C OMPOSITIO M ATHEMATICA
H ANS -C HRISTOPH I M H OF
Ellipsoids and hyperboloids with infinite foci
Compositio Mathematica, tome 52, n
o2 (1984), p. 231-244
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231
ELLIPSOIDS AND HYPERBOLOIDS WITH INFINITE FOCI
Hans-Christoph
Im Hof© 1984 Martinus Nijhoff Publishers, The Hague. Printed in The Netherlands
Introduction
In an earlier paper it was shown that the
family
ofhorospheres through
two
points
of asimply
connectedcomplete
riemannian manifold ofnonpositive
curvature ishomeomorphic
to asphere (Im
Hof[5]).
Thisresult was obtained
by investigating
the families of confocalellipsoids
and confocal
hyperboloids
withrespect
to twogiven points
as foci.Here we will
investigate
two families ofhypersurfaces,
called tubes andslices,
which can be viewed asellipsoids
andhyperboloids
withrespect
totwo infinite
points
as foci. Oursetting
will be asimply
connectedcomplete
riemannian manifold of dimension n and sectional curvature bounded from aboveby
anegative
constant.Fixing
two infinitepoints, represented by
two Busemannfunctions,
we define tubes and slices as the level sets of the sum and thedifference, respectively,
of the chosen Busemann functions.Here are our main results.
THEOREM 2.4: Tubes are
diffeomorphic
toSn-2
XR;
slices arediffeomor- phic to Rn-1.
COROLLARY 3.10: The set
of infinite points of
a slice ishomeomorphic
toSn 2.
The
proofs
are similar to the ones in[5],
however some modificationsare necessary in order to deal with infinite foci. In the case of finite foci
we used
polar
coordinates around onefocus,
and so we were led toconsider
angles
at this focus. Here it is natural to use "polar
coordinates"around an infinite
focus,
but since at an infinitepoint
there is noangle
measurement we have to
replace angles by
distances onhorospheres.
Inour
arguments
we will makeample
use ofcomparison
theorems for Jacobi fields and fortriangles
with infinite vertices. These theorems allowus to transform exact calculations in the
hyperbolic plane
of constantcurvature into estimates valid for
given
situations in the manifold under consideration. The necessarypreliminaries
are summarized in the firstchapter.
The secondchapter
contains ageneral study
of tubes andslices,
and in the third
chapter
we willinvestigate
the behavior of a slice atinfinity.
At the end we add some remarksconcerning
the case of onefinite and one infinite focus.
The
present
paper answers aquestion
which has itsorigin
in the work of M. Brin and H. Karcher on theergodicity
of the frame flow onnegatively
curved manifolds of even dimensions.Corollary
3.10 wasindependently proved by
P. Eberlein. The paper was conceived at theSonderforschungsbereich
"Theoretische Mathematik" in Bonn and worked out at the IHES in Bures-sur-Yvette withsupport
from theStiftung Volkswagenwerk.
Wegratefully
thank all these institutions for theirhospitality
andsupport.
1. Preliminaries
Infinite points
andhorospheres (cf.
Eberlein-O’Neill[2], § 1-§ 3) Throughout
this paper M denotes an n-dimensionalsimply
connectedcomplete
riemannian manifold of sectional curvature Ksatisfying
K-1. An
infinite point
of M isby
definition a class ofasymptotic geodesic
rays. We will write
y( oo)
= z to indicate that thegeodesic
ray ybelongs
tothe
asymptoticity
class z. The set of infinitepoints
of M is denotedby M(oo),
and M stands forthe union
M UM(oo).
Ourassumptions
on Mimply
that any twopoints of
M canbe joined by
ageodesic unique
up toparametrization.
The set M carries atopology
withrespect
to which it ishomeomorphic
to the closed ballD",
whileM(oo)
ishomeomorphic
tothe
boundary sphere Sn-1.
Let
d( p, q)
denote the distance of twopoints p, q ~
M. The functiona: M M M ~ R defined
by a(p, m, q) = d(m, q) - d(m, p)
has acontinuous extension to M X M X
M,
which isgiven by
theexpression a ( p,
z,q) = f(q) - f(p), where f is
a Busemann function at the infinitepoint
z(Eberlein [1], Proposition 2.6).
