This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

footnotetext: File: main.tex, printed: 2025-2-14, 16.06

Collinearity of points on Poincaré unit disk and Riemann sphere

Masayo Fujimura Oona Rainio  and  Matti Vuorinen
Abstract.

We study certain points significant for the hyperbolic geometry of the unit disk. We give explicit formulas for the intersection points of the Euclidean lines and the stereographic projections of great circles of the Riemann sphere passing through these points. We prove several results related to collinearity of these intersection points, offer new ways to find the hyperbolic midpoint, and represent a formula for the chordal midpoint. The proofs utilize Gröbner bases from computer algebra for the solution of polynomial equations.

Key words and phrases:
Chordal metric, elliptic geometry, Gröbner bases, hyperbolic geometry, stereographic projection
2010 Mathematics Subject Classification:
Primary 51M10, Secondary 51M09

Author information.
Masayo Fujimura1, email: [email protected], ORCID: 0000-0002-5837-8167
Oona Rainio2, email: [email protected], ORCID: 0000-0002-7775-7656
Matti Vuorinen2, email: [email protected], ORCID: 0000-0002-1734-8228
1: Department of Mathematics, National Defense Academy of Japan, Yokosuka, Japan
2: Department of Mathematics and Statistics, University of Turku, FI-20014 Turku, Finland
Funding. The first author was partially supported by JSPS KAKENHI (Grant number: JP19K03531) and the second author was supported by Finnish Culture Foundation and Magnus Ehrnrooth Foundation.
Data availability statement. Not applicable, no new data was generated.
Conflict of interest statement. There is no conflict of interest.
Acknowledgements. We are grateful to the referees for their careful work and, in particular, the second part of Remark 3.9 was suggested by one of the referees. We are thankful to Heikki Ruskeepää for his help with Figure 7.

1. Introduction

In recent decades, hyperbolic geometry and its many generalizations have found numerous applications to geometric function theory and analysis in Euclidean spaces n,n2,\mathbb{R}^{n},n\geq 2, and in metric spaces [11]. One of the reasons why the hyperbolic geometry is better suited to function theoretic applications than the Euclidean metric is its natural invariance properties under conformal mappings and Möbius transformations. Conformal invariants play an important role in geometric function theory and potential theory.

Introduction to hyperbolic geometry is given for instance in [4, 5, 15, 16]. Many classical facts of Euclidean geometry have their counterparts in the hyperbolic geometry, usually in substantially different form, for instance the sum of angles of a triangle is smaller than π.\pi. A systematic compilation of trigonometric formulas for the three geometries: Euclidean, hyperbolic, and spherical geometries can be found in [13]. Yet it is difficult to find explicit formulas even for simple geometric constructions such as the point of intersection of two hyperbolic lines, the hyperbolic midpoint of two points or the distance of a point from a hyperbolic line. See also [7, 12].

For any two distinct arbitrary points in the unit disk non-collinear with the origin, we can create a group of six points by including the original points, the end points of the hyperbolic line passing through the two points, and their image points after an inversion in the unit circle. With these six points, we can define several intersection points by using such Euclidean lines that pass through certain pair of points chosen among them. In the article [19], it was proven that five of these intersection points occur on the Euclidean line passing the origin and the hyperbolic midpoint of the original two points in the unit disk. An explicit formula for this hyperbolic midpoint, recently found in [21], see Theorem 2.16 below, has an important role in our work.

We continue here the earlier work by finding explicit formulas for the five collinear intersection points. This problem is difficult to solve either by hand calculations or by using symbolic computation systems alone, but a combination of these two methods produces results when applied correctly. During the course of this work, we have used a symbolic computation program called Risa/Asir [14] to perform substitution calculations and reduction of fractions so that the resulting formulas are simple enough to be of use. These formulas of the intersection points are summarized in Table 1 in Section 3, which can be understood better by looking at the related geometry shown in Figure 1. We also studied the same problem in the spherical geometry by computing the similar formulas for the stereographic projections of intersection points of the great circle that pass through the same points used to define Euclidean lines. These intersection points are also collinear, as proven in Theorem 4.2, and their definitions and formulas are presented in Figure 2 and Table 2.

The structure of this article is as follows. In Section 3, we give explicit formulas for the intersection points defined with Euclidean lines. In Section 4, we study the stereographic projections of intersection points of the great circles and prove that they are collinear not only with each other but also the earlier intersection points. In Section 5, we present several results related to the hyperbolic midpoint and also give a formula for the chordal midpoint of two points in the unit disk. We also formulate a conjecture about hyperbolic distances of certain intersection points.

2. Preliminaries

Define the complex conjugate of the point zz in the complex plane \mathbb{C} as z¯=Re(z)Im(z)i\overline{z}={\rm Re}(z)-{\rm Im}(z)i. Denote the nn-dimensional unit ball by 𝔹n\mathbb{B}^{n} and the unit sphere by Sn1S^{n-1}. The Euclidean line L[a,b]L[a,b] passing through a,ba,b (aba\neq b) is given by

(2.1) (a¯b¯)z(ab)z¯=a¯bab¯.(\overline{a}-\overline{b})z-(a-b)\overline{z}=\overline{a}b-a\overline{b}.

The reflection of a point xx in the line L[a,b]L[a,b] is given by

(2.2) w(x)=aba¯b¯x¯ab¯a¯ba¯b¯.w(x)=\frac{a-b}{\overline{a}-\overline{b}}\,\overline{x}-\frac{a\overline{b}-\overline{a}b}{\overline{a}-\overline{b}}.

If the two lines L[a,b]L[a,b] and L[c,d]L[c,d] are non-parallel, their unique intersection point is given by

(2.3) LIS[a,b,c,d]=(a¯bab¯)(cd)(c¯dcd¯)(ab)(a¯b¯)(cd)(c¯d¯)(ab).{\rm LIS}[a,b,c,d]=\frac{(\overline{a}b-a\overline{b})(c-d)-(\overline{c}d-c\overline{d})(a-b)}{(\overline{a}-\overline{b})(c-d)-(\overline{c}-\overline{d})(a-b)}.

This formula can be found in Exercise 4.3(1) on p. 57 and the solution on p. 373 of [11].

Proposition 2.4.

Let a,ba,b\in\mathbb{C} with |a||b|,|a||b|1.|a|\neq|b|,|a||b|\neq 1. Then

(1)\displaystyle(1) LIS[a,b,1/a¯,1/b¯]=b(1+|a|2)a(1+|b|2)|a|2|b|2,\displaystyle\quad\quad{\rm LIS}[a,b,-1/\overline{a},-1/\overline{b}]=\frac{b(1+|a|^{2})-a(1+|b|^{2})}{|a|^{2}-|b|^{2}},
(2)\displaystyle(2) LIS[a,b,1/a¯,1/b¯]=a(1|b|2)b(1|a|2)|a|2|b|2,\displaystyle\quad\quad{\rm LIS}[a,b,1/\overline{a},1/\overline{b}]=\frac{a(1-|b|^{2})-b(1-|a|^{2})}{|a|^{2}-|b|^{2}},
(3)\displaystyle(3) LIS[a,1/b¯,b,1/a¯]=a(1|b|2)+b(1|a|2)1|a|2|b|2,\displaystyle\quad\quad{\rm LIS}[a,1/\overline{b},b,1/\overline{a}]=\frac{a(1-|b|^{2})+b(1-|a|^{2})}{1-|a|^{2}|b|^{2}}\,,
(4)\displaystyle(4) LIS[a,1/b¯,b,1/a¯]=a(1+|b|2)+b(1+|a|2)1|a|2|b|2.\displaystyle\quad\quad{\rm LIS}[a,-1/\overline{b},b,-1/\overline{a}]=\frac{a(1+|b|^{2})+b(1+|a|^{2})}{1-|a|^{2}|b|^{2}}\,.
Proof.

The proof follows from (2.3). ∎

Proposition 2.5.

Let a,b𝔹2a,b\in\mathbb{B}^{2} be points non-collinear with 0 and c=LIS[a,b,0,i(ab)].c={\rm LIS}[a,b,0,i(a-b)]. Then L[a,b]S1={a1,b1}L[a,b]\cap S^{1}=\{a_{1},b_{1}\} where

a1=cic|c|1|c|2,b1=c+ic|c|1|c|2,a_{1}=c-i\frac{c}{|c|}\sqrt{1-|c|^{2}},\quad b_{1}=c+i\frac{c}{|c|}\sqrt{1-|c|^{2}},

and a1,a,b,b1a_{1},a,b,b_{1} are ordered in such a way that |a1a|<|a1b|.|a_{1}-a|<|a_{1}-b|.

Proof.

The proof follows from (2.3). ∎

Proposition 2.6.

[15, 4., p.13] If a,b,c,da,b,c,d are four distinct complex points on the unit circle S1S^{1}, then the complex conjugate f¯\overline{f} of the intersection point ff of the lines L[a,c]L[a,c] and L[b,d]L[b,d] is

f¯=a+cbdacbd,\displaystyle\overline{f}=\frac{a+c-b-d}{ac-bd},

assuming that these two lines intersect.

Proof.

Because z¯=1/z\overline{z}=1/z for z{a,b,c,d}z\in\{a,b,c,d\}, the proof follows from (2.3). ∎

Let C[a,b,c]C[a,b,c] be the circle through distinct non-collinear points a,b,c.\,a,\,b,\,c\,. The formula (2.3) gives easily the formula for the center m(a,b,c)m(a,b,c) of C[a,b,c].C[a,b,c]\,. For instance, we can find two points on the bisecting normal to the side [a,b][a,b] and another two points on the bisecting normal to the side [a,c][a,c] and then apply (2.3) to get m(a,b,c).m(a,b,c)\,. In this way we see that the center m(a,b,c)m(a,b,c) of C[a,b,c]C[a,b,c] is

(2.7) m(a,b,c)=|a|2(bc)+|b|2(ca)+|c|2(ab)a(c¯b¯)+b(a¯c¯)+c(b¯a¯).m(a,b,c)=\frac{|a|^{2}(b-c)+|b|^{2}(c-a)+|c|^{2}(a-b)}{a(\overline{c}-\overline{b})+b(\overline{a}-\overline{c})+c(\overline{b}-\overline{a})}\,.

The following special cases of (2.7) will be very useful:

(2.8) {m(a,1/a¯,b)=(a+b+ab(a¯b¯))/d;d=ba¯ab¯,m(a,1/a¯,b)=(ab+ab(a¯b¯))/d.\begin{cases}{\displaystyle{m(a,1/\overline{a},b)=(-a+b+ab(\overline{a}-\overline{b}))/d}}\,;\quad d=b\overline{a}-a\overline{b},&\\ {\displaystyle{m(a,-1/\overline{a},b)=(a-b+ab(\overline{a}-\overline{b}))/d\,.}}&\end{cases}

A Möbius transformation is a mapping of the form

zaz+bcz+d,a,b,c,d,z,adbc0.z\mapsto\frac{az+b}{cz+d}\,,\quad a,b,c,d,z\in{\mathbb{C}}\,,\quad ad-bc\neq 0\,.

The most important feature of Möbius transformations is that they always preserve the angle magnitude and, because of this, they map every Euclidean line or circle onto either a line or a circle. The special Möbius transformation

(2.9) Ta(z)=za1a¯z,a𝔹2{0},T_{a}(z)=\frac{z-a}{1-\overline{a}z}\,,\quad a\in\mathbb{B}^{2}\setminus\{0\}\,,

maps the unit disk 𝔹2\mathbb{B}^{2} onto itself with Ta(a)=0T_{a}(a)=0, Ta(±a/|a|)=±a/|a|T_{a}(\pm a/|a|)=\pm a/|a|.

