In geometry, the cross-ratio, also called the double ratio and anharmonic ratio, is a number associated with a list of four collinear points, particularly points on a projective line. Given four points,,, on a line, their cross ratio is defined as
(A,B;C,D)=
AC ⋅ BD | |
BC ⋅ AD |
where an orientation of the line determines the sign of each distance and the distance is measured as projected into Euclidean space. (If one of the four points is the line's point at infinity, then the two distances involving that point are dropped from the formula.)The point is the harmonic conjugate of with respect to and precisely if the cross-ratio of the quadruple is, called the harmonic ratio. The cross-ratio can therefore be regarded as measuring the quadruple's deviation from this ratio; hence the name anharmonic ratio.
The cross-ratio is preserved by linear fractional transformations. It is essentially the only projective invariant of a quadruple of collinear points; this underlies its importance for projective geometry.
The cross-ratio had been defined in deep antiquity, possibly already by Euclid, and was considered by Pappus, who noted its key invariance property. It was extensively studied in the 19th century.[1]
Variants of this concept exist for a quadruple of concurrent lines on the projective plane and a quadruple of points on the Riemann sphere.In the Cayley–Klein model of hyperbolic geometry, the distance between points is expressed in terms of a certain cross-ratio.
Pappus of Alexandria made implicit use of concepts equivalent to the cross-ratio in his Collection: Book VII. Early users of Pappus included Isaac Newton, Michel Chasles, and Robert Simson. In 1986 Alexander Jones made a translation of the original by Pappus, then wrote a commentary on how the lemmas of Pappus relate to modern terminology.[2]
Modern use of the cross ratio in projective geometry began with Lazare Carnot in 1803 with his book Géométrie de Position.[3] Chasles coined the French term French: rapport anharmonique [anharmonic ratio] in 1837.[4] German geometers call it German: das Doppelverhältnis [double ratio].
Carl von Staudt was unsatisfied with past definitions of the cross-ratio relying on algebraic manipulation of Euclidean distances rather than being based purely on synthetic projective geometry concepts. In 1847, von Staudt demonstrated that the algebraic structure is implicit in projective geometry, by creating an algebra based on construction of the projective harmonic conjugate, which he called a throw (German: Wurf): given three points on a line, the harmonic conjugate is a fourth point that makes the cross ratio equal to . His algebra of throws provides an approach to numerical propositions, usually taken as axioms, but proven in projective geometry.[5]
The English term "cross-ratio" was introduced in 1878 by William Kingdon Clifford.[6]
If,,, and are four points on an oriented affine line, their cross ratio is:
(A,B;C,D)=
AC:BC | |
AD:BD |
,
with the notation
WX:YZ
If the displacements themselves are taken to be signed real numbers, then the cross ratio between points can be written
(A,B;C,D)=
AC | |
BC |
/
AD | |
BD |
=
AC ⋅ BD | |
BC ⋅ AD |
.
If
\widehat\R=\R\cup\{infty\}
x1,x2,x3,x4
\widehat\R
(x1,x2;x3,x4) =
x3-x1 | |
x3-x2 |
/
x4-x1 | |
x4-x2 |
=
(x3-x1)(x4-x2) | |
(x3-x2)(x4-x1) |
.
When one of
x1,x2,x3,x4
(infty,x2;x3,x4) =
(x3-infty)(x4-x2) | |
(x3-x2)(x4-infty) |
=
(x4-x2) | |
(x3-x2) |
.
The same formulas can be applied to four distinct complex numbers or, more generally, to elements of any field, and can also be projectively extended as above to the case when one of them is
infty=\tfrac10.