Horospheres
with center z EM(~)
areby
definition level sets of Buse-mann functions at z. Since Busemann functions are
C2 (see Proposition
1.2
below), horospheres
areC2 submanifolds,
and so we canspeak
of theinduced metric on a
given horosphere.
Stable Jacobi
fields
A Jacobi field Y
along
ageodesic
y is called stableif ~Y(t)~
is bounded for t 0. From Heintze-Im Hof[4]
wequote
thefollowing
results.PROPOSITION 1.1
([4],
Thm.2.4):
Let Y be a stable Jacobifield along a geodesic
y and assume Y isperpendicular
to. Then ~Y(t)~ ~Y(0)~e-t for
t 0.
PROPOSITION 1.2
(Eberlein, unpublished; [4], Prop. 3.1):
Letf be a Busemann function at
z.Then f is C2, (grad f)(p) = - 03B3(0),
and pUgrad f
= -Y’(0),
where y denotes the unitspeed geodesic
with03B3(0)
= p andy(oo)
= z, and Y denotes the stable Jacobifield along
y withY(O)
v.Infinite triangles
In this section we will compare
triangles
in M withtriangles
in thehyperbolic plane H2
of constant sectional curvature -1. Asimply infinite triangle 0
is determinedby
two vertices p, q E M and one vertexz E
M(~).
Itsparameters
ared(p, q), a(p, z, q ),
and theangles a
and03B2 at p and q, respectively.
Ifa(p,
z,q) = 0,
then à is called isosceles.Let
0394 0
be asimply
infinitetriangle
inH 2
determinedby
its vertices po,qo E H2
andzo E H2(~),
and consider itsrespective parameters
d(p0, q0), a(po,
Zo,q0),
03B10, and03B20.
The relations among these parame- ters aregoverned by hyperbolic trigonometry.
We recall the basic for- mula. Under theassumption
ao =-ul2,
theremaining parameters
ofAo satisfy
the relationsFor
triangles
in M we have thefollowing comparison
theorems.PROPOSITION 1.3: Let à and
Ao
besimply infinite triangles
in M andH2, respectively.
(i) If d(p, q)
=d(po, R’o)
and a = ao, thena( p,
z,q) a(po,
Zo,qo) and 03B2 03B20.
(ii) If d(p, q) = d(po, qo)
anda(p,
z,q) = a(p0,
Zo,qo),
then 03B1 aoand 03B2 03B20.
PROOF: See Heintze-Im Hof
[4], Propositions
4.4 and 4.5.(Observe
thatProposition
4.4 of[4]
contains amisprint.
Theinequalities
for03B2
shouldbe
reversed.)
A
doubly infinite triangle à
is determinedby
one vertex p E M and two vertices x, y EM(~).
Itsparameters
are theangle
a at p and itsdetour,
which we define as follows. We choose Busemann functions
f
at x and g at y, normalized such thatf
+ g = 0 on thegeodesic joining
x and y. Thenwe define
detour(0394)
=f ( p )
+g(p).
For any twosequences {xl}
c Mand {yl}
c Mconverging
to x and y,respectively,
we haveAnother useful
parameter
of à is itsheight,
which is defined to be thelength
of theperpendicular
from the finite vertex to theopposite
side.Let
03940
denote adoubly
infinitetriangle
inH2
with verticespo E H2
and xg, yo EH 2( oc).
Then we have the relationsFor
triangles
in M we have thefollowing comparison
theorems.PROPOSITION 1.4: Let 0 and
03940 be doubly infinite triangles
in M andH2, respectively.
( i ) If height(0394) = height(03940),
thendetour(0394) detour(03940)
and 03B1ao.
(ii) If detour(0394) = detour(03940),
thenheight(0394) height(L1o)
and 03B1ao.
