystyle {\overline {\mathbb {R} ^{n}}}}, is homeomorphic to then-dimensional sphereSn{\displaystyle S^{n}}. The canonical isomorphism between these two spaces is theCayley transform, which is itself a Möbius transformation ofRn+1¯{\displaystyle {\overline {\mathbb {R} ^{n+1}}}}. This identification means that Möbius transformations can also be thought of as conformal isomorphisms ofSn{\displaystyle S^{n}}. Then-sphere, together with action of the Möbius group, is a geometric structure (in the sense of Klein'sErlangen program) calledMöbius geometry.[10]

Applications

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Lorentz transformation

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Main article:Lorentz transformation

An isomorphism of the Möbius group with theLorentz group was noted by several authors: Based on previous work ofFelix Klein (1893, 1897)[11] onautomorphic functions related to hyperbolic geometry and Möbius geometry,Gustav Herglotz (1909)[12] showed thathyperbolic motions (i.e.isometricautomorphisms of ahyperbolic space) transforming theunit sphere into itself correspond to Lorentz transformations, by which Herglotz was able to classify the one-parameter Lorentz transformations into loxodromic, elliptic, hyperbolic, and parabolic groups. Other authors includeEmil Artin (1957),[13]H. S. M. Coxeter (1965),[14] andRoger Penrose,Wolfgang Rindler (1984),[15]Tristan Needham (1997)[16] and W. M. Olivia (2002).[17]

Minkowski space consists of the four-dimensional real coordinate spaceR4 consisting of the space of ordered quadruples(x0,x1,x2,x3) of real numbers, together with aquadratic formQ(x0,x1,x2,x3)=x02x12x22x32.{\displaystyle Q(x_{0},x_{1},x_{2},x_{3})=x_{0}^{2}-x_{1}^{2}-x_{2}^{2}-x_{3}^{2}.}

Borrowing terminology fromspecial relativity, points withQ > 0 are consideredtimelike; in addition, ifx0 > 0, then the point is calledfuture-pointing. Points withQ < 0 are calledspacelike. Thenull coneS consists of those points whereQ = 0; thefuture null coneN+ are those points on the null cone withx0 > 0. Thecelestial sphere is then identified with the collection of rays inN+ whose initial point is the origin ofR4. The collection oflinear transformations onR4 with positivedeterminant preserving the quadratic formQ and preserving the time direction form therestricted Lorentz groupSO+(1, 3).

In connection with the geometry of the celestial sphere, the group of transformationsSO+(1, 3) is identified with the groupPSL(2,C) of Möbius transformations of the sphere. To each(x0,x1,x2,x3) ∈R4, associate thehermitian matrixX=[x0+x1x2+ix3x2ix3x0x1].{\displaystyle X={\begin{bmatrix}x_{0}+x_{1}&x_{2}+ix_{3}\\x_{2}-ix_{3}&x_{0}-x_{1}\end{bmatrix}}.}

Thedeterminant of the matrixX is equal toQ(x0,x1,x2,x3). Thespecial linear group acts on the space of such matrices via

XAXA{\displaystyle X\mapsto AXA^{*}}1

for eachA ∈ SL(2,C), and this action ofSL(2,C) preserves the determinant ofX becausedetA = 1. Since the determinant ofX is identified with the quadratic formQ,SL(2,C) acts by Lorentz transformations. On dimensional grounds,SL(2,C) covers a neighborhood of the identity ofSO(1, 3). SinceSL(2,C) is connected, it covers the entire restricted Lorentz groupSO+(1, 3). Furthermore, since thekernel of the action (1) is the subgroup {±I}, then passing to thequotient group gives thegroup isomorphism

PSL(2,C)SO+(1,3).{\displaystyle \operatorname {PSL} (2,\mathbb {C} )\cong \operatorname {SO} ^{+}(1,3).}2

Focusing now attention on the case when(x0,x1,x2,x3) is null, the matrixX has zero determinant, and therefore splits as theouter product of a complex two-vectorξ with its complex conjugate:

X=ξξ¯T=ξξ.{\displaystyle X=\xi {\bar {\xi }}^{\text{T}}=\xi \xi ^{*}.}3

The two-component vectorξ is acted upon bySL(2,C) in a manner compatible with (1). It is now clear that the kernel of the representation ofSL(2,C) on hermitian matrices is {±I}.