In the extended real space ¯n\overline{\mathbb{R}}^{n}, the spherical (chordal) metric qq is defined as [11, (3.6), p. 29]

(2.10) {q(x,y)=|xy|1+|x|21+|y|2;xy,q(x,)=11+|x|2.\begin{cases}{\displaystyle q(x,y)=\frac{|x-y|}{\sqrt{1+|x|^{2}}\;\sqrt{1+|y|^{2}}}}\;;\,\;x\neq\infty\neq y\;,&\\ {\displaystyle q(x,\infty)=\frac{1}{\sqrt{1+|x|^{2}}}}\;\,.&\end{cases}

By using this metric, we can define the absolute ratio of any four distinct points a,b,c,d¯na,b,c,d\in\overline{\mathbb{R}}^{n} as [11, (3.10), p. 33], [4]

|a,b,c,d|=q(a,c)q(b,d)q(a,b)q(c,d),\displaystyle|a,b,c,d|=\frac{q(a,c)q(b,d)}{q(a,b)q(c,d)},

where the spherical distances can be replaced with the Euclidean distances if and only if {a,b,c,d}\infty\notin\{a,b,c,d\}. The absolute ratio is a very useful tool in complex analysis because it is invariant under Möbius transformations, which means that |a,b,c,d|=|h(a),h(b),h(c),h(d)||a,b,c,d|=|h(a),h(b),h(c),h(d)| for any Möbius transformation hh.

Next, let us recall some basic formulas and notation for hyperbolic geometry from [4]. The hyperbolic metric ρ𝔹n\rho_{\mathbb{B}^{n}} in the unit ball 𝔹n\mathbb{B}^{n} is defined by

(2.11) shρ𝔹n(x,y)2=|xy|(1|x|2)(1|y|2),{\rm sh}\frac{\rho_{\mathbb{B}^{n}}(x,y)}{2}=\frac{|x-y|}{\sqrt{(1-|x|^{2})(1-|y|^{2})}}\,,

where sh stands for the hyperbolic sine function. Correspondingly, we denote the hyperbolic cosine and tangent by ch and th. In the two-dimensional case, the formula (2.11) is equivalent to

(2.12) thρ𝔹2(x,y)2=|xy||1xy¯|=|xy|A[x,y],\displaystyle{\rm th}\frac{\rho_{\mathbb{B}^{2}}(x,y)}{2}=\frac{|x-y|}{|1-x\overline{y}|}=\frac{|x-y|}{A[x,y]},

where A[x,y]A[x,y] is the Ahlfors bracket defined as [3, 7.37]

(2.13) A[x,y]=|1xy¯|=|xy|2+(1|x|2)(1|y|2).A[x,y]=|1-x\overline{y}|=\sqrt{|x-y|^{2}+(1-|x|^{2})(1-|y|^{2})}.

The hyperbolic line through a,b𝔹2a,b\in\mathbb{B}^{2} is denoted by J[a,b]J^{*}[a,b]. If a,ba,b are collinear with the origin, the line J[a,b]J^{*}[a,b] is a diameter of the unit disk and, otherwise, an arc of the circle that passes through a,ba,b and is orthogonal to the unit circle. For a,b𝔹2{0}a,b\in\mathbb{B}^{2}\setminus\{0\}, let

(2.14) ep(a,b)=Tb(Tb(a)/|Tb(a)|).ep(a,b)=T_{-b}(T_{b}(a)/|T_{b}(a)|).

This formula defines the end points on the unit circle for the hyperbolic line J[a,b]J^{*}[a,b]. The hyperbolic metric also satisfies

(2.15) ρ𝔹2(x,y)=log|ep(a,b),a,b,ep(b,a)|,\rho_{\mathbb{B}^{2}}(x,y)=\log|ep(a,b),a,b,ep(b,a)|,

which shows, in particular, that the hyperbolic metric is invariant under Möbius transformations of the unit disk onto itself. In fact, the hyperbolic metric is invariant under all conformal mappings and the Möbius transformations are one subclass of conformal mappings.

Theorem 2.16.

[21, Thm 1.4, p. 126] For given x,y𝔹2x,y\in\mathbb{B}^{2}, the hyperbolic midpoint z𝔹2z\in\mathbb{B}^{2} with ρ𝔹2(x,z)=ρ𝔹2(y,z)=ρ𝔹2(x,y)/2\rho_{\mathbb{B}^{2}}(x,z)=\rho_{\mathbb{B}^{2}}(y,z)=\rho_{\mathbb{B}^{2}}(x,y)/2 is given by

(2.17) z=y(1|x|2)+x(1|y|2)1|x|2|y|2+A[x,y](1|x|2)(1|y|2).z=\frac{y(1-|x|^{2})+x(1-|y|^{2})}{1-|x|^{2}|y|^{2}+A[x,y]\sqrt{(1-|x|^{2})(1-|y|^{2})}}.

The extended real plane ¯2\overline{\mathbb{R}}^{2} is identified with the Riemann sphere via the stereographic projection. Denote e3=(0,0,1)e_{3}=(0,0,1). The stereographic projection  π:¯2S2(12e3,12)\ \pi:\overline{\mathbb{R}}^{2}\to S^{2}(\frac{1}{2}e_{3},\frac{1}{2}) is defined by [11, (3.4), p. 28]

(2.18) π(x)=e3+xe3|xe3|2,x2;π()=e3.\pi(x)=e_{3}+\frac{x-e_{3}}{|x-e_{3}|^{2}}\,,\;x\in{\mathbb{R}}^{2}\;;\;\,\pi(\infty)=e_{3}\;.

Then π\pi is the restriction to ¯2\overline{\mathbb{R}}^{2} of the inversion in S2(e3,1)S^{2}(e_{3},1). Because f1=ff^{-1}=f for every inversion ff, it follows that π\pi maps the “Riemann sphere” S2(12e3,12)S^{2}(\frac{1}{2}e_{3},\frac{1}{2}) onto ¯2\overline{\mathbb{R}}^{2}. By applying the stereographic projection π\pi from (2.18), the definition of the chordal metric qq in ¯2\overline{\mathbb{R}}^{2} can be written as [11, (3.5), p. 29]

(2.19) q(x,y)=|π(x)π(y)|;x,y¯2,q(x,y)=|\pi(x)-\pi(y)|\;;\;\,x,\,y\in\overline{\mathbb{R}}^{2}\;,

which is equivalent to (2.10) for n=2n=2.

The antipodal point a~=1/a¯\tilde{a}=-1/\overline{a} satisfies q(a,a~)=1q(a,\tilde{a})=1 [11, p. 29]. Thus, the great circle through two given points a,ba,b\in\mathbb{C} has the center m(a,a~,b)m(a,\tilde{a},b) given by (2.8) and its Euclidean radius is of course |am(a,a~,b)||a-m(a,\tilde{a},b)| while its chordal radius is 1/2.1/\sqrt{2}. For instance, if a2{0},a\in{\mathbb{R}^{2}}\setminus\{0\}, then q(a,±ia/|a|)=1/2.q(a,\pm ia/|a|)=1/\sqrt{2}. Note that if a,ba,b\in\mathbb{C} are collinear with the origin, then m(a,a~,b)m(a,\tilde{a},b) is not well-defined, and the stereographic projection of the great circle through aa and bb on the plane \mathbb{C} is a Euclidean line L(a,b)L(a,b). For further information, see [5, Thm 18.4.2].

Hereafter, we will discuss mainly geometry on the complex plane.

For a point zz\in\mathbb{C}, the stereographic projection π\pi in (2.18) is written as

(2.20) π:z(Rez1+|z|2,Imz1+|z|2,|z|21+|z|2).\displaystyle\pi\,:\,z\mapsto\Big{(}\frac{\mbox{Re}\,z}{1+|z|^{2}},\frac{\mbox{Im}\,z}{1+|z|^{2}},\frac{|z|^{2}}{1+|z|^{2}}\Big{)}.

Conversely, the point zz\in\mathbb{C} corresponding to the point (ξ,η,ζ)(\xi,\eta,\zeta) on the Riemann sphere can be written as

z=ξ1ζ+iη1ζ,whereξ2+η2+(ζ12)2=(14).z=\frac{\xi}{1-\zeta}+i\frac{\eta}{1-\zeta},\quad\mbox{where}\quad\ \xi^{2}+\eta^{2}+\big{(}\zeta-\frac{1}{2}\big{)}^{2}=\big{(}\frac{1}{4}\big{)}.

Assume that points π(a)\pi(a), π(b)\pi(b), π(c)\pi(c), and π(d)\pi(d) are not on the same great circle. The intersection point of stereographic projections of two great circles passing through π(a)\pi(a), π(b)\pi(b) and π(c)\pi(c), π(d)\pi(d) inside the closed unit disk is denoted as

(2.21) GCIS[a,b,c,d]={z𝔹¯2:F(z;a,b,c,d)=0},\displaystyle{\rm GCIS}[a,b,c,d]=\{z\in\overline{\mathbb{B}}^{2}\,:\,F(z;a,b,c,d)=0\},

where the function FF is as follows:

F(z;a,b,c,d)\displaystyle F(z;a,b,c,d)\equiv ((a¯b¯(ab)+a¯b¯)(cd¯c¯d)(ab¯a¯b)(c¯d¯(cd)+c¯d¯))z2\displaystyle\big{(}(\overline{a}\overline{b}(a-b)+\overline{a}-\overline{b})(c\overline{d}-\overline{c}d)-(a\overline{b}-\overline{a}b)(\overline{c}\overline{d}(c-d)+\overline{c}-\overline{d})\big{)}z^{2}
+((1a¯b¯cd)(ab)(c¯d¯)+(1abc¯d¯)(a¯b¯)(cd)\displaystyle\ +\big{(}-(1-\overline{a}\overline{b}cd)(a-b)(\overline{c}-\overline{d})+(1-ab\overline{c}\overline{d})(\overline{a}-\overline{b})(c-d)
+(ab)(cd)(a¯b¯c¯d¯)(a¯b¯)(c¯d¯)(abcd))z\displaystyle\ +(a-b)(c-d)(\overline{a}\overline{b}-\overline{c}\overline{d})-(\overline{a}-\overline{b})(\overline{c}-\overline{d})(ab-cd)\big{)}z
(cd¯c¯d)(ab(a¯b¯)+(ab))+(ab¯a¯b)(cd(c¯d¯)+(cd)).\displaystyle\ -(c\overline{d}-\overline{c}d)(ab(\overline{a}-\overline{b})+(a-b))+(a\overline{b}-\overline{a}b)(cd(\overline{c}-\overline{d})+(c-d)).

This result follows from the definition of great circles passing through two points and the formula of intersection points of two Euclidean circles. See also the proof of Theorem 5.12 and Appendix.

3. Five collinear intersection points

In this section, we study the five collinear intersection points of the Euclidean lines passing through such points that are defined in terms of two given points in the unit disk.

Fix first two distinct points a,b𝔹2\{0}a,b\in\mathbb{B}^{2}\backslash\{0\} so that they are non-collinear with the origin. Let aa^{\ast} and bb^{\ast} be the reflections of aa and bb with respect to the unit circle, respectively. Then,

(3.1) a=1a¯,b=1b¯.a^{\ast}=\frac{1}{\overline{a}},\quad b^{\ast}=\frac{1}{\overline{b}}.

Let aa_{\ast} and bb_{\ast} be the intersection points of the unit circle and the hyperbolic line passing through aa and bb that are near aa and bb, respectively. These points can be found with (2.14), which yields the formulas

(3.2) a=b(1ab¯)|ab|+(ab)|1ab¯|(1ab¯)|ab|+b¯(ab)|1ab¯|,b=a(1a¯b)|ba|+(ba)|1a¯b|(1a¯b)|ba|+a¯(ba)|1a¯b|.a_{\ast}=\frac{b(1-a\overline{b})|a-b|+(a-b)|1-a\overline{b}|}{(1-a\overline{b})|a-b|+\overline{b}(a-b)|1-a\overline{b}|},\quad b_{\ast}=\frac{a(1-\overline{a}{b})|b-a|+(b-a)|1-\overline{a}{b}|}{(1-\overline{a}{b})|b-a|+\overline{a}(b-a)|1-\overline{a}{b}|}.