The cross ratio of the four collinear points,,, and can be written as
(A,B;C,D)=
AC:CB | |
AD:DB |
Four points can be ordered in ways, but there are only six ways for partitioning them into two unordered pairs. Thus, four points can have only six different cross-ratios, which are related as:
\begin{align} &(A,B;C,D)=(B,A;D,C)=(C,D;A,B)=(D,C;B,A)=λ,\vphantom{
11} | |
\\[4mu] & |
(A,B;D,C)=(B,A;C,D)=(C,D;B,A)=(D,C;A,B)=
1 | |
λ, |
\\[4mu] &(A,C;B,D)=(B,D;A,C)=(C,A;D,B)=(D,B;C,A)=1-λ,\vphantom{
11} | |
\\[4mu] & |
(A,C;D,B)=(B,D;C,A)=(C,A;B,D)=(D,B;A,C)=
1 | |
1-λ |
,\\[4mu] &(A,D;B,C)=(B,C;A,D)=(C,B;D,A)=(D,A;C,B)=
λ-1 | |
λ, |
\\[4mu] &(A,D;C,B)=(B,C;D,A)=(C,B;A,D)=(D,A;B,C)=
λ | |
λ-1 |
. \end{align}
The cross-ratio is a projective invariant in the sense that it is preserved by the projective transformations of a projective line.
In particular, if four points lie on a straight line in then their cross-ratio is a well-defined quantity, because any choice of the origin and even of the scale on the line will yield the same value of the cross-ratio.
Furthermore, let be four distinct lines in the plane passing through the same point . Then any line not passing through intersects these lines in four distinct points (if is parallel to then the corresponding intersection point is "at infinity"). It turns out that the cross-ratio of these points (taken in a fixed order) does not depend on the choice of a line , and hence it is an invariant of the 4-tuple of lines
This can be understood as follows: if and are two lines not passing through then the perspective transformation from to with the center is a projective transformation that takes the quadruple of points on into the quadruple of points on .
Therefore, the invariance of the cross-ratio under projective automorphisms of the line implies (in fact, is equivalent to) the independence of the cross-ratio of the four collinear points on the lines from the choice of the line that contains them.
If four collinear points are represented in homogeneous coordinates by vectors
\alpha,\beta,\gamma,\delta
\gamma=a\alpha+b\beta
\delta=c\alpha+d\beta
(b/a)/(d/c)
C
GC
G=\operatorname{PGL}(3,R)
C
GC
Explicitly, let the conic be the unit circle. For any two points and, inside the unit circle . If the line connecting them intersects the circle in two points, and and the points are, in order, . Then the hyperbolic distance between and in the Cayley–Klein model of the hyperbolic plane can be expressed as
d | ||||
|
\left|log
|XQ||PY| | |
|XP||QY| |
\right|
(the factor one half is needed to make the curvature). Since the cross-ratio is invariant under projective transformations, it follows that the hyperbolic distance is invariant under the projective transformations that preserve the conic .
Conversely, the group acts transitively on the set of pairs of points in the unit disk at a fixed hyperbolic distance.
Later, partly through the influence of Henri Poincaré, the cross ratio of four complex numbers on a circle was used for hyperbolic metrics. Being on a circle means the four points are the image of four real points under a Möbius transformation, and hence the cross ratio is a real number. The Poincaré half-plane model and Poincaré disk model are two models of hyperbolic geometry in the complex projective line.
These models are instances of Cayley–Klein metrics.
The cross-ratio may be defined by any of these four expressions:
(A,B;C,D)=(B,A;D,C)=(C,D;A,B)=(D,C;B,A).
These differ by the following permutations of the variables (in cycle notation):
1, (AB)(CD), (AC)(BD), (AD)(BC).
S4/K
S4/K
Thus, the other permutations of the four variables alter the cross-ratio to give the following six values, which are the orbit of the six-element group
S4/K\congS3
\begin{align} (A,B;C,D)&=λ&(A,B;D,C)&=
1 | |
λ, |
\\[4mu] (A,C;D,B)&=
1 | |
1-λ |
&(A,C;B,D)&=1-λ,\\[4mu] (A,D;C,B)&=
λ | |
λ-1 |
&(A,D;B,C)&=
λ-1 | |
λ. \end{align} |
As functions of
λ,
1-λ
-1,
2,
x2-x+1
e\pm
S3\toS2
Further, the fixed points of the individual -cycles are, respectively,
-1,
2,
The anharmonic group is generated by and Its action on
\{0,1,infty\}
S3 ≈ PGL(2,Z2)
-1=[-1:1]
S4 ≈ PGL(2,Z3)
S3\hookrightarrowS4
-1
For certain values of
λ
λ
The first set of fixed points is
\{0,1,infty\}.
\begin{align} (Z,B;Z,D)&=(A,Z;C,Z)=0,\\[4mu] (Z,Z;C,D)&=(A,B;Z,Z)=1,\\[4mu] (Z,B;C,Z)&=(A,Z;Z,D)=infty. \end{align}
The second set of fixed points is This situation is what is classically called the , and arises in projective harmonic conjugates. In the real case, there are no other exceptional orbits.