PROOF:
(i)
is an immediate consequence ofProposition
1.3(i) applied
tothe two
rectangular simply
infinitetriangles
obtained from àby drop- ping
theperpendicular
from p to theopposite
side.The first estimate in
(ii)
follows from(i)
and the fact thatdetour(03940)
is monotone
increasing
as a function ofheight(03940).
In order toget
the estimate for a weapproximate A by
finite isoscelestriangles 0394(t).
Let yand ju denote the unit
speed geodesic
rays withy(0) = p(0)
= p,y(oo)
= x, and03BC(~) = y, respectively.
Then we define0394(t)
to be thetriangle
withvertices p,
03B3(t),
and03BC(t).
Wecompare A and 0394 (t)
totriangles 03940
and03940(t)
as follows.By 03940
we denote adoubly
infinitetriangle
inH2
withdetour
(03940)
=detour(à).
Let ao be theangle
of03940
at the finite vertex.By 03940(t)
we denote an isoscelestriangle
inH2
whose sides have the samelength
as those of0394(t).
Let a, be theangle
of03940(t) opposite
to the basis.From the
angle comparison
theorem for finitetriangles, applied
to0394(t) and 03940(t),
weobtain a
at . We claim thatlimt-+ 00 at
= ao. Con-sider the number
d(t) = 2t - d(03B3(t), 03BC(t)).
Itplays
the rôle of a detour in bothtriangles, 0394(t) and 03940(t). By
theapproximation
of àby 0394(t)
wehave
limt~~ d(t)
=detour(à).
Theassumption detour(0394)
=detour(03940)
then
implies limt~~ d(t) = detour(03940),
therefore thetriangles 03940(t) approximate 03940,
thuslimt~~
a, = ao . We concludethat a
03B10.COROLLARY 1.5: Let 0 be a
doubly infinite triangle
inM,
thenThe ball
topology
and thehalf
spacetopology
There are
different
ways ofextending
the manifoldtopology
of M to atopology
on M.Using
theexponential
map at apoint
p E M andpolar
coordinates in the
tangent
spaceTpM,
weget
adiffeomorphism
(Here SpM
denotes the unitsphere
inTp M.)
The mapXp
extends to abijective
mapand by requiring
this map tobe
ahomeomorphism
we induce atopology
on
MB{p},
which extends to M in the obvious way.Equipped
with thistopology
M becomeshomeomorphic
to the closed ball.Although
theconstruction
depends
on the choiceof p E M,
theresulting topology
turns out to be
independent of p (Eberlein-O’Neill [2], § 2).
We will callthis
topology
the balltopology,
in contrast to the half spacetopology
which we define next.
We fix a
point
z EM(~)
andtry
to construct ananalogous map 03BBZ.
Since there is no unit
tangent sphere
at z, we have to use one of thehorospheres
centered at z as a substitute. Choose a Busemann functionf
at z and consider the
horosphere
F =f-1(0).
Let 03C0: M ~ F denote theprojection along geodesic
raysbelonging
to z. Then the map03BBZ:
F X( - ~, + ~) ~ M
is definedby 03BBZ(03C0(m),f(m))=m.
This map is ahomeomorphism (Eberlein-O’Neill [2], Proposition 3.4),
andit has
anobvious extension to a
bijective
map03BBZ: F (- ~, + ~] ~ MB{z}.
Requiring
this map to be ahomeomorphism
we induce atopology
onMB{z},
which extends to atopology
on Mby using
horoballs centered at z(i.e.,
sets of the form{m ~ M; f ( m ) c})
asbasic neighborhoods
ofz. This
topology
is called thehalf
spacetopology
of M. Itdepends
on thechoice of z E
M(~),
and infact,
thispoint plays
aspecial
rôle inM(~).
With
respect
to the half spacetopology, M(oo) decomposes
into theconnected
components M(~)B{z}, homeomorphic to Rn-1,
and thesingleton {z}.
This reflects the basic difference between the unit disc model and the upper halfplane
model forH2.
Later we will use a uniform structure on M which induces the half space
topology.
We choose a Busemann functionf
at z and fix thehorosphere
F =f-1(0).