The action ofPSL(2,C) on the celestial sphere may also be described geometrically usingstereographic projection. Consider first the hyperplane inR4 given byx0 = 1. The celestial sphere may be identified with the sphereS+ of intersection of the hyperplane with the future null coneN+. The stereographic projection from the north pole(1, 0, 0, 1) of this sphere onto the planex3 = 0 takes a point with coordinates(1,x1,x2,x3) withx12+x22+x32=1{\displaystyle x_{1}^{2}+x_{2}^{2}+x_{3}^{2}=1}to the point(1,x11x3,x21x3,0).{\displaystyle \left(1,{\frac {x_{1}}{1-x_{3}}},{\frac {x_{2}}{1-x_{3}}},0\right).}

Introducing thecomplex coordinateζ=x1+ix21x3,{\displaystyle \zeta ={\frac {x_{1}+ix_{2}}{1-x_{3}}},}the inverse stereographic projection gives the following formula for a point(x1,x2,x3) onS+:

x1=ζ+ζ¯ζζ¯+1x2=ζζ¯i(ζζ¯+1)x3=ζζ¯1ζζ¯+1.{\displaystyle {\begin{aligned}x_{1}&={\frac {\zeta +{\bar {\zeta }}}{\zeta {\bar {\zeta }}+1}}\\x_{2}&={\frac {\zeta -{\bar {\zeta }}}{i(\zeta {\bar {\zeta }}+1)}}\\x_{3}&={\frac {\zeta {\bar {\zeta }}-1}{\zeta {\bar {\zeta }}+1}}.\end{aligned}}}4

The action ofSO+(1, 3) on the points ofN+ does not preserve the hyperplaneS+, but acting on points inS+ and then rescaling so that the result is again inS+ gives an action ofSO+(1, 3) on the sphere which goes over to an action on the complex variableζ. 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 ofζ variable goes over to a unique Lorentz transformation onN+, 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 variableζ =z:w as a ratio of a pair of homogeneous coordinates for the complex projective lineCP1. The stereographic projection goes over to a transformation fromC2 − {0} toN+ which is homogeneous of degree two with respect to real scalings

(z,w)(x0,x1,x2,x3)=(zz¯+ww¯,zz¯ww¯,zw¯+wz¯,i1(zw¯wz¯)){\displaystyle (z,w)\mapsto (x_{0},x_{1},x_{2},x_{3})=(z{\bar {z}}+w{\bar {w}},z{\bar {z}}-w{\bar {w}},z{\bar {w}}+w{\bar {z}},i^{-1}(z{\bar {w}}-w{\bar {z}}))}5

which agrees with (4) upon restriction to scales in whichzz¯+ww¯=1.{\displaystyle z{\bar {z}}+w{\bar {w}}=1.} The components of (5) are precisely those obtained from the outer product[x0+x1x2+ix3x2ix3x0x1]=2[zw][z¯w¯].{\displaystyle {\begin{bmatrix}x_{0}+x_{1}&x_{2}+ix_{3}\\x_{2}-ix_{3}&x_{0}-x_{1}\end{bmatrix}}=2{\begin{bmatrix}z\\w\end{bmatrix}}{\begin{bmatrix}{\bar {z}}&{\bar {w}}\end{bmatrix}}.}

In summary, the action of the restricted Lorentz group SO+(1,3) agrees with that of the Möbius groupPSL(2,C). This motivates the following definition. In dimensionn ≥ 2, theMöbius group Möb(n) is the group of all orientation-preservingconformalisometries of the round sphereSn to itself. By realizing the conformal sphere as the space of future-pointing rays of the null cone in the Minkowski spaceR1,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 formQ(x1, x2, x3 x4)=x12+x22+x32x42{\displaystyle Q(x_{1},\ x_{2},\ x_{3}\ x_{4})=x_{1}^{2}+x_{2}^{2}+x_{3}^{2}-x_{4}^{2}}.