In the notation of (2.14), a=ep(a,b)a_{*}=ep(a,b) and b=ep(b,a)b_{*}=ep(b,a).

Fix then the intersection points

(3.3) k\displaystyle k =LIS[a,a,b,b],\displaystyle={\rm LIS}[a_{\ast},a^{\ast},b_{\ast},b^{\ast}], s\displaystyle s =LIS[a,b,b,a],\displaystyle={\rm LIS}[a,b_{\ast},b,a_{\ast}], t\displaystyle t =LIS[a,b,b,a],\displaystyle={\rm LIS}[a_{\ast},b^{\ast},b_{\ast},a^{\ast}],
u\displaystyle u =LIS[a,b,b,a],\displaystyle={\rm LIS}[a,b^{\ast},b,a^{\ast}], v\displaystyle v =LIS[a,a,b,b].\displaystyle={\rm LIS}[a,a_{\ast},b,b_{\ast}].

Furthermore, let mm be the hyperbolic midpoint of aa and bb. See Figure 1.

kkaa^{*}bb^{*}aabb_{*}bbaa_{*}0vvmmssuutt
Figure 1. The points of Theorem 3.4 for a=0.5a=0.5 and b=0.7eib=0.7e^{i}. The line passing through kk and the origin contains the points k,0,v,m,s,u,tk,0,v,m,s,u,t in this order. The dashed circle passing through b,b,b,m,a,a,ab^{*},b_{*},b,m,a,a_{*},a^{*} is orthogonal to the unit circle.

The following result was obtained in [19] by using the properties of Möbius transformations without finding the explicit formulas for the intersection points.

Theorem 3.4.

[19, Lemma 4.6, p. 282] For a,b𝔹2a,b\in\mathbb{B}^{2}, the five points k,s,t,u,vk,s,t,u,v fixed as in (3.3), the hyperbolic midpoint mm of aa and bb, and the origin are all collinear.

The exact coordinates of the intersection points are given as follows.

Theorem 3.5.

The explicit formulas of the points k,s,t,u,vk,s,t,u,v in (3.3) are

k\displaystyle k =(a(1|b|2)+b(1|a|2))|ab||1a¯b|(1|ab|2)|ab|+(2|ab|2(|a|2+|b|2))|1a¯b|,\displaystyle=\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}\dfrac{|a-b|-|1-\overline{a}b|}{(1-|ab|^{2})|a-b|+\big{(}2|ab|^{2}-(|a|^{2}+|b|^{2})\big{)}|1-\overline{a}b|},
s\displaystyle s =a(1|b|2)+b(1|a|2)2(ab¯+ba¯)|ab||1a¯b|,\displaystyle=\dfrac{a(1-|b|^{2})+b(1-|a|^{2})}{2-(a\overline{b}+b\overline{a})-|a-b||1-\overline{a}b|},
t\displaystyle t =a(1|b|2)+b(1|a|2)(ab¯+a¯b)2|ab|2+|ab||1a¯b|,\displaystyle=\frac{a(1-|b|^{2})+b(1-|a|^{2})}{(a\overline{b}+\overline{a}b)-2|ab|^{2}+|a-b||1-\overline{a}b|},
u\displaystyle u =a(1|b|2)+b(1|a|2)1|ab|2,\displaystyle=\dfrac{a(1-|b|^{2})+b(1-|a|^{2})}{1-|ab|^{2}},
v\displaystyle v =(a(1|b|2)+b(1|a|2))|1a¯b||ab|(2(|a|2+|b|2))|1a¯b|(1|ab|2)|ab|.\displaystyle=\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}\dfrac{|1-\overline{a}b|-|a-b|}{\big{(}2-(|a|^{2}+|b|^{2})\big{)}|1-\overline{a}b|-(1-|ab|^{2})|a-b|}.
Proof.

The point uu is already obtained in [19, (4.8), p.282]. By fixing mab=|ab|m_{ab}=|a-b| and m1=|1ab¯|m_{1}=|1-a\overline{b}|, aa_{\ast} can be written as

(3.6) a=b(1ab¯)mab+(ab)m1(1ab¯)mab+b¯(ab)m1.a_{\ast}=\frac{b(1-a\overline{b})m_{ab}+(a-b)m_{1}}{(1-a\overline{b})m_{ab}+\overline{b}(a-b)m_{1}}.

As |ab|=|ba||a-b|=|b-a| and |1a¯b|=|1ab¯||1-\overline{a}b|=|1-a\overline{b}|,

(3.7) b=a(1a¯b)mab(ab)m1(1a¯b)maba¯(ab)m1.b_{\ast}=\frac{a(1-\overline{a}{b})m_{ab}-(a-b)m_{1}}{(1-\overline{a}{b})m_{ab}-\overline{a}(a-b)m_{1}}.

By substituting (3.1), (3.6), and (3.7) into (2.3), we have

t=LIS[a,b,b,a]=(a(1bb¯)+b(1aa¯))m1(1ab¯)(1a¯b)mab+(ab¯+a¯b2aba¯b¯)m1.t={\rm LIS}[a_{\ast},b^{\ast},b_{\ast},a^{\ast}]=\frac{\big{(}a(1-b\overline{b})+b(1-a\overline{a})\big{)}m_{1}}{(1-a\overline{b})(1-\overline{a}b)m_{ab}+(a\overline{b}+\overline{a}b-2ab\overline{a}\overline{b})m_{1}}.

The substitution calculations and reduction of fractions here can be obtained by using the symbolic computation system Risa/Asir as the calculation of substitutions and reduction of fractions is just an algebraic process.

From (1ab¯)(1a¯b)=m12(1-a\overline{b})(1-\overline{a}b)=m_{1}^{2}, it follows that

t\displaystyle t =(a(1bb¯)+b(1aa¯))m1m12mab+(ab¯+a¯b2aba¯b¯)m1=a(1bb¯)+b(1aa¯)(ab¯+a¯b)2aba¯b¯+m1mab\displaystyle=\frac{\big{(}a(1-b\overline{b})+b(1-a\overline{a})\big{)}m_{1}}{m_{1}^{2}m_{ab}+(a\overline{b}+\overline{a}b-2ab\overline{a}\overline{b})m_{1}}=\frac{a(1-b\overline{b})+b(1-a\overline{a})}{(a\overline{b}+\overline{a}b)-2ab\overline{a}\overline{b}+m_{1}m_{ab}}
=a(1|b|2)+b(1|a|2)(ab¯+a¯b)2|ab|2+|ab||1a¯b|.\displaystyle=\frac{a(1-|b|^{2})+b(1-|a|^{2})}{(a\overline{b}+\overline{a}b)-2|ab|^{2}+|a-b||1-\overline{a}b|}.

By using the same method as above for the points s,ks,k, and vv, we have

s\displaystyle s =LIS[a,b,b,a]\displaystyle={\rm LIS}[a,b_{\ast},b,a_{\ast}]
=(a(1bb¯)+b(1aa¯))mab(2ab¯a¯b)mab(ab)(a¯b¯)m1=(a(1bb¯)+b(1aa¯))mab(2ab¯a¯b)mabmab2m1\displaystyle=\frac{\big{(}a(1-b\overline{b})+b(1-a\overline{a})\big{)}m_{ab}}{(2-a\overline{b}-\overline{a}b)m_{ab}-(a-b)(\overline{a}-\overline{b})m_{1}}=\frac{\big{(}a(1-b\overline{b})+b(1-a\overline{a})\big{)}m_{ab}}{(2-a\overline{b}-\overline{a}b)m_{ab}-m_{ab}^{2}m_{1}}
=a(1bb¯)+b(1aa¯)(2ab¯a¯b)mabm1=a(1|b|2)+b(1|a|2)2(ab¯+ba¯)|ab||1a¯b|,\displaystyle=\frac{a(1-b\overline{b})+b(1-a\overline{a})}{(2-a\overline{b}-\overline{a}b)-m_{ab}m_{1}}=\dfrac{a(1-|b|^{2})+b(1-|a|^{2})}{2-(a\overline{b}+b\overline{a})-|a-b||1-\overline{a}b|},
k\displaystyle k =LIS[a,a,b,b]\displaystyle={\rm LIS}[a_{\ast},a^{\ast},b_{\ast},b^{\ast}]
=(a(1bb¯)+b(1aa¯))(mabm1)(1aba¯b¯)mab+(2aba¯b¯(aa¯+bb¯))m1\displaystyle=\frac{\big{(}a(1-b\overline{b})+b(1-a\overline{a})\big{)}(m_{ab}-m_{1})}{(1-ab\overline{a}\overline{b})m_{ab}+(2ab\overline{a}\overline{b}-(a\overline{a}+b\overline{b}))m_{1}}
=(a(1|b|2)+b(1|a|2))|ab||1a¯b|(1|ab|2)|ab|+(2|ab|2(|a|2+|b|2))|1a¯b|,\displaystyle=\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}\dfrac{|a-b|-|1-\overline{a}b|}{(1-|ab|^{2})|a-b|+\big{(}2|ab|^{2}-(|a|^{2}+|b|^{2})\big{)}|1-\overline{a}b|},

and

v\displaystyle v =LIS[a,a,b,b]\displaystyle={\rm LIS}[a,a_{\ast},b,b_{\ast}]
=(a(1bb¯)+b(1aa¯))((1ab¯)(1a¯b)mab(ab)(a¯b¯)m1)(1ab¯)(1a¯b)(2aa¯bb¯)mab(ab)(a¯b¯)(1aba¯b¯)m1\displaystyle=\frac{\big{(}a(1-b\overline{b})+b(1-a\overline{a})\big{)}\big{(}(1-a\overline{b})(1-\overline{a}b)m_{ab}-(a-b)(\overline{a}-\overline{b})m_{1}\big{)}}{(1-a\overline{b})(1-\overline{a}b)(2-a\overline{a}-b\overline{b})m_{ab}-(a-b)(\overline{a}-\overline{b})(1-ab\overline{a}\overline{b})m_{1}}
=(a(1bb¯)+b(1aa¯))m12mabmab2m1m12(2aa¯bb¯)mabmab2(1aba¯b¯)m1\displaystyle=\big{(}a(1-b\overline{b})+b(1-a\overline{a})\big{)}\frac{m_{1}^{2}m_{ab}-m_{ab}^{2}m_{1}}{m_{1}^{2}(2-a\overline{a}-b\overline{b})m_{ab}-m_{ab}^{2}(1-ab\overline{a}\overline{b})m_{1}}
=(a(1|b|2)+b(1|a|2))|1a¯b||ab|(2(|a|2+|b|2))|1a¯b|(1|ab|2)|ab|.\displaystyle=\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}\dfrac{|1-\overline{a}b|-|a-b|}{\big{(}2-(|a|^{2}+|b|^{2})\big{)}|1-\overline{a}b|-(1-|ab|^{2})|a-b|}.

