The chordal metric is a metric on the Riemann sphere that is defined with the help of stereographic projection .
definition
The sphere embedded in Euclidean space is denoted by. Now let the inverse image of the stereographic projection by the North Pole with . For two points on the Riemann sphere, the chordal metric is defined by
S.
2
⊂
R.
3
{\ displaystyle \ mathbb {S} ^ {2} \ subset \ mathbb {R} ^ {3}}
R.
3
{\ displaystyle \ mathbb {R} ^ {3}}
P
N
-
1
:
C.
∪
{
∞
}
→
S.
2
{\ displaystyle P_ {N} ^ {- 1} \ colon \ mathbb {C} \ cup \ {\ infty \} \ to \ mathbb {S} ^ {2}}
N
{\ displaystyle N}
P
N
-
1
(
∞
)
=
N
{\ displaystyle P_ {N} ^ {- 1} (\ infty) = N}
z
,
w
∈
C.
∪
{
∞
}
{\ displaystyle z, w \ in \ mathbb {C} \ cup \ {\ infty \}}
χ
{\ displaystyle \ chi}
χ
(
z
,
w
)
: =
‖
P
N
-
1
(
z
)
-
P
N
-
1
(
w
)
‖
2
{\ displaystyle \ chi (z, w): = \ | P_ {N} ^ {- 1} (z) -P_ {N} ^ {- 1} (w) \ | _ {2}}
,
where denotes the Euclidean norm .
‖
⋅
‖
2
{\ displaystyle \ | \ cdot \ | _ {2}}
The representation results explicitly
for points
w
,
z
∈
C.
{\ displaystyle w, z \ in \ mathbb {C}}
χ
(
z
,
w
)
=
‖
P
N
-
1
(
z
)
-
P
N
-
1
(
w
)
‖
2
=
2
⋅
‖
w
-
z
‖
1
+
‖
w
‖
2
1
+
‖
z
‖
2
{\ displaystyle \ chi (z, w) = \ | P_ {N} ^ {- 1} (z) -P_ {N} ^ {- 1} (w) \ | _ {2} = {\ frac {2 \ cdot \ | wz \ |} {{\ sqrt {1+ \ | w \ | ^ {2}}} {\ sqrt {1+ \ | z \ | ^ {2}}}}}}
.
For and can the representation
w
=
∞
{\ displaystyle w = \ infty}
z
∈
C.
{\ displaystyle z \ in \ mathbb {C}}
d
c
(
z
,
∞
)
=
‖
P
N
-
1
(
z
)
-
N
‖
2
=
2
1
+
‖
z
‖
2
{\ displaystyle d_ {c} (z, \ infty) = \ | P_ {N} ^ {- 1} (z) -N \ | _ {2} = {\ frac {2} {\ sqrt {1+ \ | z \ | ^ {2}}}}}
can be determined and applies to
w
=
z
=
∞
{\ displaystyle w = z = \ infty}
χ
(
∞
,
∞
)
=
‖
N
-
N
‖
2
=
0
{\ displaystyle \ chi (\ infty, \ infty) = \ | NN \ | _ {2} = 0}
.
properties
The Riemann number sphere is a compact metric space with regard to the chordal metric. Since the chordal metric and the Euclidean metric are equivalent for any one , properties such as openness or closure of bounded subsets of are identical for the two metrics.
C.
∪
{
∞
}
{\ displaystyle \ mathbb {C} \ cup \ {\ infty \}}
B.
R.
(
0
)
{\ displaystyle B_ {R} (0)}
R.
>
0
{\ displaystyle R> 0}
C.
{\ displaystyle \ mathbb {C}}
generalization
Since there is also a stereographic projection from the - sphere into the one-point compactification of , the above definition can be generalized and one obtains that with regard to this metric there is also a compact metric space.
P
N
:
S.
n
→
R.
n
^
{\ displaystyle P_ {N} \ colon S ^ {n} \ to {\ widehat {\ mathbb {R} ^ {n}}}}
n
{\ displaystyle n}
R.
n
^
{\ displaystyle {\ widehat {\ mathbb {R} ^ {n}}}}
R.
n
{\ displaystyle \ mathbb {R} ^ {n}}
R.
n
^
{\ displaystyle {\ widehat {\ mathbb {R} ^ {n}}}}
Individual evidence
^ Rolf Walter: Introduction to Analysis 1 . Walter de Gruyter 2007, ISBN 9783110195392 , pp. 354-355.
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