On F we have the riemannian metric inducedby
the metric of M. Let
dF
denote thecorresponding
distance function on F.We extend
dF
to aquasi-distance
onMB{z} by defining dF(p, q) = dF(03C0(P), 03C0(q)), where 03C0 denotes
the extendedprojection
03C0:MB{z} ~
F.Now two
points p, q E MB{z}
are said to be close ifdF(p, q)
is smalland
the
numbersf(p), f(q)
are close in[- ~, - ~],
and apoint
p ~
MB{z}
is close to zif f(p)
is close to - oo . The use of this uniform structure for the half spacetopology
makes our estimates more trans-parent. However,
we are interested in resultsexpressible
in terms of theball
topology.
The two are relatedby
thefollowing proposition.
PROPOSITION 1.6: On
MB{z}
thehalf
spacetopology
coincides with the balltopology.
PROOF: At finite
points
the twotopologies
coincide with theordinary topology
of M. Theequivalence
at infinitepoints
different from z is settledby
Lemma 1.8 below.DEFINITION 1.7: Let x be a
point
ofM(~)B{z}.
A truncated p-coneneighborhood
of x is a set of the formHere p E
Mand p (m, x )
denotes theangle
at p subtendedby
m and x.A truncated z-cone
neighborhood
of x is a set of the formLEMMA 1.8: Each
TZ(~, r )
contains a suitableTp(03B4, s),
and vice versa.PROOF: Observe that we are free to choose any
point
p ~ M to represent the balltopology.
A convenient choicefor p
is thepoint
where thegeodesic
linethrough x
and z intersects F. Now letTZ(~, r)
begiven.
Lety be a
geodesic
raystarting
at p andincluding
anangle
8 with the axis of7§(e, r).
Let a be theprojection
of y on F. Thenlength(03B1) (1
+cos
03B4)-1 sin 03B4 (Heintze-Im
Hof[4], Corollary 4.8),
hence for 8sufficiently
small we
have Tp(03B4, 0) ~ Tz(~, 0).
After suitable truncation weget
Tp(03B4, s) ~ Tz(~, r).
Conversely,
letTp(~, r)
begiven.
The construction of a suitableTZ(03B4, s)
contained inTp(~, r)
iscompletely analogous
to theproof
ofLemma 2.8 in Eberlein-O’Neill
[2], except
for one modification. State- ment(1)
of[2]
has to bereplaced by
the statement:For s
sufficiently large, f(m) s implies m(p, z) ~/3.
But thisfollows from
Proposition
1.3(i)
andtrigonometry
inH 2.
2. Tubes and slices
From now on we fix two distinct
points x, y E M( oo)
and a unitspeed geodesic
Q with03C3 ( - oo )
= y and03C3(+ oo )
= x.Up
to the choice of03C3(0)
thisgeodesic
isuniquely
determined. Thepoints x and y give
rise to thefollowing
functions.DEFINITION 2.1:
Let f :
M - R and g: M - R denote Busemann func- tions at x and y,respectively,
normalized such thatf( 0(0))
=g(or(0»
= 0.Then we define e =
1 2(f + g)
and h =1 2 (g - f).
The functions e and h are defined and
C2 throughout
M.They give
rise to two families of
hypersurfaces.
DEFINITION 2.2: For t 0 we define the tube
Et
as level sete-1(t);
fors E R we define the slice
H,
as level seth-1(s).
The families{Et; t 0}
and
{HS; s ~ R}
can beregarded
as the families of confocalellipsoids
and
hyperboloids
withrespect
to the twogiven
infinitepoints
x, y as foci.The basic
properties
of e and h are summarized in thefollowing proposition.
PROPOSITION 2.3:
( i )
Thefunction
e assumes its minimal value 0 on the set03C3(R);
outside03C3(R) it
has no criticalpoints.
( ii )
Thefunction
h has no criticalpoints
in M.PROOF:
(i)
If m=,u(s)
for s ~R,
thene(m)
= 0. If m OE03C3(R),
then m anda span a
doubly
infinitetriangle
à ofpositive height.