He identified the Lorentz group with transformations for which {x | Q(x) = −1} isstable. Then he interpreted thex's ashomogeneous coordinates and {x | Q(x) = 0}, thenull cone, as theCayley absolute for a hyperbolic space of points {x | Q(x) < 0}. Next, Coxeter introduced the variablesξ=x1x4, η=x2x4, ζ=x3x4{\displaystyle \xi ={\frac {x_{1}}{x_{4}}},\ \eta ={\frac {x_{2}}{x_{4}}},\ \zeta ={\frac {x_{3}}{x_{4}}}}so that the Lorentz-invariant quadric corresponds to the sphereξ2+η2+ζ2=1{\displaystyle \xi ^{2}+\eta ^{2}+\zeta ^{2}=1}. Coxeter notes thatFelix Klein also wrote of this correspondence, applying stereographic projection from(0, 0, 1) to the complex planez=ξ+iη1ζ.{\textstyle z={\frac {\xi +i\eta }{1-\zeta }}.} Coxeter used the fact that circles of the inversive plane represent planes of hyperbolic space, and the general homography is the product of inversions in two or four circles, corresponding to the general hyperbolic displacement which is the product of inversions in two or four planes.

Hyperbolic space

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As seen above, the Möbius groupPSL(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 whereQ = 1 in the positive light cone, which form a model ofhyperbolic 3-spaceH3, we see that the Möbius group acts onH3 as a group of orientation-preserving isometries. In fact, the Möbius group is equal to the group of orientation-preserving isometries of hyperbolic 3-space. If we use thePoincaré ball model, identifying the unit ball inR3 withH3, then we can think of the Riemann sphere as the "conformal boundary" ofH3. Every orientation-preserving isometry ofH3 gives rise to a Möbius transformation on the Riemann sphere and vice versa.

See also

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Notes

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  1. ^Geometrically this map is thestereographic projection of a rotation by 90° around ±i with period 4, which takes0110.{\displaystyle 0\mapsto 1\mapsto \infty \mapsto -1\mapsto 0.}

References

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Specific

  1. ^Arnold & Rogness 2008, Theorem 1.
  2. ^Needham, Tristan (2021).Differential Geometry and Forms; A Mathematical Drama in Five Acts. Princeton University Press. p. 77, footnote 16.ISBN 9780691203690.
  3. ^Olsen, John,The Geometry of Mobius Transformations(PDF)
  4. ^Weisstein, Eric W."Symmetric Points".MathWorld.
  5. ^Tóth 2002, Section 1.2, Rotations and Möbius Transformations,p. 22.
  6. ^Tóth 2002, Section 1.6, Additional Topic: Klein's Theory of the Icosahedron,p. 66.
  7. ^Iwaniec, Tadeusz and Martin, Gaven, The Liouville theorem, Analysis and topology, 339–361, World Sci. Publ., River Edge, NJ, 1998
  8. ^J.B. Wilker (1981) "Inversive Geometry",MR0661793
  9. ^Berger, Marcel (1987),Geometry II, Springer (Universitext), p. 18.10
  10. ^Akivis, Maks; Goldberg, Vladislav (1992),Conformal differential geometry and its generalizations, Wiley-Interscience
  11. ^Felix Klein (1893),Nicht-Euklidische Geometrie, Autogr. Vorl., Göttingen;
    Robert Fricke & Felix Klein (1897),Autormorphe Funktionen I., Teubner, Leipzig
  12. ^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
  13. ^Emil Artin (1957)Geometric Algebra, page 204
  14. ^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
  15. ^Penrose & Rindler 1984, pp. 8–31.
  16. ^Needham, Tristan (1997).Visual Complex Analysis(PDF). Oxford: Oxford University Press. pp. 122–124.
  17. ^Olivia, Waldyr Muniz (2002). "Appendix B: Möbius transformations and the Lorentz group".Geometric Mechanics. Springer. pp. 195–221.ISBN 3-540-44242-1.MR 1990795.

General

Further reading

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External links

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