Each of these five points k,s,t,uk,s,t,u, and vv has the form r(a(1|b|2)+b(1|a|2))r\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)} for some real number rr. From the formula (2.17) of Theorem 2.16, we see trivially that the hyperbolic midpoint mm also has this same property. Therefore, all these six points are on the line passing through the origin and the point a(1|b|2)+b(1|a|2)a(1-|b|^{2})+b(1-|a|^{2}). This would also prove the collinearity stated in Theorem 3.4. Additionally, we can write these points in the form cjHc_{j}H for j=1,,6j=1,...,6 when H=a(1|b|2)+b(1|a|2)H=a(1-|b|^{2})+b(1-|a|^{2}) and the constants cjc_{j} are as in Table 1.

jj Point Definition cjc_{j}
1 kk LIS[a,a,b,b]{\rm LIS}[a_{\ast},a^{\ast},b_{\ast},b^{\ast}] |ab||1a¯b|(1|ab|2)|ab|+(2|ab|2(|a|2+|b|2))|1a¯b|\dfrac{|a-b|-|1-\overline{a}b|}{(1-|ab|^{2})|a-b|+\big{(}2|ab|^{2}-(|a|^{2}+|b|^{2})\big{)}|1-\overline{a}b|}
2 ss LIS[a,b,b,a]{\rm LIS}[a,b_{\ast},b,a_{\ast}] 12(ab¯+ba¯)|ab||1a¯b|\dfrac{1}{2-(a\overline{b}+b\overline{a})-|a-b||1-\overline{a}b|}
3 tt LIS[a,b,b,a]{\rm LIS}[a_{\ast},b^{\ast},b_{\ast},a^{\ast}] 1(ab¯+a¯b)2|ab|2+|ab||1a¯b|\dfrac{1}{(a\overline{b}+\overline{a}b)-2|ab|^{2}+|a-b||1-\overline{a}b|}
4 uu LIS[a,b,b,a]{\rm LIS}[a,b^{\ast},b,a^{\ast}] 11|ab|2\dfrac{1}{1-|ab|^{2}}
5 vv LIS[a,a,b,b]{\rm LIS}[a,a_{\ast},b,b_{\ast}] |1a¯b||ab|(2(|a|2+|b|2))|1a¯b|(1|ab|2)|ab|\dfrac{|1-\overline{a}b|-|a-b|}{\big{(}2-(|a|^{2}+|b|^{2})\big{)}|1-\overline{a}b|-(1-|ab|^{2})|a-b|}
6 mm Hyperbolic 11|a|2|b|2+A[a,b](1|a|2)(1|b|2)\dfrac{1}{1-|a|^{2}|b|^{2}+A[a,b]\sqrt{(1-|a|^{2})(1-|b|^{2})}}
midpoint of
aa and bb
Table 1. The constants cjc_{j}, j=1,,6j=1,...,6, with which the formulas of the points k,s,t,u,vk,s,t,u,v from (3.3) and the hyperbolic midpoint mm of a,ba,b can be written in the form cjHc_{j}H where H=a(1|b|2)+b(1|a|2)H=a(1-|b|^{2})+b(1-|a|^{2}).
Remark 3.8.

The origin coincides with the intersection point LIS[a,a,b,b]{\rm LIS}[a,a^{\ast},b,b^{\ast}] because aa^{\ast} and bb^{\ast} are the reflections of aa and bb, respectively.

Remark 3.9.

(1) It is clear from Pascal’s theorem (can be found e.g. in [9, Sect. 3]) that the three points s,t,us,t,u are collinear.
(2) The triangles sabsab and tbatb^{*}a^{*} are perspectives from the point uu. According to the Desargues theorem [9, Sect. 3], the point M=L(a,b)L(a,b)M=L(a,b)\cap L(a^{*},b^{*}) is located on the line L(a,b)L(a_{*},b_{*}). From Desargues’s theorem, concerning suitable triangles, the other correspondences can also be proved, the only exception being the point mm. Let mm^{*} be the point of intersection of the dashed circle with the axis. The central-axial collinearity given by the center MM, the axis OuOu and the pair of points {a,b}\{a,b\} sends the cross-section (a,a,m,b)(a_{*},a,m^{*},b_{*}) to the cross-section (b,b,m,a)(b_{*},b,m^{*},a_{*}), therefore m=mm^{*}=m, i.e. mm is also a point of the corresponding line.

4. Collinearity results for great circles

In this section, we define points similar to k,s,t,u,vk,s,t,u,v in (3.3) but by using the stereographic projections of intersection points of great circles instead the intersection points of Euclidean lines. The new points are also collinear, as stated in Theorem 4.2, which is the corresponding version of Theorems 3.4 and 3.5. In fact, we show in Corollary 4.10 that all the resulting eleven points are collinear with the origin. At the end of this section, another collinearity result, Theorem 4.11, is also proved.

For such two points a,b𝔹2a,b\in\mathbb{B}^{2} that are non-collinear with the origin, let a,b,a,ba^{*},b^{*},a_{*},b_{*} be as in (3.1) and (3.2). Fix then kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} as the intersection points of the stereographic projections of great circles so that

(4.1) kc\displaystyle k_{c} =GCIS[a,a,b,b],sc=GCIS[a,b,b,a],tc=GCIS[a,b,b,a],\displaystyle={\rm GCIS}[a_{\ast},a^{\ast},b_{\ast},b^{\ast}],\quad s_{c}={\rm GCIS}[a,b_{\ast},b,a_{\ast}],\quad t_{c}={\rm GCIS}[a_{\ast},b^{\ast},b_{\ast},a^{\ast}],
uc\displaystyle u_{c} GCIS[a,b,b,a],vc=GCIS[a,a,b,b].\displaystyle\in{\rm GCIS}[a,b^{\ast},b,a^{\ast}],\quad v_{c}={\rm GCIS}[a,a_{\ast},b,b_{\ast}].

In other words, kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} are as the points k,s,t,u,vk,s,t,u,v in (3.3), except they are the stereographic projections of intersection points of great circles while k,s,t,u,vk,s,t,u,v are simply the intersection points of Euclidean lines. Note that there are two possible choices for ucu_{c} as there are two intersection points in GCIS[a,b,b,a]{\rm GCIS}[a,b^{\ast},b,a^{\ast}] that both lie on the unit circle.

aabbaa^{*}bb^{*}aa_{*}bb_{*}0kck_{c}scs_{c}tct_{c}ucu_{c}vcv_{c}
Figure 2. The intersection points of Theorem 4.2 for a=0.5a=0.5 and b=0.6eib=0.6e^{i}. The circle marked with the black solid outline is the unit circle S1S^{1}. All other circles and arcs are stereographic projections of great circles.

Theorem 4.2.

If a,b𝔹2a,b\in\mathbb{B}^{2} are non-collinear with the origin, then the points kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} in (4.1) are on a line passing through the origin.

Proof.

Since the points kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} are all given as stereographic projections of intersections of two great circles, we can use the formula (2.21) and its function FF.

For tct_{c}, let

Tc:=F(z;b,a,b,a).T_{c}:=F(z;b_{\ast},a^{\ast},b^{\ast},a_{\ast}).

By using the symbolic computation system Risa/Asir, we have

numerator(Tc)=\displaystyle numerator(T_{c})= 2|ab|3|1ab¯|(1|b|2)(1|a|2)(ab¯a¯b)(|ab|+|1ab¯|)\displaystyle 2|a-b|^{3}|1-a\overline{b}|(1-|b|^{2})(1-|a|^{2})(a\overline{b}-\overline{a}b)\big{(}|a-b|+|1-a\overline{b}|\big{)}
((a¯(1|b|2)+b¯(1|a|2))z2+2|1ab¯|(|ab||1ab¯|)z\displaystyle\Big{(}\big{(}\overline{a}(1-|b|^{2})+\overline{b}(1-|a|^{2})\big{)}z^{2}+2|1-a\overline{b}|(|a-b|-|1-a\overline{b}|)z
(a(1|b|2)+b(1|a|2))),\displaystyle-\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}\Big{)},
denominator(Tc)=\displaystyle denominator(T_{c})= |a|2|b|2|(a¯b1)|ab|+b(b¯a¯)|1ab¯||2\displaystyle|a|^{2}|b|^{2}\big{|}(\overline{a}b-1)|a-b|+b(\overline{b}-\overline{a})|1-a\overline{b}|\big{|}^{2}
×|(a¯b1)|ab|+a¯(ab)|1ab¯||2.\displaystyle\times\big{|}(\overline{a}b-1)|a-b|+\overline{a}(a-b)|1-a\overline{b}|\big{|}^{2}.

Because of the assumption that the two points a,ba,b are not collinear with the origin, the inequality ab¯a¯b0a\overline{b}-\overline{a}b\neq 0 holds. Therefore, tct_{c} can be obtained by solving the following equation for zz:

(4.3) (a¯(1|b|2)+b¯(1|a|2))z2+2|1ab¯|(|ab||1ab¯|)z(a(1|b|2)+b(1|a|2))=0.\big{(}\overline{a}(1-|b|^{2})+\overline{b}(1-|a|^{2})\big{)}z^{2}+2|1-a\overline{b}|(|a-b|-|1-a\overline{b}|)z-\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}=0.

For ucu_{c}, we have

F(z;b,a,a,b)\displaystyle F(z;b,a^{\ast},a,b^{\ast})
=2(ab¯a¯b)((a¯(1|b|2)+b¯(1|a|2))z2(a(1|b|2)+b(1|a|2)))|ab|2.\displaystyle\quad=\frac{-2(a\overline{b}-\overline{a}b)\Big{(}\big{(}\overline{a}(1-|b|^{2})+\overline{b}(1-|a|^{2})\big{)}z^{2}-\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}\Big{)}}{|ab|^{2}}.

Hence, ucu_{c} can be obtained by solving the equation

(4.4) (a¯(1|b|2)+b¯(1|a|2))z2(a(1|b|2)+b(1|a|2))=0.\big{(}\overline{a}(1-|b|^{2})+\overline{b}(1-|a|^{2})\big{)}z^{2}-\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}=0.

For scs_{c}, set

Sc:=F(z;b,a,a,b).S_{c}:=F(z;b,a_{\ast},a,b_{\ast}).

By eliminating the non-zero factors from numerator(Sc)=0numerator(S_{c})=0 under the assumptions of the theorem, we find that scs_{c} can be obtained as the solution of the following equation

(4.5) (a¯(1|b|2)+b¯(1|a|2))z2+2|1ab¯|(|1ab¯||ab|)z(a(1|b|2)+b(1|a|2))=0.\big{(}\overline{a}(1-|b|^{2})+\overline{b}(1-|a|^{2})\big{)}z^{2}+2|1-a\overline{b}|(|1-a\overline{b}|-|a-b|)z-\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}=0.

For vcv_{c}, set

Vc:=F(z;b,b,a,a),V_{c}:=F(z;b,b_{\ast},a,a_{\ast}),

and again, by eliminating the non-zero factors from numerator(Vc)=0numerator(V_{c})=0, we have the following equation

(4.6) (a¯(1|b|2)+b¯(1|a|2))z2+2(1|a|2)(1|b|2)|1ab¯||1ab¯||ab|z\displaystyle\big{(}\overline{a}(1-|b|^{2})+\overline{b}(1-|a|^{2})\big{)}z^{2}+2\frac{(1-|a|^{2})(1-|b|^{2})|1-a\overline{b}|}{|1-a\overline{b}|-|a-b|}z
(a(1|b|2)+b(1|a|2))=0.\displaystyle-\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}=0.

(Note that, if |1ab¯|=|ab||1-a\overline{b}|=|a-b|, then either |a|=1|a|=1 or |b|=1|b|=1 holds by (2.13).)

For kck_{c}, set

Kc:=F(z;b,b,a,a).K_{c}:=F(z;b^{\ast},b_{\ast},a^{\ast},a_{\ast}).

By eliminating the non-zero factors from numerator(Kc)=0numerator(K_{c})=0, we have the following.

(4.7) (a¯(1|b|2)+b¯(1|a|2))z2+2(1|a|2)(1|b|2)|1ab¯||ab||1ab¯|z\displaystyle\big{(}\overline{a}(1-|b|^{2})+\overline{b}(1-|a|^{2})\big{)}z^{2}+2\frac{(1-|a|^{2})(1-|b|^{2})|1-a\overline{b}|}{|a-b|-|1-a\overline{b}|}z
(a(1|b|2)+b(1|a|2))=0.\displaystyle-\big{(}a(1-|b|^{2})+b(1-|a|^{2})\big{)}=0.