FromProposition
1.4
(i)
and anargument
inH2
it follows that à haspositive
detour aswell. Since detour
(0394) = 2e(m),
thisimplies e(m)
> 0.Now assume that m is a critical
point for e, i.e., (grad e)(m)
= 0. Sincethe
geodesic joining x and y
isunique
up toparametrization,
thisimplies m ~ 03C3(R).
(ii) Clearly grad
h never vanishes.From
Proposition
2.3 weimmediately
conclude that the setsEt ( t
>0)
and
HS
are(n - l)-dimensional
submanifolds of M. In thefollowing
theorem we determine their differential
types.
THEOREM 2.4: For t > 0 the
submanifolds Et
arediffeomorphic
tosn-2
XR;
for s e R
thesubmanifolds Hs
arediffeomorphic to Rn-1.
PROOF: Assume t > 0. We claim that the
restriction es
of e toHs
is aMorse function on
Hs
with one criticalpoint,
and that the restrictionh
tof h to
Et
has no criticalpoints.
Sincegrad e
andgrad
h arealways perpendicular
to eachother,
we havegrad es
=grad e
onHS
andgrad h
t=
grad
h onEt . Therefore es
hasexactly
one criticalpoint,
viz. thepoint 03C3(s),
which is the minimalpoint
for es, andh has
no criticalpoint
at all.We have to show that
03C3(s)
isnondegenerate.
For v ET03C3(s) Hs
we havewhere ps denotes covariant differentiation on
Hs,
and 03BB ~ Rdepends
onv.
By Proposition
1.2 we havewhere X and Y are Jacobi fields
along
Qsatisfying X(s) = Y(s) = v,
andsuch that X is stable in the direction of
a(+ oo )
and Y is stable in the direction ofJ( - oo ).
Inparticular,
~vgrad e
is normal to Q, hence À = 0.Now
~sv grad es
= 0implies X’( s )
=Y(s),
thus X =Y,
and X is stable in both directions. ThereforeX = 0,
and hence v = 0.Applying
the Morse Lemma to the criticalpoint 03C3(s)
of es, we find that for small t > 0 the sete-1s(t)
isdiffeomorphic
to S" -2.
Since es hasno further critical
points,
the same conclusion holds for all t > 0. Observ-ing
theequality e-1s(t) = h-1t(s) = HS ~ Et,
wefinally
conclude thatHS and Et
arediffeomorphic to Rn-1
andsn - 2 X R, respectively.
3. Behavior at
infinity
In this
chapter
we willinvestigate the behavior
of a slice atinfinity.
Webegin by extending
the function h to M.LEMMA 3.1:
The function h:
M ~ R has a continuousextension
to afunction
h:M ~ R,
where M carries the balltopology
and R denotesR U
{± ~}.
PROOF: In a first
step
we extend h to a continuous function h:MB f x, y}
- R. Let F and G denote the
horospheres f -’ 1(0)
andg - 1(0),
and let 03C0and T denote the
projections
ofMB{x, y}
onto F andG, respectively.
Then for any
point m E
Mwith f(m)
> 0 andg( m )
> 0 we haveFor z E
M(~)B {x, y}
we now defineWe have to show that
{h(ml)}
converges toh(z)
for any sequence{ml}
c Mconverging
to z.Since f(ml)
andg( m, )
tend to + oo, we havef(m,)
>0, g(m,)
> 0 for ilarge.
Therefore2h(m,)
=a(03C0(ml),
ml,T(ml)).
By
thecontinuity
of 77-, rand a,
this in fact tends toa(03C0(z),
z,03C4(z))=
2h(z).
Now we extend h to M
by defining h ( x )
= + oc andh ( y )
oc. Weclaim that this extension is continuous at x and y. Let s be any real number and let G denote the
horosphere g-1 (s
+03B4)
for some 8 > 0. Since h is continuous onG,
there is aneighborhood
U of03C3(s
+8)
inG,
on which h is greaterthan s,
and since h is monotoneincreasing
on allgeodesics emanating from y,
it exceeds s on the whole truncated y-coneneighborhood
determinedby
U. This shows thecontinuity
of h at x.Now we consider the vector field Z =
grad eliigrad e112,
which isdefined on
MB03C3(R).
