12.3: Auxiliary statements
( \newcommand{\kernel}{\mathrm{null}\,}\)
One may compare the conformal model with a telescope — it makes it possible to see the h-plane from the Euclidean plane. Continuing this analogy further, we may say that the following lemma will be used to aim the telescope at any particular point in the h-plane.
Consider an h-plane with a unit circle as the absolute. Let O be the center of the absolute and P be another h-point. Suppose that P′ denotes the inverse of P in the absolute.
Then the circle Γ with the center P′ and radius √1−OP2OP is perpendicular to the absolute. Moreover, O is the inverse of P in Γ.
- Proof
-
Follows from Exercise 10.5.2.
Assume Γ is a circline that is perpendicular to the absolute. Consider the inversion X↦X′ in Γ, or if Γ is a line, set X↦X′ to be the reflection across Γ.
The following observation says that the map X↦X′ respects all the notions introduced in the previous section. Together with the lemma above, it implies that in any problem that is formulated entirely in h-terms we can assume that a given h-point lies in the center of the absolute.
The map X↦X′ described above is a bijection from the h-plane to itself. Moreover, for any h-points P, Q, R such that P≠Q and Q≠R, the following conditions hold:
- The h-line (PQ)h, h-half-line [PQ)h, and h-segment [PQ]h are transformed into (P′Q′)h, [P′Q′)h, and [P′Q′]h respectively.
- δ(P′,Q′)=δ(P,Q) and P′Q′h=PQh.
- ∡hP′Q′R′≡−∡hPQR.
It is instructive to compare this observation with Proposition [prop:reflection].
- Proof
-
According to Theorem 10.5.1, the map sends the absolute to itself. Note that the points on Γ do not move, it follows that points inside of the absolute remain inside after the mapping. Whence the X↦X′ is a bijection from the h-plane to itself.
Part (a) follows from Theorem 10.3.1 and Theorem 10.6.1.
Part (b) follows from Theorem 10.2.1.
Part (c) follows from Theorem 10.6.1.
Assume that the absolute is a unit circle centered at O. Given an h-point P, set x=OP and y=OPh. Then
y=ln1+x1−x and x=ey−1ey+1.
Observe that according to lemma, OPh→∞ as OP→1. That is if P approaches absolute in Euclidean sense, it escapes to infinity in the h-sense.
- Proof
-
Note that the h-line (OP)h forms a diameter of the absolute. If A and B are the ideal points as in the definition of h-distance, then
OA=OB=1,PA=1+x,PB=1−x.
In particular,
y=lnAP⋅BOPB⋅OA=ln1+x1−x.
Taking the exponential function of the left and the right hand side and applying obvious algebra manipulations, we get that
x=ey−1ey+1.
Assume the points P, Q, and R appear on one h-line in the same order. Then
PQh+QRh=PRh.
- Proof
-
Note that
PQh+QRh=PRh
is equivalent to
δ(P,Q)⋅δ(Q,R)=δ(P,R).
Let A and B be the ideal points of (PQ)h. Without loss of generality, we can assume that the points A, P, Q, R, and B appear in the same order on the circline containing (PQ)h. Then
δ(P,Q)⋅δ(Q,R)=AQ⋅BPQB⋅PA⋅AR⋅BQRB⋅QA==AR⋅BPRB⋅PA==δ(P,R).
Hence 12.3.1 follows.
Let P be an h-point and ρ>0. The set of all h-points Q such that PQh=ρ is called an h-circle with the center P and the h-radius ρ.
Any h-circle is a Euclidean circle that lies completely in the h-plane.
More precisely for any h-point P and ρ≥0 there is a ˆρ≥0 and a point ˆP such that
for any h-point Q.
Moreover, if O is the center of the absolute, then
- ˆO=O for any ρ and
- ˆP∈(OP) for any P≠O.
- Proof
-
According to Lemma 12.3.2, OQh\z=ρ if and only if
Therefore, the locus of h-points Q such that OQh=ρ is a Euclidean circle, denote it by Δρ.
If P≠O, then by Lemma 12.3.1 and the main observation (Theorem 12.3.1) there is inversion that respects all h-notions and sends O↦P.
Let Δ′ρ be the inverse of Δρ. Since the inversion preserves the h-distance, PQh=ρ if and only if Q∈Δ′ρ.
According to Theorem 10.3.1, Δ′ρ is a Euclidean circle. Let ˆP and ˆρ denote the Euclidean center and radius of Δ′ρ.
Finally, note that Δ′ρ reflects to itself across (OP); that is, the center ˆP lies on (OP).
Assume P, ˆP, and O are as in the Lemma 12.3.1 and P≠O. Show that ˆP∈[OP].
- Hint
-
Let X and Y denote the point of intersections of (OP) and Δ′rho. Consider an isometry (OP)→R such that O corresponds to 0. Let x,y,p, and ˆp denote the real number corresponding to X,Y,P, and ˆP.
We can assume that p>0 and x<y. Note that ˆp=x+y2 and
(1+x)⋅(1−p)(1−x)⋅(1+p)=(1+p)˙(1−y)(1−p)⋅(1+y).
It remains to show that all this implies 0<ˆp<p.