Let H=a(1|b|2)+b(1|a|2)H=a(1-|b|^{2})+b(1-|a|^{2}) as in Table 1. Then the equations (4.3), (4.4), (4.5), (4.6), and (4.7) can be written in the form

(4.8) H¯z2+2RzH=0,(R),\overline{H}z^{2}+2Rz-H=0,\quad(R\in\mathbb{R}),

for some real RR, whose exact value can be seen from Table 2.

Note that the solution zz of equation (4.8) has the form

R+R2+|H|2H¯=R+R2+|H|2|H|2HorRR2+|H|2|H|2H.\frac{-R+\sqrt{R^{2}+|H|^{2}}}{\overline{H}}=\frac{-R+\sqrt{R^{2}+|H|^{2}}}{|H|^{2}}H\qquad\mbox{or}\qquad\frac{-R-\sqrt{R^{2}+|H|^{2}}}{|H|^{2}}H.

In both cases, the solution has the form z=MHz=MH for some real value MM. Therefore, Arg(z)=Arg(H){\rm Arg}(z)={\rm Arg}(H) for M>0M>0 and Arg(z)=Arg(H)+π{\rm Arg}(z)={\rm Arg}(H)+\pi for M<0M<0. Hence, it follows that the five points bc,uc,sc,vc,kcb_{c},u_{c},s_{c},v_{c},k_{c} are on the line passing through HH and the origin. ∎

Point Definition RR
kck_{c} GCIS[a,a,b,b]{\rm GCIS}[a_{\ast},a^{\ast},b_{\ast},b^{\ast}] (1|a|2)(1|b|2)|1ab¯||ab||1ab¯|\dfrac{(1-|a|^{2})(1-|b|^{2})|1-a\overline{b}|}{|a-b|-|1-a\overline{b}|}
scs_{c} GCIS[a,b,b,a]{\rm GCIS}[a,b_{\ast},b,a_{\ast}] |1ab¯|(|1ab¯||ab|)|1-a\overline{b}|(|1-a\overline{b}|-|a-b|)
tct_{c} GCIS[a,b,b,a]{\rm GCIS}[a_{\ast},b^{\ast},b_{\ast},a^{\ast}] |1ab¯|(|ab||1ab¯|)|1-a\overline{b}|(|a-b|-|1-a\overline{b}|)
ucu_{c} GCIS[a,b,b,a]{\rm GCIS}[a,b^{\ast},b,a^{\ast}] 0
vcv_{c} GCIS[a,a,b,b]{\rm GCIS}[a,a_{\ast},b,b_{\ast}] (1|a|2)(1|b|2)|1ab¯||1ab¯||ab|\dfrac{(1-|a|^{2})(1-|b|^{2})|1-a\overline{b}|}{|1-a\overline{b}|-|a-b|}
Table 2. The real numbers RR with which the formulas of the intersection points kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} from (4.1) can be written as the roots of the equation H¯z2+2RzH=0\overline{H}z^{2}+2Rz-H=0, where H=a(1|b|2)+b(1|a|2)H=a(1-|b|^{2})+b(1-|a|^{2}).
Remark 4.9.

The equation (4.8) has two solutions in the form zz and 1/z¯-1/\overline{z}. Assuming R0R\neq 0, there is one solution inside and one outside the unit disk. Therefore, under the condition a,b𝔹2a,b\in\mathbb{B}^{2}, every equation of Tc=0T_{c}=0, Sc=0S_{c}=0, Vc=0V_{c}=0, and Kc=0K_{c}=0 in the proof of Theorem 4.2 has a unique solution in the unit disk, and the points tct_{c}, scs_{c}, vcv_{c}, and kck_{c} are well defined from (2.21). While there are two possible choices for ucu_{c}, it does not matter which of them is considered as they both are collinear with the other points. Furthermore, the intersection points kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} of the stereographic projections of great circles in Theorem 4.2 are also collinear with the corresponding intersection points of kc,sc,tc,vck_{c},s_{c},t_{c},v_{c} outside the unit circle. The proof for this claim follows from the fact that these intersection points in the complement of the unit disk also fulfill the condition F(z;a,b,c,d)=0F(z;a,b,c,d)=0 in (2.21). Their collinearity can be seen from Figure 2.

Corollary 4.10.

If a,b𝔹2a,b\in\mathbb{B}^{2} are non-collinear with the origin, mm is the hyperbolic midpoint of aa and bb, the five points k,s,t,u,vk,s,t,u,v are as in (3.3) for these choices of aa and bb, and the other five kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} are as in (4.1), then the 11 points k,m,s,t,u,v,kc,sc,tc,uc,vck,m,s,t,u,v,k_{c},s_{c},t_{c},u_{c},v_{c} and the origin are collinear.

Proof.

As can be seen from Theorem 3.5 or Table 1, the arguments of points k,m,s,t,u,vk,m,s,t,u,v are all equal to either Arg(H){\rm Arg}(H) or Arg(H)+π{\rm Arg}(H)+\pi with H=a(1|b|2)+b(1|a|2)H=a(1-|b|^{2})+b(1-|a|^{2}), and they therefore coincide with the arguments of points kc,sc,tc,uc,vck_{c},s_{c},t_{c},u_{c},v_{c} in Theorem 4.2. ∎


aabbaa^{*}bb^{*}aa_{*}bb_{*}0ppqqpcp_{c}qcq_{c}
Figure 3. The intersection points of Theorem 4.11 for a=0.5a=0.5 and b=0.6eib=0.6e^{i}. The circle with solid line is the unit circle and the dashed circle is the orthogonal circle to the unit circle passing through a,ba,b. All the circle arcs are arcs from the stereographic projections of great circles passing through the end points of the arc in question.
Theorem 4.11.

Choose such a,b𝔹2\{0}a,b\in\mathbb{B}^{2}\backslash\{0\} non-collinear with the origin and let a,b,a,ba^{*},b^{*},a_{*},b_{*} be as in in (3.1) and (3.2). Fix p=LIS[a,b,a,b]p={\rm LIS}[a,b_{*},a^{*},b] and q=LIS[a,b,a,b]q={\rm LIS}[a,b^{*},a^{*},b_{*}]. Similarly, let pc=GCIS[a,b,a,b]p_{c}={\rm GCIS}[a,b_{*},a^{*},b], and qc=GCIS[a,b,a,b]q_{c}={\rm GCIS}[a,b^{*},a^{*},b_{*}]. The intersection points p,q,pc,qcp,q,p_{c},q_{c} and the origin are collinear.

Proof.

For qcq_{c}, calculating F(z;a,b,a,b)=0F(z;a,b^{\ast},a^{\ast},b_{\ast})=0, eliminating the non-desired factors, qcq_{c} is obtained by the solution of the following equation,

(4.12) Qz2+RzQ¯=0,where\displaystyle Qz^{2}+Rz-\overline{Q}=0,\quad\text{where}
Q=b¯(1|a|2)2+a¯|ab|(|1a¯b||ab|),\displaystyle Q=\overline{b}(1-|a|^{2})^{2}+\overline{a}|a-b|(|1-\overline{a}b|-|a-b|),
R=(1|a|2)|1a¯b|(|ab||1a¯b|).\displaystyle R=(1-|a|^{2})|1-\overline{a}b|(|a-b|-|1-\overline{a}b|).

Note that RR\in\mathbb{R} above.


Similarly for pcp_{c}, the point pcp_{c} is given by the equation Qz2+Rz+Q¯=0Qz^{2}+Rz+\overline{Q}=0, where QQ and RR are as in (4.12), and the arguments of the solutions qcq_{c} and pcp_{c} are therefore Arg(Q¯){\rm Arg}(\overline{Q}) or Arg(Q¯)+π{\rm Arg}(\overline{Q})+\pi.


For points pp and qq, the following is also obtained from calculation of LIS[a,b,a,b]{\rm LIS}[a,b^{\ast},a^{\ast},b_{\ast}] and LIS[a,b,a,b]{\rm LIS}[a,b_{\ast},a^{\ast},b], respectively.

q\displaystyle q =b(1|a|2)2+a|ab|(|1a¯b||ab|)|b|2(1|a|2)2+|ab|(|1a¯b||ab|),\displaystyle=\frac{b(1-|a|^{2})^{2}+a|a-b|(|1-\overline{a}b|-|a-b|)}{|b|^{2}(1-|a|^{2})^{2}+|a-b|(|1-\overline{a}b|-|a-b|)},
p\displaystyle p =b(1|a|2)2+a|ab|(|1a¯b||ab|)(1|a|2)2+|a|2|ab|(|1a¯b||ab|).\displaystyle=\frac{b(1-|a|^{2})^{2}+a|a-b|(|1-\overline{a}b|-|a-b|)}{(1-|a|^{2})^{2}+|a|^{2}|a-b|(|1-\overline{a}b|-|a-b|)}.

Since the denominators of pp and qq both have positive real values, clearly,

Arg(q)=Arg(p)=Arg(b(1|a|2)2+a|ab|(|1a¯b||ab|))=Arg(Q¯){\rm Arg}(q)={\rm Arg}(p)={\rm Arg}\big{(}b(1-|a|^{2})^{2}+a|a-b|(|1-\overline{a}b|-|a-b|)\big{)}={\rm Arg}(\overline{Q})

hold. Hence, the four points qc,pc,q,pq_{c},p_{c},q,p are on the line passing through the origin and Q¯=b(1|a|2)2+a|ab|(|1a¯b||ab|)\overline{Q}=b(1-|a|^{2})^{2}+a|a-b|(|1-\overline{a}b|-|a-b|). ∎

5. Hyperbolic and chordal midpoints

In this section, we first introduce a few results related to the hyperbolic midpoint. In Theorems 5.2 and 5.4, we show new ways to construct the hyperbolic midpoint of two points in the unit disk. This geometric construction reveals the simple geometry not apparent from the explicit formula in Theorem 2.16 for the hyperbolic midpoint. Similar constructions for the hyperbolic midpoint can be found in the book [1] by Ahara. At the end of this section, Theorem 5.12 offers an explicit formula for the chordal midpoint of two points in the unit disk.

Lemma 5.1.

If V𝔹2V\subset\mathbb{B}^{2} is a lens-shaped domain symmetric with respect to the real axis bounded by two circular arcs with endpoints 1-1 and 11, and a,bVa,b\in\partial V so that Imb<0<Ima{\rm Im}\,b<0<{\rm Im}\,a, then the hyperbolic midpoint of aa and bb with respect to the domain 𝔹2\mathbb{B}^{2} is on the real axis.

Proof.