For eachpoint m
outside03C3(R)
we denoteby
Ilm the maximalintegral
curve of Z with theparametrization
determinedby 03BCm(e(m)) = m.
LEMMA 3.2:
( i )
Whenever03BCm(t)
isdefined,
we havee(03BCm(t))
= t andh(03BCm(t))
=h(m).
(ii )
The domainof
Il m is the interval(0, oc).
(iii )
Theimage of
Ilm is contained inHh(m)’
The
proofs
are as in Im Hof[5].
Observe that in(ii)
we need thecompactness
of the sublevel setsHs ~ { e c}
for s ~ R and c > 0.Now we fix the tube
El,
and for t > 0 we define ~t:E1 ~ M by
~t(m) = 03BCm(t). Obviously
theimage ~t(E1)
is contained inEt .
Thefollowing
lemmaagain
isproved
as in[5].
LEMMA 3.3: For t > 0 the maps (p,:
Ej - Et
arediffeomorphisms satisfying
h o
(p, = h.
We will
study
the limit ofthe family {~t}
for ttending
to 00. For thispurpose we
have
to admit M’ =MB{x, y}
as range for the maps ~t.Observe that on M’ the half space
topology
based at x or y coincides with the balltopology.
PROPOSITION 3.4: The
family of
maps Tt:E1 ~
M’ convergeslocally uniformly
onEl
as t tends to 00 .PROOF: For any c > 0 we
introduce
thecompact
setsM(c) = {m ~ M;
|h(m)| c}
andE, (c) = El
~M(c).
Our claim will beproved by
show-ing
that for all c > 0 the restricted maps (p,:E1(c) ~ M(c)
convergeuniformly
onEl ( c)
as t tends to 00 . In order to check thisconvergence
we will estimate
expressions
of theform f(03BCm(t))
anddF(03BCm(t), it
where F is a suitable
horosphere
centered at x.1.
Step : Since Ilm(t) E Et,
we havefor all
m ~ E1(c).
Thereforef(03BCm(t))
tends to oc with t,uniformly
inEl(c).
2.
Step:
We fix apoint
m EEl(c).
For shortness we willwrite it =
ILm’Let F denote the
horosphere J-’(- c)
and 7r theprojection
ofMB{x}
onto F. Consider the curve 03B1 = 03C0 ° IL:
(0, oo )
- F. ThendF(03BC(t), IL( t’))
=
dF(03B1(t), 03B1(t’)),
hence3.
Step :
We willestimate lIali by using comparison theory.
Fix t > 0 and consider thedifferential 03C0 *: T03BC(t)M~ T03B1(t)F.
This mapdecomposes
intothe linear
projection
p :T03BC(t)M~ T03BC(t)Ft
and the map03C0*|T03BC(t)Ft: T03BC(t)Ft
~
T03B1(t)F.
HereF
denotes thehorosphere through 03BC(t)
with center x.Now look at the
doubly
infinitetriangle spanned by
o and03BC(t),
anddenote
by
2(A) theangle
at03BC(t). By Proposition
1.2 this is also theangle
subtended
by grad f
andgrad g
at03BC(t). Therefore ~(grad e)(03BC(t))~ =
cos 03C9,
hence ~(t)~
=(cos 03C9)-1,
andso ~03C1((t))~ = ~(t)~
sin 03C9 = tan w.Corollary
1.5implies
sin 03C9e - t,
thusThe effect of
03C0* |T03BC(t)Ft is expressed
in terms of Jacobi fields. Let Y be the stable Jacobi fieldalong
thegeodesic
from03BC(t)
to x with initial valueY(O)
=p(ft(t». By
Lemma 3.2(i), f(03BC(t))
=e(03BC(t)) - h(03BC(t))
= t -h(m),
hence
à(t)
=Y( t - h(m)
+c),
andProposition
1.1implies
Using (3)
andobserving that |h(m)|
c we obtain4.