In the complex case, the most symmetric cross-ratio occurs when
λ=e\pm
See main article: Möbius transformation.
The cross-ratio is invariant under the projective transformations of the line. In the case of a complex projective line, or the Riemann sphere, these transformations are known as Möbius transformations. A general Möbius transformation has the form
f(z)=
az+b | |
cz+d |
, wherea,b,c,d\inCandad-bc\ne0.
These transformations form a group acting on the Riemann sphere, the Möbius group.
The projective invariance of the cross-ratio means that
(f(z1),f(z2);f(z3),f(z4))=(z1,z2;z3,z4).
The cross-ratio is real if and only if the four points are either collinear or concyclic, reflecting the fact that every Möbius transformation maps generalized circles to generalized circles.
The action of the Möbius group is simply transitive on the set of triples of distinct points of the Riemann sphere: given any ordered triple of distinct points,
(z2,z3,z4)
f(z)
(0,1,infty)
(z,z2;z3,z4)
(f(z),1;0,infty)
f(z)
f(z)=(z,z2;z3,z4).
An alternative explanation for the invariance of the cross-ratio is based on the fact that the group of projective transformations of a line is generated by the translations, the homotheties, and the multiplicative inversion. The differences
zj-zk
z\mapstoz+a
where
a
F
z\mapstobz
for a non-zero constant
b
F
In order to obtain a well-defined inversion mapping
T:z\mapstoz-1,
the affine line needs to be augmented by the point at infinity, denoted
infty
P1(F)
f:F\toF
P1(F)
T
0
infty
T
P1(F)
F=C
T
P1(F)
If we write the complex points as vectors
\vec{xn}=[\Re(zn),\Im(z
T | |
n)] |
xnm=xn-xm
(a,b)
a
b
C1=
(x12,x14)(x23,x34)-(x12,x34)(x14,x23)+(x12,x23)(x14,x34) | |
|x23|2|x14|2 |
This is an invariant of the 2-dimensional special conformal transformation such as inversion
x\mu →
x\mu | |
|x|2 |
The imaginary part must make use of the 2-dimensional cross product
a x b=[a,b]=a2b1-a1b2
C2=
(x12,x14)[x34,x23]-(x43,x23)[x12,x34] | |
|x23|2|x14|2 |
The concept of cross ratio only depends on the ring operations of addition, multiplication, and inversion (though inversion of a given element is not certain in a ring). One approach to cross ratio interprets it as a homography that takes three designated points to and . Under restrictions having to do with inverses, it is possible to generate such a mapping with ring operations in the projective line over a ring. The cross ratio of four points is the evaluation of this homography at the fourth point.
The theory takes on a differential calculus aspect as the four points are brought into proximity. This leads to the theory of the Schwarzian derivative, and more generally of projective connections.
The cross-ratio does not generalize in a simple manner to higher dimensions, due to other geometric properties of configurations of points, notably collinearity – configuration spaces are more complicated, and distinct -tuples of points are not in general position.
While the projective linear group of the projective line is 3-transitive (any three distinct points can be mapped to any other three points), and indeed simply 3-transitive (there is a unique projective map taking any triple to another triple), with the cross ratio thus being the unique projective invariant of a set of four points, there are basic geometric invariants in higher dimension. The projective linear group of -space
Pn=P(Kn+1)
PGL(n,K)=P(GL(n+1,K)),
Collinearity is not the only geometric property of configurations of points that must be maintained – for example, five points determine a conic, but six general points do not lie on a conic, so whether any 6-tuple of points lies on a conic is also a projective invariant. One can study orbits of points in general position – in the line "general position" is equivalent to being distinct, while in higher dimensions it requires geometric considerations, as discussed – but, as the above indicates, this is more complicated and less informative.
However, a generalization to Riemann surfaces of positive genus exists, using the Abel–Jacobi map and theta functions.
. Lazare Carnot . 1803 . Géométrie de Position. Crapelet .