Let kk be the intersection point of the hyperbolic line J[a,b]J^{*}[a,b] and the real axis. Trivially, if k=0k=0, then J[a,b]J^{*}[a,b] is a diameter of the unit disk 𝔹2\mathbb{B}^{2} and, by the symmetry of the domain VV, a=ba=-b and the hyperbolic midpoint is the origin. Let us next assume that k0k\neq 0. Now, the line J[a,b]J^{*}[a,b] is the arc of the circle that contains a,ba,b and is orthogonal to the unit circle S1S^{1}. Consider the Möbius transformation Tk:¯¯T_{k}:\overline{\mathbb{C}}\to\overline{\mathbb{C}}, defined as in (2.9). Clearly, Tk(k)=0T_{k}(k)=0, Tk(1)=1T_{k}(1)=1, and Tk(1)=1T_{k}(-1)=-1, and it also follows that the mapping preserves the unit disk 𝔹2\mathbb{B}^{2}, the lens-shaped domain VV, and its boundary V\partial V. As Tk(k)=0T_{k}(k)=0 for a point kJ[a,b]k\in J^{*}[a,b], the mapped hyperbolic line is a diameter of 𝔹2\mathbb{B}^{2}. Since the points Tk(a)T_{k}(a) and Tk(b)T_{k}(b) are the intersection points of this diameter and the domain VV, it is clear that Tk(a)=Tk(b)T_{k}(a)=-T_{k}(b) and Tk(k)=0T_{k}(k)=0 is their hyperbolic midpoint. Thus, kk is the hyperbolic midpoint of aa and bb, and it is on the real axis. ∎

aabbkkTk(a)T_{k}(a)Tk(b)T_{k}(b)0
Figure 4. The hyperbolic line J[a,b]J^{*}[a,b] before and after the Möbius transformation TkT_{k} for a=1.1i+2.21e1.9ia=-1.1i+\sqrt{2.21}e^{1.9i}, b=1.1i2.21e1.5ib=1.1i-\sqrt{2.21}e^{1.5i}, and k=J[a,b]k=J^{*}[a,b]\cap\mathbb{R}, and the lens-shaped domain V=B2(1.1i,2.21)B2(1.1i,2.21)V=B^{2}(-1.1i,\sqrt{2.21})\cap B^{2}(1.1i,\sqrt{2.21}).
Theorem 5.2.

Fix a,b𝔹2\{0}a,b\in\mathbb{B}^{2}\backslash\{0\} so that a,ba,b are not collinear with the origin. Let cc be the center of the great circle through aa and b/|b|2b/|b|^{2}, and fix uu so that {u,u}=S1S1(c,|ac|)\{u,-u\}=S^{1}\cap S^{1}(c,|a-c|). The hyperbolic midpoint mm of aa and bb is the intersection point [u,u]S1(v,|av|)[-u,u]\cap S^{1}(v,|a-v|), where vv is the center of the circle through aa, bb, and a/|a|2a/|a|^{2}.

Proof.

The stereographic projections of two great circles passing through a,b/|b|2a,b/|b|^{2} and b,a/|a|2b,a/|a|^{2} are symmetric with respect to the line L(u,u)L(u,-u), so the points aa and bb are on different sides of L(u,u)L(u,-u) on the boundary of a lens-shaped domain B2(c,|cu|)B2(c,|cu|)B^{2}(c,|c-u|)\cap B^{2}(c,|c-u|). The circle S1(v,|av|)S^{1}(v,|a-v|) passing through aa, bb, and a/|a|2a/|a|^{2} is orthogonal to the unit circle so J[a,b]=S1(v,|av|)𝔹2J^{*}[a,b]=S^{1}(v,|a-v|)\cap\mathbb{B}^{2}. Consequently, the hyperbolic midpoint mm must be the intersection point J[a,b][u,u]J^{*}[a,b]\cap[u,-u] and, by rotating all the points around the origin until uu is at 1, we see that this result follows from Lemma 5.1. ∎

Remark 5.3.

The fact that {u,u}=S1S1(c,|ac|)\{u,-u\}=S^{1}\cap S^{1}(c,|a-c|) for a complex point uu in Theorem 5.2 follows from [11, Ex. 3.15(1), p. 33].

Theorem 5.4.

Fix a,b𝔹2\{0}a,b\in\mathbb{B}^{2}\backslash\{0\} so that a,ba,b are not collinear with the origin and |a||b||a|\neq|b|. Let c=LIS[a,b,a,b]c={\rm LIS}[a,b,a_{*},b_{*}], where a,ba_{*},b_{*} are as in (3.2). Then the point m=J[a,b]S1(c,|c|21)m=J^{*}[a,b]\cap S^{1}(c,\sqrt{|c|^{2}-1}) is the hyperbolic midpoint of aa and bb.

Proof.

Clearly, the circle S1(c,|c|21)S^{1}(c,\sqrt{|c|^{2}-1}) is orthogonal to the unit circle S1S^{1} and it passes through mm. Let hh be the inversion in the circle S1(c,|c|21)S^{1}(c,\sqrt{|c|^{2}-1}). Now, h(m)=mh(m)=m, h(a)=bh(a)=b, h(a)=bh(a_{*})=b_{*} as this inversion preserves the unit disk 𝔹2\mathbb{B}^{2} and the angle magnitudes. It follows that

|b,b,m,a|=|h(a),h(a),h(m),h(b)|=|a,a,m,b|.\displaystyle|b_{*},b,m,a_{*}|=|h(a_{*}),h(a),h(m),h(b_{*})|=|a_{*},a,m,b_{*}|.

Thus, mm is the hyperbolic midpoint of aa and bb by [11, (4.9)] or by (2.15). ∎

aabbaa_{*}bb_{*}ccmm0
Figure 5. The hyperbolic midpoint mm of a=0.5e0.6ia=0.5e^{0.6i} and b=0.7e6ib=0.7e^{6i} in the unit disk, the hyperbolic line J[a,b]J^{*}[a,b] with end points aa_{*} and bb_{*}, and an arc of the circle S1(c,|c|21)S^{1}(c,\sqrt{|c|^{2}-1}), where cc is the intersection point of Euclidean lines L(a,b)L(a,b) and L(a,b)L(a_{*},b_{*}).
Remark 5.5.

In Theorem 5.4, the hyperbolic line J[a,b]J^{*}[a,b] is orthogonal to the circle S1(c,|c|21)S^{1}(c,\sqrt{|c|^{2}-1}) because of the choice of cc.

aabbccddffggmmhhjjkkll0
Figure 6. The intersection points of Lemma 5.7, Corollary 5.9, and Conjecture 5.10 for a=e0.1ia=e^{-0.1i}, b=e0.5ib=e^{0.5i}, c=e1.5ic=e^{1.5i}, d=e3.3id=e^{3.3i}, and h=b+0.447(cb)h=b+0.447(c-b).
Theorem 5.6.

[21] Let a,b,c,dS1a,b,c,d\in S^{1} be points listed in the order they occur when one traverses the unit circle in the positive direction.

(1) Let

w1=LIS[a,b,c,d],w2=LIS[a,c,b,d],w3=LIS[a,d,b,c].w_{1}={\rm LIS}[a,b,c,d],\quad w_{2}={\rm LIS}[a,c,b,d],\quad w_{3}={\rm LIS}[a,d,b,c]\,.

Then the point w2w_{2} is the orthocenter of the triangle with vertices at the points 0, w1w_{1}, w3.w_{3}.

(2) The point of intersection of the hyperbolic lines J[a,c]J^{*}[a,c] and J[b,d]J^{*}[b,d] is given by

w=(acbd)±(ab)(bc)(cd)(da)ab+cd,w=\frac{(ac-bd)\pm\sqrt{(a-b)(b-c)(c-d)(d-a)}}{a-b+c-d}\,,

where the sign ”++” or ”-” in front of the square root is chosen such that |w|<1.|w|<1\,.

Lemma 5.7.

Fix four complex points a,b,c,da,b,c,d on the unit circle S1S^{1} in this order. Let ff be the intersection point of the Euclidean lines L(a,c)L(a,c) and L(b,d)L(b,d), and mm the intersection point of the hyperbolic lines J[a,c]J^{*}[a,c] and J[b,d]J^{*}[b,d]. If f0f\neq 0, then ff and mm are collinear with the origin.

Proof.

The points mm and ff are collinear with the origin, if and only if m/f\{0}m/f\in\mathbb{R}\backslash\{0\} or, equivalently, mf¯\{0}m\overline{f}\in\mathbb{R}\backslash\{0\}. Here, m=0m=0 or f¯=0\overline{f}=0 is possible only in the special case f=m=0f=m=0 and, since f0f\neq 0, we only need to show mf¯m\overline{f}\in\mathbb{R}. Theorem 5.6(2) gives an explicit formula for mm and the complex conjugate of ff is as in Proposition 2.6. By using these formulas, we will have

(5.8) mf¯=1±(ab)(bc)(cd)(da)acbd.\displaystyle m\overline{f}=1\pm\frac{\sqrt{(a-b)(b-c)(c-d)(d-a)}}{ac-bd}.

The expression under the square root can be written as

(ab)(bc)(cd)(da)=(ac+bdadbc)(ac+bdabcd)\displaystyle(a-b)(b-c)(c-d)(d-a)=(ac+bd-ad-bc)(ac+bd-ab-cd)
=(ac+bd)2(ac+bd)(ab+cd)(ac+bd)(ad+bc)+(ab+cd)(ad+bc).\displaystyle=(ac+bd)^{2}-(ac+bd)(ab+cd)-(ac+bd)(ad+bc)+(ab+cd)(ad+bc).

Hence, the quotient in (5.8) is

(ac+bdacbd)2(acbd)(ab+cd)(acbd)2(acbd)(ad+bc)(acbd)2+(ab+cd)(ad+bc)(acbd)2\displaystyle\sqrt{\left(\frac{ac+bd}{ac-bd}\right)^{2}-\frac{(ac-bd)(ab+cd)}{(ac-bd)^{2}}-\frac{(ac-bd)(ad+bc)}{(ac-bd)^{2}}+\frac{(ab+cd)(ad+bc)}{(ac-bd)^{2}}}

Because zz¯=|z|2=1z\overline{z}=|z|^{2}=1 for all zS1z\in S^{1} and yy¯iy-\overline{y}\in i\mathbb{R} for all yiy\in i\mathbb{R}, we will have

ac+bdacbd\displaystyle\frac{ac+bd}{ac-bd} =(ac+bd)(acbd)¯|acbd|2=ac¯bdacbd¯|acbd|2i,\displaystyle=\frac{(ac+bd)\overline{(ac-bd)}}{|ac-bd|^{2}}=\frac{\overline{ac}bd-ac\overline{bd}}{|ac-bd|^{2}}\in i\mathbb{R},
ab+cdacbd\displaystyle\frac{ab+cd}{ac-bd} =(ab+cd)(acbd)¯|acbd|2=a¯dad¯+bc¯bc¯|acbd|2i,\displaystyle=\frac{(ab+cd)\overline{(ac-bd)}}{|ac-bd|^{2}}=\frac{\overline{a}d-a\overline{d}+b\overline{c}-b\overline{c}}{|ac-bd|^{2}}\in i\mathbb{R},
ad+bcacbd\displaystyle\frac{ad+bc}{ac-bd} =(ad+bc)(acbd)¯|acbd|2=a¯bab¯+c¯dcd¯|acbd|2i.\displaystyle=\frac{(ad+bc)\overline{(ac-bd)}}{|ac-bd|^{2}}=\frac{\overline{a}b-a\overline{b}+\overline{c}d-c\overline{d}}{|ac-bd|^{2}}\in i\mathbb{R}.

Consequently, it follows that the quotient in (5.8) consists of such products of imaginary numbers that are all real numbers and therefore mf¯m\overline{f} is also a real number. ∎

Corollary 5.9.

If a,b,c,da,b,c,d are four complex points on the unit circle S1S^{1} in this order so that the intersection point ff of the Euclidean lines L(a,c)L(a,c) and L(b,d)L(b,d) is not the origin, then the intersection point mm of the hyperbolic lines J[a,c]J^{*}[a,c] and J[b,d]J^{*}[b,d] is the hyperbolic midpoint of the origin and the point ff.

Proof.

Since f0f\neq 0, the origin cannot be on both of the lines L(a,c)L(a,c) and L(b,d)L(b,d), which means that at least one of the points pairs a,ca,c and b,db,d are non-collinear with the origin. By symmetry, we can suppose that a,ca,c are non-collinear with the origin. By Lemma 5.7, the points ff and mm are collinear with the origin and the inequality |m|<|f||m|<|f| must hold because J[a,c]J^{*}[a,c] is an arc of a circle orthogonal to the unit circle S1S^{1}. Consequently, m=[0,f]J[a,c]m=[0,f]\cap J^{*}[a,c], where the point ff trivially fulfills f[a,c]𝔹2f\in[a,c]\cap\mathbb{B}^{2}. The corollary follows from [18, Prop. 3.1(1), p. 447]. ∎

Conjecture 5.10.