Step : Integrating (4)
andobserving (2)
weget dF(03BC(t), 03BC(t’))
1 -(1
-
e-2t)1/2
for t’ > t >0,
hencefor
t’ > t, t sufficiently large,
andm ~ E1(c). (Recall
03BC = 03BCm and F =f-1(- c).)
From(1)
and(5)
we conclude thatlimt~~ JLm(t)
exists inM(c), uniformly
for m ~E1(c).
DEFINITION 3.5: We define
03BCm(~) = limt~~ 03BCm(t)
and~(m) = limt~~ ~t(m) = 03BCm(~)
for m EEl’
Obviously ~(m) ~ M(~).
Our next aim is to showthat ~
is ahomeomorphism
ofEl
ontoM’(~) = M(~)B {x, y}.
We start with twolemmata which are used to prove
that ~
isinjective.
LEMMA 3.6: Fix
m E El
and lety be
thegeodesic joining
x to JL m(~).
Thend(03BCm(t), 03B3) 1 for t > 0.
PROOF: Assume
h ( m )
= s and fix t > 0. Let F be thehorosphere through 03BCm(t)
centered at x, andconsider
the curve a = ’TT 003BCm |[t, ~],
where qr denotes theprojection
ofMB{x}
onto F. Thena( (0)
is apoint
of y, andhence
d(03BCm(t), 03B3) length( a ).
As in the
proof
ofProposition
3.4 weestimate Ilâll by comparison theory,
andby integration
we obtainLEMMA 3.7: Fix two
points
ml, m 2 EEl
withh(m1)
=h(m2)
and consider Mi = itnr for
i =1,
2. Thend(MI (t), 03BC2(t))
2 t - kfor
t 1 and a suitableconstant
kdepending
ond(m1, m2)’
PROOF: Let
c(t)
denote the distanced(03BC1(t), 03BC2(t)).
For a fixed t >0,
let03B2: [0, c(t)]
- M be thegeodesic segment
with03B2(0) = 03BC1(t) and 03B2(c(t)) = M2(t),
and write v = -(0)
and V2 =(c(t))
for shortness. We have(cf.
Gromoll et al.
[3],
p.251)
We
begin by estimating
the terms~(grad e)(03BCl(t)), vl~
for i =1, 2. By
definition
The scalar
products
on theright
hand side are cosines of certainangles, they
will be estimatedusing comparison theory.
Consider thetriangle A
formed
by 03BC1(t), 03BC2(t),
and x and denoteby w,
theangle
at03BCl(t).
Observe that à is isosceles
since f (03BC1(t)) = f(03BC2(t)).
NowProposition
1.3(ii)
andhyperbolic trigonometry imply
cos 03C9ltanh(c(t)/2),
henceSimilarly
weget
by considering
thetriangle
formedby ILl (t), 03BC2(t),
and y.Finally
we obtainRecalling
that(grad e)(03BCl(t)) = ~(grad e)(03BCl(t))~2l(t) with 1 grad e~ 1,
and
observing
thattanh(c(t)/2)
ispositive,
we get from(1)
and(2)
We set
a(t) = sinh(c(t)/2).
Thena(1) = sinh(d(m1, m 2 )/2)
anda’(t) a(t). By integration
thisimplies
for t 1.
Using 2a(t) ec(t)/2
and2a(1) d(m,, m2)
weget
and hence our assertion.
After these
preparations
we are able to prove our main result.THEOREM 3.8: The map ~:
E1 ~ M’(~)
is ahomeomorphism satisfying h - 99
= h.PROOF: Since h is continuous the
property
h° (p, = h carries over to ~.Local uniform convergence of the sequence
{~t}
ensuresthat W
iscontinuous. The
injectivity of (p
follows from thepreceding
two lemmataexactly
as in Im Hof[5].
Now we will provethat ~
issurjective.
Wechoose a
point
z EM’( oo ) and a
sequence{rl}
c Mconverging
to z. Fora suitable c > 0 we have z E
M(c)
and(r, 1 c M(c).
Let 03BCl:(0, oo )
~ Mbe the maximal
integral
curve of Zsatisfying 03BCl(tl)
= rifor tl
=e(rl),
andconsider the sequence of
points
m, =03BCl(1)
EEl ( c).