Let a,b,c,da,b,c,d be four complex points on the unit circle S1S^{1} in this order so that L(a,b)L(a,b) and L(c,d)L(c,d) are not parallel. Let hh be an arbitrary point on the Euclidean segment [b,c][b,c], and fix then g=LIS[a,b,c,d]g={\rm LIS}[a,b,c,d], j=LIS[g,h,a,c]j={\rm LIS}[g,h,a,c], k=LIS[g,h,b,d]k={\rm LIS}[g,h,b,d], and l=LIS[g,h,a,d]l={\rm LIS}[g,h,a,d]. Note that the special case j=kj=k is possible. Now, ρ𝔹2(h,j)=ρ𝔹2(k,l)\rho_{\mathbb{B}^{2}}(h,j)=\rho_{\mathbb{B}^{2}}(k,l). See Figure 6.

Remark 5.11.

To prove Conjecture 5.10, it might be useful to consider the Möbius transformation TgT_{g^{*}} from (2.9), where g=1/g¯g^{*}=1/\overline{g}. It preserves the unit disk and circle, but it maps gg to the infinity. Numerical tests suggest that |Tg(h)|=|Tg(l)||T_{g^{*}}(h)|=|T_{g^{*}}(l)| and |Tg(j)|=|Tg(k)||T_{g^{*}}(j)|=|T_{g^{*}}(k)| and, since the mapped points Tg(h),Tg(j),Tg(k),Tg(l)T_{g^{*}}(h),T_{g^{*}}(j),T_{g^{*}}(k),T_{g^{*}}(l) are collinear, this would be enough to prove that ρ𝔹2(Tg(h),Tg(j))=ρ𝔹2(Tg(k),Tg(l))\rho_{\mathbb{B}^{2}}(T_{g^{*}}(h),T_{g^{*}}(j))=\rho_{\mathbb{B}^{2}}(T_{g^{*}}(k),T_{g^{*}}(l)), from which the result follows because of the conformal invariance of the hyperbolic metric.


Refer to caption
Figure 7. Two points a,ba,b in the unit disk, their chordal midpoint mm, and the stereographic projection of the great circle passing through a,b,ma,b,m on the complex plane with the Riemann sphere. This figure is a courtesy of Heikki Ruskeepää [17].

Theorem 5.12.

Let points aa and bb be points on \mathbb{C} and assume that the corresponding π(a)\pi(a) and π(b)\pi(b) are not symmetric with respect to the center (0,0,12)(0,0,\frac{1}{2}). For a,ba,b, the chordal midpoint mm is given by

m=a(1+|b|2)+b(1+|a|2)|1+ab¯|(1+|a|2)(1+|b|2)|ab|2+1.m=\frac{a(1+|b|^{2})+b(1+|a|^{2})}{|1+a\overline{b}|\sqrt{(1+|a|^{2})(1+|b|^{2})}-|ab|^{2}+1}.

Moreover, the stereographic projection of the great circle passing through π(a)\pi(a) and π(b)\pi(b) is given by

|za(1|b|2)b(1|a|2)ba¯ab¯|=|ab||1+ab¯||ab¯a¯b|.\bigg{|}z-\frac{a(1-|b|^{2})-b(1-|a|^{2})}{b\overline{a}-a\overline{b}}\bigg{|}=\frac{|a-b||1+a\overline{b}|}{|a\overline{b}-\overline{a}b|}.
Proof.

Let a,ba,b\in\mathbb{C}. Recall from (2.20) that the points on the Riemann sphere π(a),π(b)\pi(a),\pi(b) corresponding to the two points aa and bb are respectively given by

π(a)=(Rea1+|a|2,Ima1+|a|2,|a|21+|a|2),andπ(b)=(Reb1+|b|2,Imb1+|b|2,|b|21+|b|2).\pi(a)=\Big{(}\frac{\mbox{Re}\,a}{1+|a|^{2}},\frac{\mbox{Im}\,a}{1+|a|^{2}},\frac{|a|^{2}}{1+|a|^{2}}\Big{)},\quad\mbox{and}\quad\pi(b)=\Big{(}\frac{\mbox{Re}\,b}{1+|b|^{2}},\frac{\mbox{Im}\,b}{1+|b|^{2}},\frac{|b|^{2}}{1+|b|^{2}}\Big{)}.

The chordal midpoint mm is given by the projection of the midpoint π(m)\pi(m) on the arc(π(a),π(b))\mbox{arc}(\pi(a),\pi(b)) of the circle with center (0,0,12)(0,0,\frac{1}{2}) which passes through π(a)\pi(a) and π(b)\pi(b), where the arc(π(a),π(b))\mbox{arc}(\pi(a),\pi(b)) is chosen to be a smaller of the two. The point π(m)\pi(m) is the point on the line passing through the Euclidean midpoint (π(a)+π(b))/2(\pi(a)+\pi(b))/2 and (0,0,12)(0,0,\frac{1}{2}) whose distance from (0,0,12)(0,0,\frac{1}{2}) is 1/21/2. Therefore, π(m)\pi(m) is given as follows:

(14Rea(1+|b|2)+Reb(1+|a|2)(1+|a|2)(1+|b|2)L,14Ima(1+|b|2)+Imb(1+|a|2)(1+|a|2)(1+|b|2)L,\displaystyle\Big{(}\frac{1}{4}\frac{\mbox{Re}\,a(1+|b|^{2})+\mbox{Re}\,b(1+|a|^{2})}{(1+|a|^{2})(1+|b|^{2})L},\,\frac{1}{4}\frac{\mbox{Im}\,a(1+|b|^{2})+\mbox{Im}\,b(1+|a|^{2})}{(1+|a|^{2})(1+|b|^{2})L},
141+|ab|2(1+|a|2)(1+|b|2)L+12),\displaystyle\frac{1}{4}\frac{1+|ab|^{2}}{(1+|a|^{2})(1+|b|^{2})L}+\frac{1}{2}\Big{)},

where L2=14(1+ab¯)(1+a¯b)(1+|a|2)(1+|b|2)L^{2}=\dfrac{1}{4}\dfrac{(1+a\overline{b})(1+\overline{a}b)}{(1+|a|^{2})(1+|b|^{2})} and LL is chosen so that π(m)\pi(m) is the point on a smaller arc(π(a),π(b))\mbox{arc}(\pi(a),\pi(b)). So, we can assume L>0L>0 since such π(m)\pi(m) is in the same direction as the Euclidean midpoint (π(a)+π(b))/2(\pi(a)+\pi(b))/2 from the center (0,0,12)(0,0,\frac{1}{2}).

The point on the complex plane corresponding to the above point is the chordal midpoint mm given by

m=a(1+|b|2)+b(1+|a|2)2(1+|a|2)(1+|b|2)L|ab|2+1=a(1+|b|2)+b(1+|a|2)|1+ab¯|(1+|a|2)(1+|b|2)|ab|2+1.m=\frac{a(1+|b|^{2})+b(1+|a|^{2})}{2(1+|a|^{2})(1+|b|^{2})L-|ab|^{2}+1}=\frac{a(1+|b|^{2})+b(1+|a|^{2})}{|1+a\overline{b}|\sqrt{(1+|a|^{2})(1+|b|^{2})}-|ab|^{2}+1}.

To prove the second part of the theorem, note that the equation of the plane {PL=0}3\{PL=0\}\subset\mathbb{R}^{3} passing through π(a)\pi(a), π(b)\pi(b), and (0,0,12)(0,0,\frac{1}{2}) is given by

PL=\displaystyle PL= (Ima(1|b|2)+Imb(1|a|2))ξ+(Rea(1|b|2)Reb(1|a|2))η\displaystyle\big{(}-\mbox{Im}\,{a}(1-|b|^{2})+\mbox{Im}\,{b}(1-|a|^{2})\big{)}\xi+\big{(}\mbox{Re}\,{a}(1-|b|^{2})-\mbox{Re}\,{b}(1-|a|^{2})\big{)}\eta
+(ImbReaRebIma)(2ζ1)=0.\displaystyle\quad+(\mbox{Im}\,{b}\cdot\mbox{Re}\,a-\mbox{Re}\,{b}\cdot\mbox{Im}\,{a})(2\zeta-1)=0.

The great circle with center (0,0,12)(0,0,\frac{1}{2}) which passes through π(a)\pi(a) and π(b)\pi(b) is given as the intersection of the plane PL=0PL=0 and the sphere ξ2+η2+(ζ12)2=1/4\xi^{2}+\eta^{2}+(\zeta-\frac{1}{2})^{2}=1/4.

Consider the system of equations

(5.13) PL=0,ξ2+η2+(ζ12)2=1/4,Rez=ξ1ζ, and Imz=η1ζ.PL=0,\quad\xi^{2}+\eta^{2}+(\zeta-\frac{1}{2})^{2}=1/4,\quad\mbox{Re}\,z=\frac{\xi}{1-\zeta},\mbox{\quad and \quad}\mbox{Im}\,z=\frac{\eta}{1-\zeta}.

By eliminating ξ,η,ζ\xi,\eta,\zeta from the above equations, we have

(5.14) (ab¯+a¯b)zz¯+(aa¯b¯a¯bb¯+a¯b¯)z+(((a¯+b¯)b1)a+b)z¯+ab¯a¯b=0.(-a\overline{b}+\overline{a}b)z\overline{z}+(a\overline{a}\overline{b}-\overline{a}b\overline{b}+\overline{a}-\overline{b})z+\big{(}\big{(}(-\overline{a}+\overline{b})b-1\big{)}a+b\big{)}\overline{z}+a\overline{b}-\overline{a}b=0.

The equation (5.14) is obtained from the calculation of the Gröbner basis by Risa/Asir the symbolic computation system. This equation can be written as

|za(1|b|2)b(1|a|2)ba¯ab¯|=|ab||1+ab¯||ab¯a¯b|,\bigg{|}z-\frac{a(1-|b|^{2})-b(1-|a|^{2})}{b\overline{a}-a\overline{b}}\bigg{|}=\frac{|a-b||1+a\overline{b}|}{|a\overline{b}-\overline{a}b|},

which gives the equation of the stereographic projection of the intersection PL=0PL=0 and the sphere.

Let us yet prove the last part of the theorem. The equation of the plane {PO=0}3\{PO=0\}\subset\mathbb{R}^{3} orthogonal to the line passing through π(a)\pi(a) and π(b)\pi(b) that passes through π(m)\pi(m) is

PO\displaystyle PO =2(Reb(1+|a|2)Rea(1+|b|2))ξ+2(Imb(1+|a|2)Ima(1+|b|2))η\displaystyle=2\big{(}\mbox{Re}\,b(1+|a|^{2})-\mbox{Re}\,a(1+|b|^{2})\big{)}\xi+2\big{(}\mbox{Im}\,b(1+|a|^{2})-\mbox{Im}\,a(1+|b|^{2})\big{)}\eta
+2(|a|2+|b|2)ζ+|a|2|b|2=0.\displaystyle\qquad+2(-|a|^{2}+|b|^{2})\zeta+|a|^{2}-|b|^{2}=0.

Consider the system of equations

(5.15) PO=0,ξ2+η2+(ζ12)2=1/4,Rez=ξ1ζ, and Imz=η1ζ.PO=0,\quad\xi^{2}+\eta^{2}+(\zeta-\frac{1}{2})^{2}=1/4,\quad\mbox{Re}\,z=\frac{\xi}{1-\zeta},\mbox{\quad and \quad}\mbox{Im}\,z=\frac{\eta}{1-\zeta}.

By eliminating ξ,η,ζ\xi,\eta,\zeta from the above equations, we have

(|a|2+|b|2)zz¯+(b¯(1+|a|2)a¯(1+|b|2))z+(b(1+|a|2)a(1+|b|2))z¯+|a|2|b|2=0.(-|a|^{2}+|b|^{2})z\overline{z}+(\overline{b}(1+|a|^{2})-\overline{a}(1+|b|^{2}))z+(b(1+|a|^{2})-a(1+|b|^{2}))\overline{z}+|a|^{2}-|b|^{2}=0.

This equation can be written as

|zb(1+|a|2)a(1+|b|2)|a|2|b|2|=|ab|(1+|a|2)(1+|b|2)||a|2|b|2|,\bigg{|}z-\frac{b(1+|a|^{2})-a(1+|b|^{2})}{|a|^{2}-|b|^{2}}\bigg{|}=\frac{|a-b|\sqrt{(1+|a|^{2})(1+|b|^{2})}}{\big{|}|a|^{2}-|b|^{2}\big{|}},

and it gives the equation of the stereographic projection of the intersection PO=0PO=0 and the sphere. ∎

References

  • [1] K. Ahara, Introduction to Hyperbolic Geometry with GeoGebra (In Japanese) Kyoritsu Shuppan Co., Ltd. 2016
  • [2] L.V. Ahlfors, Möbius transformations in several dimensions. Ordway Professorship Lectures in Mathematics. University of Minnesota, School of Mathematics. 1981
  • [3] G.D. Anderson, M.K. Vamanamurthy, and M. Vuorinen, Conformal Invariants, Inequalities, and Quasiconformal Maps. John Wiley & Sons 1997
  • [4] A.F. Beardon, The Geometry of Discrete Groups, Graduate Texts in Math., Vol. 91 Springer-Verlag. 1983
  • [5] M. Berger, Geometry I,II. Springer-Verlag. 1987
  • [6] D.A. Cox, J. Little, and D. O’Shea Ideals, varieties, and algorithms. Undergraduate Texts in Mathematics. 4th Ed. An introduction to computational algebraic geometry and commutative algebra Springer 2015
  • [7] D. Fraivert, New applications of method of complex numbers in the geometry of cyclic quadrilaterals. International journal of Geometry 7, (2018) 1, pp. 5–16.
  • [8] F.W. Gehring and K. Hag, The ubiquitous quasidisk. With contributions by Ole Jacob Broch. Mathematical Surveys and Monographs, 184. American Mathematical Society, Providence, RI. 2012
  • [9] J. Gray, Worlds out of nothing. Springer Undergraduate Mathematics Series, 2nd Ed. Springer-Verlag, 2011
  • [10] M.J. Greenberg, Euclidean and non-Euclidean geometries. Development and history. 4th ed. W.H. Freeman and Company, 2008
  • [11] P. Hariri, R. Klén and M. Vuorinen, Conformally Invariant Metrics and Quasiconformal Mappings. Springer, 2020
  • [12] A. Horvath, Hyperbolic plane geometry revisited. J. Geom., 106, 2015, 341–362
  • [13] S. Janson, Euclidean, spherical and hyperbolic trigonometry. Manuscript, 2015
  • [14] M. Noro, A computer algebra system Risa/Asir. http://www.math.kobe-u.ac.jp/Asir/asir.html
  • [15] V.V. Prasolov and V.M. Tikhomirov, Geometry, vol. 200 of Translations of Mathematical Monographs. Translated from the 1997 Russian original by O. V. Sipacheva. American Mathematical Society, Providence, RI. 2001
  • [16] J.G. Ratcliffe, Foundations of hyperbolic manifolds. 3rd Ed. Graduate Texts in Mathematics, 149. Springer, 2019
  • [17] H. Ruskeepää, Mathematica navigator. Mathematics, statistics and graphics. With CD-ROM. 3rd Ed. Elsevier/Academic Press, 2009
  • [18] M. Vuorinen and G. Wang, Hyperbolic Lambert quadrilaterals and quasiconformal maps Ann. Acad. Sci. Fenn. Math., 38, 2013, 433–453
  • [19] M. Vuorinen and G. Wang, Bisection of geodesic segments in hyperbolic geometry Complex Analysis and Dynamical Systems V, Contemp. Math., Israel Math. Conf. Proc., Amer. Math. Soc., Providence, RI. 591, 2013, 273–290
  • [20] G. Wang and M. Vuorinen, The visual angle metric and quasiregular maps. Proc. Amer. Math. Soc. 144, 2016, 4899–4912
  • [21] G. Wang, M. Vuorinen, and X. Zhang, On cyclic quadrilaterals in Euclidean and hyperbolic geometries. Publ. Math. Debrecen 99/1-2, 2021, 123–140

6. Appendix: Computer algebra and Gröbner bases with Risa/Asir

The proofs in Sections 3-5 require finding the points of intersection of circles and lines in a form as simple as possible. Hence we have a system of polynomial equations which we want to solve exactly. Manual computations are often very difficult due to complicated formulas. Therefore we use the Gröbner base method [6] from computer algebra as a tool and combine it with manual processing. We will here outline our procedure.

6.1.

Gröbner bases and Risa/Asir

Our procedure using the Gröbner bases has usually the following steps

  1. (1)

    Setting up the polynomial equations f1=f2==fn=0f_{1}=f_{2}=\cdots=f_{n}=0 and defining the ideal I=f1,f2,,fnI=\left<f_{1},f_{2},\cdots,f_{n}\right>

  2. (2)

    Set variable ordering

  3. (3)

    Choice of the monomial ordering (The lexicographic ordering is the most convenient for solving polynomial equations)

  4. (4)

    Finding the Gröbner basis GG for the ideal II

  5. (5)

    Choose the elimination ideal from GG

  6. (6)

    Manual postprocessing

In this appendix, we show how we used the symbolic computation system Risa/Asir [14] to find equation (5.14). Similar calculations could be performed also by using Mathematica, Maple, or some other system.

Let z.re, z.im, and zb denote the real, imaginary, and complex conjugate of z respectively. Then z = z.re + i*z.im represents a point on \mathbb{C}, Setting ξ=\xi=xx, η=\eta=yy, ζ=\zeta=zz, the system of equation (5.13) can be expressed in Risa/Asir as follows. Below, ”ord” is a command that specifies the order of variables in the output polynomial and ”nm” is a command that returns a numerator.

[2062] ord([z,zb,z.re,z.im])$
[2063] PL=(b.im*(1-a*ab)-a.im*(1-b*bb))*xx
        +(a.re*(1-b*bb)-b.re*(1-a*ab))*yy
        +(2*zz-1)*(b.im*a.re-b.re*a.im)$
[2064] RS=xx^2+yy^2+(zz-1/2)^2-1/4$
[2065] Z.xx=nm(xx/(1-zz)-z.re)$
[2066] Z.yy=nm(yy/(1-zz)-z.im)$

Above, [20**] are input prompts.

To eliminate xx, yy, and zz from the system of equation, we use the following method.

Let I be the ideal generated by polynomials PL, RS, Z.xx, Z.yy. We can compute the Gröbner basis for the ideal I by using the following block order

[xx,yy,zz] > [a.re,a.im,b.re,b.im, a,ab,b,bb,z.re,z.im].\mbox{\tt[xx,yy,zz] > [a.re,a.im,b.re,b.im, a,ab,b,bb,z.re,z.im]}.

by

[2067] G=nd_gr([PL,RS,Z.xx,Z.yy],
        [xx,yy,zz, a.re,a.im,b.re,b.im, a,ab,b,bb,z.re,z.im],
        0,[[0,3],[0,10]])$

Then, we need to choose the polynomials that belong to the polynomial ring

[a.re,a.im,b.re,b.im, a,ab,b,bb,z.re,z.im]\mathbb{C}[\mbox{\tt a.re,a.im,b.re,b.im, a,ab,b,bb,z.re,z.im}]

from the elements of the Gröbner basis G.

[2068] length(G);
12
[2069] vars(G[0]);
[a,b,b.im,ab,a.im,bb,a.re,b.re,z.re,z.im]
[2070] vars(G[1]);
[b.im,a.im,a.re,b.re,zz,z.re,z.im]

From the above calculation, we can see that the Gröbner basis G is generated by 12 polynomials and that the first polynomial G[0] in the list of elements is the required one. (The second G[1] and subsequent polynomials in the list are polynomials containing variables to be eliminated such as zz.) We can obtain the desired elimination ideal <G[0]>.

We then extract the required factor from G[0].

[2071] fctr(G[0]);
[[1,1],[a.re*b.im-b.re*a.im,1],
 [(a.re*b.im-b.re*a.im)*z.re^2+(-ab*b.im*a+bb*a.im*b+b.im-a.im)*z.re
 +(a.re*b.im-b.re*a.im)*z.im^2+(b.re*ab*a-a.re*bb*b+a.re-b.re)*z.im
 -a.re*b.im+b.re*a.im,1]]

From the assumption, the points aa, bb and 0 are not collinear, so a.re*b.im-b.re*a.im =Re(a)Im(b)Re(b)Im(a)0=\mbox{Re}(a)\mbox{Im}(b)-\mbox{Re}(b)\mbox{Im}(a)\neq 0. Therefore, the second factor is zero. As the second factor forms the equation of a circle on 2\mathbb{R}^{2}, we need to rewrite it as the equation on \mathbb{C}, as follows.

[2072] Circ=car(@2071[2]);
(a.re*b.im-b.re*a.im)*z.re^2+(-ab*b.im*a+bb*a.im*b+b.im-a.im)*z.re
 +(a.re*b.im-b.re*a.im)*z.im^2+(b.re*ab*a-a.re*bb*b+a.re-b.re)*z.im
 -a.re*b.im+b.re*a.im
[2073] GCircAB=2*@i*subst(Circ,a.re,(a+ab)/2,b.re,(b+bb)/2,
    a.im,(a-ab)/(2*@i),b.im,(b-bb)/(2*@i),z.re,
    (z+zb)/2,z.im,(z-zb)/(2*@i));
((-bb*a+ab*b)*zb+bb*ab*a-bb*ab*b+ab-bb)*z+(((-ab+bb)*b-1)*a+b)*zb
 +bb*a-ab*b

We have now obtained the equation (5.14).


Note that the equation F(z;a,b,c,d)=0F(z;a,b,c,d)=0 that determines the GCIS[a,b,c,d]\mbox{GCIS}[a,b,c,d] is given by eliminating zb from GCircAB and GCircCD, where

   GCircCD=((-c*db+cb*d)*zb+(cb*c-cb*d-1)*db+cb)*z
            +(d*c*db+(-cb*d-1)*c+d)*zb+c*db-cb*d.

In general, the solution to the equation that eliminates zb=z¯\mbox{\tt zb}=\overline{z} from the equation of two circles may not make sense. For example, for two circles |z2|=1|z-2|=1 and |zi|=1|z-i|=1, eliminating z¯\overline{z} from the general forms

zz¯2z2z¯+3=0andzz¯+iziz¯=0z\overline{z}-2z-2\overline{z}+3=0\quad\mbox{and}\quad z\overline{z}+iz-i\overline{z}=0

gives the equation

(2+i)z2(3+4i)z+3i=0.(2+i)z^{2}-(3+4i)z+3i=0.

But, clearly, the solution to this equation satisfies neither |z2|=1|z-2|=1 nor |zi|=1|z-i|=1. This happens because these two circles do not intersect.

Now, we return to the topic of circles on the Riemann sphere. Two great circles on the Riemann sphere have exactly two intersection points unless they coincide. Thus, the two solutions of F(z;a,b,c,d)=0F(z;a,b,c,d)=0 are guaranteed to give the intersection points of the two great circles as long as a,b,c,da,b,c,d are not on the same great circle.