SinceEl ( c)
is com-pact
we may assumethat {ml}
converges to apoint
m EEl (c).
We claim~(w)
= z.Obviously ~(m) ~ M’(~),
so it is sufficient to estimate horo-spherical
distances onF = f-1(-c).
From thetriangle inequality
weget
We fix E > 0 and assert that each of the distances on the
right
hand side is smaller than E as soon as i issufficiently large.
For the first distance we use the convergence off ml}
to m and thecontinuity
of T, for the secondwe use the convergence of
{tl}
to oc and the uniform convergence of{~tl} to T
on the setEl ( c),
and for the third we use the convergence of{ri}
to z.Observing
thatE1(c)
iscompact
andM’(~) Hausdorff,
we concludethat qq restricted to
E1(c)
is ahomeomorphism
onto itsimage. Together
with the fact that the
global
map ~:E1 ~ M’(oo)
isbijective,
thisimplies
(p:
El - M’(~)
is ahomeomorphism.
Our final aim is to determine the set of infinite
points
of asingle
sliceH,.
Apriori
there are different ways to define such a set. We choose the definitionHs(oo)
=( z OE M(~); h(z) = s }. Alternatively,
wemight
formthe closure cl
HS
in M withrespect
to the balltopology
and intersect it withM(oc). However,
we haveLEMMA 3.9:
PROOF: If
z ~ HS(~),
thenz = limt~~03BCm(t)
form = ~-1(z),
hence03BCm(t) ~ Hs.
Thisimplies z ~ cl HS.
IfzEclHsnM(oo),
thenby
thecontinuity
of h on M we haveh ( z )
= s, hence z ~HS(~).
As a consequence of Theorem 3.8 we now
get
COROLLARY 3.10:Hs(~) is homeomorphic
tosn-2.
PROOF: The
homeomorphism
~:Ej - M’(~)
of Theorem 3.8 satisfies ho~ = h,
so it restricts to ahomeomorphism
betweenE1 ~ HS
andHS(~).
In theproof
of Theorem 2.4 we have observed thatEl
~HS
isdiffeomorphic
toS"-2.
This concludes theproof.
Coda
Having
studied the families ofellipsoids
andhyperboloids
withrespect
totwo finite or two infinite
foci,
we are left with the case of one finite andone infinite focus.
Again
there are two families ofhypersurfaces,
the levelsets of the sum and those of the difference of a distance and a Busemann function.
In euclidean space, where
horospheres
coincide withhyperplanes,
weobtain in this way two families of
paraboloids
situatedsymmetrically
with
respect
to the finite focus. In manifolds ofstrictly negative
curvatureboth
types
ofhypersurfaces
are still submanifoldsdiffeomorphic
toeuclidean spaces, but
they
behavedifferently
atinfinity.
Thosehyper-
surfaces which
correspond
toellipsoids
have asingle point
atinfinity,
theinfinite
focus,
the onescorresponding
tohyperboloids
have asphere
atinfinity,
as in the cases described earlier.The
proofs
of these facts are left to the reader.References
[1] P. EBERLEIN: Geodesic flows on negatively curved manifolds. II. Trans. Amer. Math.
Soc. 178 (1973) 57-82.
[2] P. EBERLEIN and B. O’NEILL: Visibility manifolds. Pacific J. Math. 46 (1973) 45-109.
[3] D. GROMOLL, W. KLINGENBERG and W. MEYER: Riemannsche Geometrie im Grossen.
Lecture Notes in Mathematics 55. Berlin, Heidelberg, New York, 1968.
[4] E. HEINTZE and H.C. IM HOF: Geometry of horospheres. J. Differential Geometry 12 (1977) 481-491.
[5] H.C. IM HOF: The family of horospheres through two points. Math. Ann. 240 (1979)
1-11.
(Oblatum 15-VI-1982
& 22-II-1983)
Hans-Christoph Im Hof
Mathematisches Institut der Universitât Basel
Rheinsprung 21
CH-4051 Basel Switzerland